1. Introduction
Let G be a connected semisimple real algebraic group. Let
$\Gamma \lt G$
be a discrete subgroup. Patterson–Sullivan measures are certain families of Borel measures on a generalized flag variety, supported on the limit set of
$\Gamma$
. They play a crucial role in the study of dynamics on the associated locally symmetric space, especially in the counting and equidistribution of
$\Gamma$
-orbits of various geometric objects. The original construction is due to Patterson and Sullivan for Kleinian groups [Reference PattersonPat76, Reference SullivanSul79], which was generalized by Quint [Reference QuintQui02b] (for earlier works, see [Reference AlbuquerqueAlb99] and [Reference BurgerBur93]).
Sullivan showed that for convex cocompact Kleinian groups of
$\operatorname{{\rm Isom}}^+(\mathbb H_\mathbb R^n)$
, Patterson–Sullivan measures are Ahlfors regular Hausdorff measures on the limit sets in
$\mathbb S^{n-1}$
(see [Reference SullivanSul79, Theorem 8]). Since Patterson–Sullivan measures are constructed from the weighted Dirac measures on an orbit of
$\Gamma$
in the symmetric space
$\mathbb H_\mathbb R^n$
, it is remarkable that they can be given the geometric characterization purely in terms of the internal metric on the limit set of
$\Gamma$
, which is a subset of the boundary
$\partial \mathbb H_\mathbb R^n\simeq \mathbb S^{n-1}$
.
In recent decades, Anosov subgroups have emerged as a higher-rank generalization of convex cocompact Kleinian groups. Therefore it is natural to ask when the Patterson–Sullivan measures of Anosov subgroups arise as Ahlfors regular Hausdorff measures on the limit sets with respect to appropriate metrics. The main goal of this paper is to answer this question.
To state our results, fix a Cartan decomposition
$G=K A^+ K$
, where
$K \lt G$
is a maximal compact subgroup and
$A^+ \subset A$
is a positive Weyl chamber of a maximal real split torus
$A \lt G$
. We denote by X the associated Riemannian symmetric space
$G/K$
. Let
$\mathfrak g$
and
$\mathfrak a$
denote the Lie algebras of G and A, respectively, and set
$\mathfrak a^+=\log A^+$
. Let
$\Pi$
denote the set of all simple roots of
$(\mathfrak g, \mathfrak a)$
with respect to the choice of
$\mathfrak a^+$
.
Fix a non-empty subset
$\theta$
of
$\Pi$
. Let
$P_\theta$
be the standard parabolic subgroup of G associated with
$\theta$
. The quotient space
is called the
$\theta$
-boundary of X, or a generalized flag variety. We denote by
$\Lambda_\theta$
the limit set of
$\Gamma$
in
$\mathcal F_\theta$
(see [Reference BenoistBen97]). For
$\theta=\Pi$
, we omit the subscript
$\theta$
from now on; so, in particular,
$P=P_\Pi$
is a minimal parabolic subgroup of G. Set
$\mathfrak a_\theta=\bigcap_{\alpha\in \Pi-\theta} \operatorname{{\rm ker}}\alpha$
and let
$\mathfrak a_\theta^*$
denote the dual vector space of
$\mathfrak a_\theta$
. We may think of
$\mathfrak a_\theta^*$
as a subspace of
$\mathfrak a^*$
via the canonical projection
$p_\theta: \mathfrak a\to \mathfrak a_\theta$
(2.3). For
$\psi\in \mathfrak a_\theta^*$
, a
$(\Gamma, \psi)$
-Patterson–Sullivan measure is a Borel probability measure
$\nu$
on
$\Lambda_{\theta}$
such that for all
$\gamma \in \Gamma$
and
$\xi \in \Lambda_{\theta}$
,
where
$\beta$
denotes the Busemann map (see (2.8)).
A finitely generated subgroup
$\Gamma\lt G$
is called
$\theta$
-Anosov if there exists a constant
$C \gt 1$
such that for all
$\alpha \in \theta$
,
where
$|\cdot |$
is a word metric on
$\Gamma$
with respect to a fixed finite generating set and
$\mu:G\to \mathfrak a^+$
is the Cartan projection defined by the condition that
$g \in K ( \exp \mu(g)) K$
for all
$g\in G$
. For other equivalent definitions of Anosov subgroups, see [Reference LabourieLab06, Reference Guichard and WienhardGW12, Reference Kapovich, Leeb and PortiKLP17, Reference Kapovich, Leeb and PortiKLP18, Reference Guéritaud, Guichard, Kassel and WienhardGGK+17, Reference Bochi, Potrie and SambarinoBPS19], etc.
In the rest of the introduction, let
$\Gamma$
be a non-elementaryFootnote
1
$\theta$
-Anosov subgroup of G. We impose the non-elementary assumption on Anosov subgroups for the entire paper. The space of all Patterson–Sullivan measures of
$\Gamma$
is parameterized by the set
$\mathscr T_\Gamma\subset \mathfrak a_\theta^*$
of all linear forms tangent to the
$\theta$
-growth indicator
$\psi_\Gamma^\theta$
(Definition 3.1):
More precisely, for any
$\psi\in \mathscr T_\Gamma$
, there exists a unique
$(\Gamma, \psi)$
-Patterson–Sullivan measure
and every Patterson–Sullivan measure of
$\Gamma$
arises in this way (Theorem 3.4). Denote by
$\mathcal L_\theta\subset \mathfrak a_{\theta}^+$
the
$\theta$
-limit cone of
$\Gamma$
, which is the asymptotic cone of
$p_{\theta}(\mu(\Gamma))$
. Then
$\mathscr T_\Gamma$
is in bijection with the set
$\{\psi\in \mathfrak a_\theta^*: \psi\gt 0 \text{on } \mathcal L_\theta-\{0\}\}/\sim$
, where
$\psi_1\sim \psi_2$
if and only if
$\psi_1=c \cdot \psi_2$
for some
$c\gt 0$
. When the limit cone
$\mathcal L_\theta$
has non-empty interior (e.g., when
$\Gamma$
is Zariski dense in G),
$\mathscr T_\Gamma$
is homeomorphic to
$\mathbb R^{\# \theta-1}$
.
1.1 Ahlfors regularity and Hausdorff measures
Anosov subgroups of a rank-one Lie group G are precisely convex cocompact subgroups. In general rank-one groups, the unique Patterson–Sullivan measure of
$\Gamma$
is Ahlfors regular and coincides with the Hausdorff measure on
$\Lambda$
with respect to a K-invariant sub-Riemannian metric on the boundary
$\partial_\infty X $
which is defined in terms of the Gromov product [Reference CorletteCor90, Theorem 5.4]. Except for the case of
$\operatorname{{\rm SO}}(n,1)$
, this sub-Riemannian metric is not a Riemannian metric.
In this paper, we prove an analogous theorem for a general Anosov subgroup. Let
$\psi\in \mathscr T_\Gamma$
. The
$\theta$
-Anosov property of
$\Gamma$
implies that any two distinct points of
$\Lambda_\theta$
are in general position and hence the following defines a premetricFootnote
2
on
$\Lambda_\theta$
: for
$\xi, \eta\in \Lambda_\theta$
,
\begin{equation} d_{\psi}(\xi, \eta) =\begin{cases}e^{-\psi( \mathcal G(\xi, \eta))} & \text{if } \xi \neq \eta,\\ 0 &\text{if } \xi = \eta,\end{cases}\end{equation}
where
$\mathcal G$
is the
$\mathfrak a$
-valued Gromov product (see Definition 2.3). This premetric turns out to be a correct replacement of the sub-Riemannian metric of the rank-one case.
For
$s \gt 0$
, we denote by
$\mathcal H_{\psi}^s$
the s-dimensional Hausdorff measure on
$\Lambda_\theta$
with respect to the premetric
$d_\psi$
, which is a Borel outer measure (9.1). We write
$\mathcal H_\psi$
for
$\mathcal H_\psi^1$
. It turns out that the metric properties of the Patterson–Sullivan measure
$\nu_\psi$
depend on the symmetricity of
$\psi\in \mathfrak a_\theta^*$
:
$\psi$
is called symmetric if
$\psi$
is invariant under the opposition involution i of
$\mathfrak a$
(see (2.2)).
Our main theorem is as follows.
Theorem 1.1.
Let
$\Gamma$
be a non-elementary
$\theta$
-Anosov subgroup of G. Let
$\psi\in \mathscr T_\Gamma$
be a symmetric linear form. Then, the Patterson–Sullivan measure
$\nu_\psi$
is Ahlfors 1-regular and equal to the one-dimensional Hausdorff measure
$\mathcal H_\psi$
, up to a constant multiple.
The Ahlfors 1-regularity of
$\nu_\psi$
means that there exists
$C\ge 1$
such that for any
$\xi\in \Lambda_\theta$
and
$0\le r\lt \operatorname{diameter} (\Lambda_{\theta}, d_\psi)$
,
where
$B_{\psi}(\xi, r)=\{\eta\in \Lambda_{\theta}: d_\psi(\xi, \eta)\lt r\}$
. The premetric space
$(\Lambda_{\theta}, d_{\psi})$
is called Ahlfors s-regular for
$s \gt 0$
if it admits an Ahlfors s-regular Borel measure (see Definition 8.1). Noting that
$\mathcal H_{s \psi}=\mathcal H_\psi^s$
for
$s\gt 0$
, the reason that the Patterson–Sullivan measure is the one-dimensional Hausdorff measure in the above theorem is due to the normalization of
$\psi$
made by the choice that
$\psi$
is a tangent form, i.e.,
$\psi\in \mathscr T_\Gamma$
(see Remark 8.3).
Remark 1.2. If
$\psi$
has gradient in the interior of
$\mathfrak a_{\theta}^+$
, then
$\psi$
can be used to define a Finsler metric on X and Dey and Kapovich [Reference Dey and KapovichDK22, Theorem A] have shown that
$\nu_\psi$
is the Hausdorff measure, without addressing the Ahlfors regularity (see Remark 9.4). Note that Hausdorff measures need not be Ahlfors-regular in general. Our approach in this paper is different; indeed, we first establish the Ahlfors regularity of
$\nu_\psi$
and deduce the rest as a consequence of this.
The opposition involution i of
$\mathfrak a$
is known to be trivial if and only if G does not have a simple factor of type
$A_n$
(
$n\ge 2$
),
$D_{2n+1}$
(
$n\ge 2$
) or
$E_6$
(see [Reference TitsTit66, 1.5.1]). When i is non-trivial, the symmetricity hypothesis on
$\psi$
cannot be removed. In fact, we prove the following (Theorems 9.2 and 9.12, see also Remark 9.8).
Theorem 1.3.
Let
$\Gamma$
be a Zariski dense
$\theta$
-Anosov subgroup of G. For any non-symmetric
$\psi\in \mathscr T_\Gamma$
, the premetric space
$(\Lambda_{\theta}, d_{\psi})$
is Ahlfors s-regular for some
$0\lt s\lt 1$
but the Patterson–Sullivan measure
$\nu_\psi $
is not comparable
Footnote 3
to any
$\mathcal H_\psi^s$
,
$s \gt 0$
.
1.2 Critical exponents and Hausdorff dimensions
Denote by
$\mathcal L_\theta\subset \mathfrak a_{\theta}^+$
the
$\theta$
-limit cone of
$\Gamma$
, which is the asymptotic cone of
$p_{\theta}(\mu(\Gamma))$
. For
$\psi\in \mathfrak a_\theta^*$
which is positive on
$\mathcal L_{\theta}-\{0\}$
, we set
The Hausdorff dimension of
$(\Lambda_{\theta}, d_{\psi})$
is defined as
A natural question is whether
$\dim_\psi \Lambda_\theta$
is equal to
$\delta_\psi$
.
Theorem 1.4.
Let
$\Gamma$
be a non-elementary
$\theta$
-Anosov subgroup of G. For any
$\psi\in \mathfrak a_\theta^*$
which is positive on
$\mathcal L_{\theta}-\{0\}$
, we have
where
$\bar \psi = {\psi + \psi \circ {\rm i}}/{2}$
. In particular, if
$\psi$
is symmetric, then
$\dim_{\psi}\Lambda_{\theta}= \delta_{\psi}$
.
Remark 1.5.
-
– We remark that for
$\psi$
non-symmetric,
$ \dim_{\psi} \Lambda_{\theta}$
is not equal to
$\delta_\psi $
in general (Proposition 9.10). -
– As mentioned above, if
$\psi$
is symmetric and the gradient of
$\psi$
belongs to the interior of
$\mathfrak a_{\theta}^+$
, then Theorem 1.4 is due to Dey and Kapovich [Reference Dey and KapovichDK22, Theorem A(v)]. When G is of rank one, Theorem 1.4 is due to Patterson [Reference PattersonPat76], Sullivan [Reference SullivanSul79], and Corlette [Reference CorletteCor90].
Together with a work of Bridgeman, Canary, Labourie, and Sambarino [Reference Bridgeman, Canary, Labourie and SambarinoBCL+15, Proposition 8.1], Theorem 1.4 implies that for any
$\psi$
non-negative on
$\mathfrak a_\theta^+$
,
$\dim_\psi \Lambda_\theta$
depends real-analytically on
$\theta$
-Anosov representations (Corollary 9.13). We describe one concrete example as follows.
1.3 (p,q)-Hausdorff dimension and Teichmüller space
Let
$\Sigma$
be a torsion-free uniform lattice of
$\operatorname{{\rm PSL}}_2(\mathbb R)$
, and let
$\operatorname{Teich}(\Sigma)$
be the Teichmüller space:
where the equivalence relation is given by conjugations by elements of
$\operatorname{{\rm PGL}}_2(\mathbb R)$
. It is well known that
$\operatorname{Teich}(\Sigma)\simeq \mathbb R^{6g-6}$
, where g is the genus of the surface
$\Sigma \backslash \mathbb H_\mathbb R^2$
. For
$\sigma \in \operatorname{Teich}(\Sigma)$
, denote by
$\Lambda_\sigma\subset \mathbb S^1\times \mathbb S^1$
the limit set of the self-joining subgroup
$(\operatorname{{\rm id}}\times \sigma)(\Sigma)=\{(\gamma,\sigma(\gamma)): \gamma \in \Sigma\}$
, which is well-defined up to conjugations. The Hausdorff dimension of
$\Lambda_\sigma$
with respect to a Riemannian metric on
$\mathbb S^1\times \mathbb S^1$
is equal to 1 for any
$\sigma\in \operatorname{Teich}(\Sigma)$
(see [Reference Kim, Minsky and OhKMO23, Theorem 1.1]). For any pair (p,q) of positive real numbers, consider the premetric on
$\mathbb S^1\times \mathbb S^1$
given by
for any
$\xi=(\xi_1, \xi_2)$
and
$\eta= (\eta_1, \eta_2)$
in
$\mathbb S^1\times \mathbb S^1$
, where
$d_{\mathbb S^1}$
is a Riemannian metric on
$\mathbb S^1$
. For a subset
$S \subset \mathbb S^1 \times \mathbb S^1$
, denote by
$\dim_{p,q} S $
the Hausdorff dimension of S with respect to
$d_{p, q}$
. Note that on the diagonal of
$\mathbb S^1\times \mathbb S^1$
,
$d_{p,q}$
is the
$(p+q)$
th power of
$d_{\mathbb S^1}$
and hence
For each
$\sigma \in \operatorname{Teich}(\Sigma)$
, denote by
$\delta_{p, q}(\sigma)$
the critical exponent of the Poincaré series
$s\mapsto \sum_{\gamma \in \Sigma} e ^{- s(pd_{\mathbb H_\mathbb R^2}(o, \gamma o) + q d_{\mathbb H_\mathbb R^2}(o, \sigma(\gamma) o))}$
.
Corollary 1.6.
Let
$p,q \gt 0$
.
-
(1) For any
$\sigma \in \operatorname{Teich}(\Sigma)$
, we have
$$\dim_{p, q}\Lambda_{\sigma} =\delta_{p,q}(\sigma).$$
-
(2) For any
$\sigma \in \operatorname{Teich}(\Sigma)$
, we have and the equality holds if and only if
$$\dim_{p, q} \Lambda_{\sigma} \le \frac{1}{p + q}$$
$\sigma = \operatorname{{\rm id}}$
.
-
(3) The map
is a real-analytic function on
$$\sigma \mapsto \dim_{p, q}\Lambda_{\sigma} $$
$\operatorname{Teich}(\Sigma)$
.
Part (2) is an immediate consequence of part (1) by the rigidity theorem on
$\delta_{p,q}(\sigma)$
, due to Bishop and Steger [Reference Bishop and StegerBS93, Theorem 2] and to Burger [Reference BurgerBur93, Theorem 1(a)]. For a more general version for convex cocompact representations, see Corollary 9.14. If we denote by
$f=f_\sigma$
the
$\sigma$
-equivariant homeomorphism
$\mathbb S^1\to \mathbb S^1$
, then
$\Lambda_\sigma=\{(x, f(x)):x\in \mathbb S^1\}$
and
$\dim_{p,q} \Lambda_\sigma$
can also be understood as the Hausdorff dimension of
$\Lambda_\Sigma=\mathbb S^1$
with respect to the premetric
$d_{\sigma, p,q} (x,y)= d_{\mathbb S^1}(x,y)^p d_{\mathbb S^1}(f(x), f(y))^q$
,
$x,y\in \mathbb S^1$
.
1.4 Hausdorff dimension of
$\Lambda_\theta$
with respect to a Riemannian metric
We denote by
$\dim \Lambda_\theta$
the Hausdorff dimension of
$\Lambda_\theta$
with respect to a Riemannian metric on
$\mathcal F_\theta$
; since all Riemannian metrics on
$\mathcal F_\theta$
are Lipschitz equivalent to each other, this is well-defined. With the exception of
$G=\operatorname{{\rm SO}}^\circ(n,1)$
,
$\dim \Lambda$
is not in general equal to the critical exponent of
$\Gamma$
even in the rank-one case. For a discussion on this for the case of
$G=\operatorname{SU}(n,1)$
, see [Reference DuflouxDuf17].
From Theorem 1.4, we derive an estimate on
$\dim \Lambda_\theta$
in terms of critical exponents. Let
$\chi_{\alpha}$
denote the Tits weight of G associated to
$\alpha\in \Pi$
as given in (10.2). When G is split over
$\mathbb R$
,
$\chi_\alpha$
is simply the fundamental weight associated to
$\alpha$
. We prove the following.
Theorem 1.7.
For any
$\theta$
-Anosov subgroup
$\Gamma$
of G, we have
Moreover, both the upper and lower bounds are attained by some Anosov subgroups.
For
$G=\operatorname{{\rm PSL}}_n(\mathbb R)$
, we have the set of simple roots given by
When
$G=\operatorname{{\rm PSL}}_n(\mathbb R)$
and
$\theta=\{\alpha_1\}$
, the lower bound in Theorem 1.7 has been obtained by Dey and Kapovich [Reference Dey and KapovichDK22], and the upper bound by Pozzetti, Sambarino, and Wienhard [Reference Pozzetti, Sambarino and WienhardPSW23] (see also [Reference Canary, Zhang and ZimmerCZZ26]). For some special classes of Anosov subgroups, much sharper bounds are known (see [Reference Glorieux, Monclair and TholozanGMT23, Reference Pozzetti, Sambarino and WienhardPSW21, Reference Pozzetti, Sambarino and WienhardPSW23, Reference Kim, Minsky and OhKMO23]). Recently, Li, Pan, and Xu have proved that for
$G=\operatorname{{\rm PSL}}_3(\mathbb R)$
,
$\dim\Lambda_{\alpha_1} $
coincides with the affinity exponent of
$\Gamma$
(see [Reference Li, Pan and XuLPX23]). See also [Reference Lee and OhLO24, Reference Kim, Oh and WangKOW25b], which show that
$\Lambda_\theta$
has Lebesgue measure zero in higher rank, and [Reference Ledrappier and LessaLL25], which shows that
$\dim \Lambda_\theta$
has a positive co-dimension for all Zariski dense Anosov subgroups of
$\operatorname{{\rm PSL}}_n(\mathbb R)$
,
$n\ge 3$
.
The novelty of Theorem 1.7 is that it applies to all
$\theta$
-Anosov subgroups of any semisimple real algebraic group. Since both upper and lower bounds are realized by some Anosov subgroups, Theorem 1.7 cannot be improved in this generality. A Hitchin subgroup of
$\operatorname{{\rm PSL}}_n(\mathbb R)$
is the image of a representation
$\pi: \Sigma \to \operatorname{{\rm PSL}}_n(\mathbb R)$
of a uniform lattice
$\Sigma\lt \operatorname{{\rm PSL}}_2(\mathbb R)$
belonging to the same connected component as
$\iota|_\Sigma$
in the character variety
$\operatorname{Hom}(\Sigma, \operatorname{{\rm PSL}}_n(\mathbb R))/\sim$
, where
$\iota$
is the irreducible representation of
$\operatorname{{\rm PSL}}_2(\mathbb R)$
into
$\operatorname{{\rm PSL}}_n(\mathbb R)$
and the equivalence is given by conjugations. Hitchin subgroups are
$\Pi$
-Anosov, as has been shown by Labourie [Reference LabourieLab06, Theorem 1.4]. For Hitchin subgroups of
$\operatorname{{\rm PSL}}_n(\mathbb R)$
, we have
$\dim \Lambda_{\theta} = 1$
by [Reference LabourieLab06] and [Reference Canary, Zhang and ZimmerCZZ26, Proposition 1.5], and
$\delta_{\alpha} = 1$
for all
$\alpha \in \Pi$
by [Reference Potrie and SambarinoPS17, Theorem B]. Hence
The upper bound in Theorem 1.7 is also obtained for Anosov subgroups of the product of
$\operatorname{{\rm SO}}^\circ(n, 1)$
(see [Reference Kim, Minsky and OhKMO23]). For the lower bound, let
$\Gamma$
be the image of a uniform lattice
$\Sigma$
of
$\operatorname{{\rm PSL}}_2(\mathbb R)$
under the embedding
where
$I_{n-2}$
is the
$(n-2) \times (n-2)$
identity matrix. Then,
$\Gamma$
is
$\{\alpha_1\}$
-Anosov. On one hand, the limit set
$\Lambda_{\alpha_1}$
of
$\Gamma$
in
$\mathcal F_{\alpha_1} = \mathbb{P}(\mathbb R^n)$
is the projective line, and hence
$\dim \Lambda_{\alpha_1} = 1$
. On the other hand, since
$(\chi_{\alpha_1} + \chi_{{\rm i}(\alpha_1)})(\operatorname{{\rm diag}}(a_1, \ldots, a_n)) = a_1 - a_n$
, we have
Therefore, the lower bound in Theorem 1.7 is achieved for this example.
1.5 Growth indicator bounds and
$L^2$
-spectral properties
The growth indicator
$\psi_{\Gamma}=\psi_\Gamma^{\Pi}:\mathfrak a\to \mathbb R \cup\{-\infty\}$
is a higher-rank version of the critical exponent of
$\Gamma$
that captures the growth rate of
$\mu(\Gamma)$
in each direction of
$\mathfrak a$
(Definition 3.1). This was introduced by Quint [Reference QuintQui02a]. Denote by
$\rho $
the half-sum of all positive roots of
$(\mathfrak g, \mathfrak a)$
counted with multiplicity. Then, for any discrete subgroup
$\Gamma\lt G$
,
$\psi_\Gamma \le 2 \rho$
, and if G is simple and has higher rank and
$\text{Vol}(\Gamma\backslash G)=\infty$
, then Quint has proved a gap theorem that
$\psi_\Gamma \le 2\rho-\Theta$
, where
$\Theta$
denotes the half-sum of all roots in a maximal strongly orthogonal system of
$(\mathfrak g, \mathfrak a)$
(see [Reference QuintQui03b, Reference OhOh02] and [Reference Lee and OhLO24, Theorem 7.1]). We obtain the following bound on
$\psi_\Gamma$
for Anosov subgroups.
Corollary 1.8.
For any
$\theta$
-Anosov subgroup
$\Gamma$
of G, we have
Recall that
$X=G/K$
denotes the associated Riemannian symmetric space. The size of
$\psi_\Gamma$
is closely related to the spectral properties of the locally symmetric space
$\Gamma\backslash X$
. Let
$\lambda_0(\Gamma\backslash X)$
denote the bottom of the
$L^2$
-spectrum of
$\Gamma\backslash X$
(see (11.4)). As first introduced by Harish-Chandra [Har66], a unitary representation
$(\pi, \mathcal H_{\pi})$
of G is tempered if all of its matrix coefficients belong to
$L^{2+\varepsilon}(G)$
for all
$\varepsilon\gt 0$
, or, equivalently, if
$\pi$
is weakly containedFootnote
4
in the regular representation
$L^2(G)$
. Hence, the temperedness of the quasi-regular representation
$L^2(\Gamma\backslash G)$
means that
$\Gamma\backslash G$
looks like G from the
$L^2$
-viewpoints. If a discrete subgroup
$\Gamma$
of G satisfies that
$\psi_\Gamma\le \rho$
, then
$L^2(\Gamma\backslash G)$
is tempered and
$\lambda_0(\Gamma\backslash X)=\|\rho\|^2$
as shown in [Reference Edwards and OhEO23, Theorem 1.6] for
$\Pi$
-Anosov groups and in [Reference Lutsko, Weich and WolfLWW24] in general. Moreover,
$\lambda_0(\Gamma\backslash X)$
is not an
$L^2$
-eigenvalue [Reference Edwards and OhEO23, Reference Edwards, Fraczyk, Lee and OhEFL+24]. However, it is not easy to decide whether or not
$\psi_\Gamma \le \rho$
holds. We give a criterion for this in terms of
$\dim \Lambda_\theta$
using Corollary 1.8.
Define
$$\mathsf c_\theta:=\min\bigg\{c \ge 0:\sum_{\alpha\in \theta} (\chi_\alpha + \chi_{{\rm i}(\alpha)}) \le c\cdot \rho\; \text{on } \mathfrak a^+\bigg\}.$$
We set
$\mathsf c_G := \mathsf c_\Pi$
. Note that
$0 \lt \mathsf c_\theta\le \mathsf c_{G}$
and, moreover, if
$\theta\cap {\rm i}(\theta)=\emptyset$
,
$\mathsf c_\theta \le \mathsf{c}_G/2$
.
If G is
$\mathbb R$
-split, then
$\sum_{\alpha\in \Pi} \chi_\theta= \rho $
[Reference BourbakiBou02, Proposition 29], and hence
$\mathsf c_G=2$
. In general, we have
by Lemma 10.3 due to Smilga.
Corollary 1.9.
Let
$\Gamma$
be a
$\theta$
-Anosov subgroup such that
Then,
$L^2(\Gamma \backslash G)$
is tempered and
$\lambda_0(\Gamma\backslash X) = \| \rho\|^2$
. In particular, the conclusion holds for any
$\Pi$
-Anosov subgroup with
$\dim \Lambda \le {\operatorname{rank } G}/{{\mathsf c}_G}$
.
For a more general statement, see Remark 11.6. Corollary 1.9 recovers Sullivan’s theorem [Reference SullivanSul87] in rank-one Lie groups (see Remark 11.7) and immediately applies to many examples of Anosov subgroups with limit sets of low Hausdorff dimensions; for example, to all
$\Pi$
-Anosov subgroups of higher-rank Lie groups with
$\dim \Lambda\le 1$
such as Hitchin subgroups and the image of any positive representation into a real split group [Reference Canary, Zhang and ZimmerCZZ26, Propositions 1.5 and 11.1]. Although the conclusion of Corollary 1.9 was already known for Hitchin subgroups by [Reference Kim, Minsky and OhKMO24] and [Reference Edwards and OhEO23], relying on the work of [Reference Potrie and SambarinoPS17], we obtain a completely different proof in this paper. Another application is that the image of a maximal representation of a surface group into
$\operatorname{Sp}_{2n}(\mathbb R)$
is a tempered subgroup of
$\operatorname{Sp}_{2n}(\mathbb R)$
for
$n\ge 3$
. Such an image is an
$\{\alpha_n\}$
-Anosov subgroup of
$\operatorname{Sp}_{2n}(\mathbb R)$
, where
$\alpha_n$
is the long simple root of
$\operatorname{Sp}_{2n}(\mathbb R)$
,
$\dim \Lambda_{\alpha_n}=1$
by [Reference Burger, Iozzi, Labourie and WienhardBIL+05], and we can directly compute
$c_{\alpha_n}\le 1$
for
$n\ge 3$
.
Since the opposition involution i of
$\operatorname{{\rm PSL}}_n(\mathbb R)$
sends the simple root
$\alpha_i$
to
$\alpha_{n-i}$
for
$1 \le i \le n -1$
, we also deduce the following.
Corollary 1.10.
Let
$n\ge 3$
. If
$\Gamma\lt \operatorname{{\rm PSL}}_n(\mathbb R)$
is
$\{\alpha_i\}$
-Anosov with
$\dim \Lambda_{\alpha_i}\le~1$
for some
$i\ne {n}/{2}$
, then
$L^2(\Gamma \backslash \operatorname{{\rm PSL}}_n(\mathbb R))$
is tempered and
$\lambda_0(\Gamma\backslash X ) = \| \rho\|^2$
.
This corollary applies to any (1,1,2)-hyperconvex subgroup whose Gromov boundary is homeomorphic to a circle, since such a subgroup is
$\{\alpha_1\}$
-Anosov with
$\dim \Lambda_{\alpha_1} = 1$
by Pozzetti, Sambarino, and Wienhard [Reference Pozzetti, Sambarino and WienhardPSW21]. It also applies to the image of a purely hyperbolic Schottky representation of the free group
$F_k$
on k-generators in
$\operatorname{{\rm PSL}}_n(\mathbb R)$
in the sense of Burelle and Treib [Reference Burelle and TreibBT22] by [Reference Canary, Zhang and ZimmerCZZ26, Proposition 11.1].
1.6 On the proof of Theorem 1.1
The key step is to prove that for a symmetric
$\psi\in \mathscr T_\Gamma$
, the Patterson–Sullivan measure
$\nu_\psi$
is Ahlfors one-regular. Fix
$o=[K]\in X$
. The
$\theta$
-Anosov property of
$\Gamma$
implies that
$\Gamma$
is a hyperbolic group and that the orbit map
$\gamma \mapsto \gamma o$
is a quasi-isometric embedding that continuously extends to a
$\Gamma$
-equivariant homeomorphism between the Gromov boundary
$\partial \Gamma$
and limit set
$\Lambda_\theta $
. One key feature of a Gromov hyperbolic space is that the Gromov product measures the distance between a fixed point and a geodesic, up to an additive error. The main philosophy of our proof is to establish an analogue of this property, by showing that there is a metric-like function
$\mathsf{d}_\psi$
on
$\Gamma o$
that is closely related to the
$\psi$
-Gromov product
$\psi \circ \mathcal G$
on the limit set
$\Lambda_\theta$
. For
$\gamma_1, \gamma_2 \in \Gamma$
, set
We prove that
$\mathsf{d}_\psi$
satisfies the coarse triangle inequality (Theorem 4.1), using a higher-rank Morse lemma due to Kapovich, Leeb, and Porti [Reference Kapovich, Leeb and PortiKLP18]: there exists
$D\gt 0$
such that for any
$ \gamma_1, \gamma_2, \gamma_3 \in \Gamma$
,
This allows us to treat
$\mathsf{d}_{\psi}$
as a ‘metric’ on
$\Gamma o$
. Moreover,
$(\Gamma o, \mathsf{d}_{\psi})$
has a uniform thin-triangle property. That is, there exists
$\delta \gt 0$
such that for any
$\xi_1, \xi_2, \xi_3 \in \Gamma \cup \partial \Gamma$
, the image of the geodesic triangle
$[\xi_1, \xi_2] \cup [\xi_2, \xi_3] \cup [\xi_3, \xi_1]$
under the orbit map is
$\delta$
-thin in the
$\mathsf{d}_{\psi}$
-metric. On the other hand, since
$(\Gamma o, \mathsf{d}_{\psi})$
is not a geodesic space in general, the thin-triangle property does not imply that
$(\Gamma o, \mathsf{d}_{\psi})$
is a Gromov hyperbolic space. Nevertheless, investigating fine geometric properties of thin triangles in
$(\Gamma o, \mathsf{d}_{\psi})$
leads us to proving that the
$\psi$
-Gromov product measures the
$\mathsf{d}_{\psi}$
-distance between o and a geodesic (Proposition 6.7). That is, for
$\xi \neq \eta \in \Lambda_{\theta} \simeq \partial \Gamma$
,
where
$[\xi, \eta]o$
is the image of a bi-infinite geodesic
$[\xi, \eta]$
in
$\Gamma$
connecting
$\xi$
and
$\eta$
under the orbit map. We also prove that shadows on the Gromov boundary
$\partial \Gamma$
are comparable to shadows on
$\Lambda_\theta$
(Proposition 7.2) and use it to establish the comparability of the
$d_{\psi}$
-balls and shadows in
$\Lambda_{\theta}$
(Theorem 6.2): for all large
$R \gt 1$
, there exists
$c \ge 1$
such that for any
$\xi\in \Lambda_\theta$
and
$\gamma \in \Gamma$
on a geodesic ray in
$\Gamma$
toward
$\xi\in \Lambda_\theta\simeq \partial \Gamma$
from the identity
$e \in \Gamma$
, we have
where the shadow
$O_R(o, \gamma o)$
is the set of endpoints of all positive Weyl chambers based at o passing through the Riemannian ball in X of radius
$R \gt 0$
with center
$\gamma o$
in X. Then, the Ahlfors one-regularity of
$\nu_\psi$
is deduced by applying the higher-rank version of Sullivan’s shadow lemma (Lemma 8.4). While positivity of
$\mathcal H_{\psi}(\Lambda_{\theta})$
is a standard consequence of the Ahlfors 1-regularity, finiteness of
$\mathcal H_{\psi}(\Lambda_{\theta})$
is not immediate, since
$d_\psi$
is not a genuine metric. We rely on the Vitali covering type lemma for the conformal premetric
$d_{\psi}$
on
$\Lambda_{\theta}$
(Lemma 5.6).
1.7 Organization
-
– In § 2, we review some basic structures of Lie groups and
$\theta$
-boundaries. The notation set up in this section is used throughout the paper. -
– In § 3, we recall the classification of Patterson–Sullivan measures of Anosov subgroups using tangent forms and some basic properties of Anosov subgroups.
-
– In § 4, we show that for each
$\psi\in \mathfrak a_\theta^*$
positive on
$\mathcal L_\theta-\{0\}$
, the composition
$\psi \circ \mu$
defines a metric-like function
$\mathsf{d}_\psi$
on the
$\Gamma$
-orbit
$\Gamma o$
. The coarse triangle inequality of
$\mathsf{d}_\psi$
(Theorem 4.1) is a crucial ingredient of this paper. Its proof makes a heavy use of the notion of diamonds and the Morse lemma due to Kapovich, Leeb, and Porti (Theorem 4.11). -
– In § 5, we define a conformal premetric
$d_\psi$
on the limit set
$\Lambda_\theta$
and discuss its basic properties. -
– Sections 6 and 7 are devoted to the proof of the compatibility between shadows and
$d_\psi$
-balls in the limit set
$\Lambda_\theta$
as in (1.9). -
– In §§ 8 and 9, we prove Theorem 1.1. In § 8, we prove that for symmetric
$\psi \in \mathfrak a_{\theta}^*$
, the
$(\Gamma, \psi)$
-Patterson–Sullivan measure is Ahlfors one-regular. In § 9, we prove that Patterson–Sullivan measures for symmetric linear forms are Hausdorff measures on the limit set, up to a constant multiple. We also prove Theorem 1.4. -
– In § 10, we prove Theorem 1.7 on the estimate of the Hausdorff dimension of
$\Lambda_\theta$
with respect to a Riemannian metric. -
– In § 11, we obtain an upper bound on the growth indicator and discuss its implications on the temperedness of
$L^2(\Gamma \backslash G)$
.
2. Basic structure theory of Lie groups and
$\theta$
-boundaries
Throughout the paper, let G be a connected semisimple real algebraic group; more precisely, G is the identity component
$\mathbf G(\mathbb R)^\circ$
of the group of real points of a semisimple algebraic group
$\mathbf G$
defined over
$\mathbb R$
. In this section, we review some basic facts about the Lie group structure of G. Let A be a maximal real split torus of G. Let
$\mathfrak g$
and
$\mathfrak a$
, respectively, denote the Lie algebras of G and A. Fix a positive Weyl chamber
$\mathfrak a^+ \subset \mathfrak a$
and set
$A^+=\exp \mathfrak a^+$
, and a maximal compact subgroup
$K\lt G$
such that the Cartan decomposition
$G=K A^+ K$
holds. Let
$\Phi=\Phi(\mathfrak g, \mathfrak a)$
denote the set of all roots and
$\Pi$
the set of all simple roots given by the choice of
$\mathfrak a^+$
. Denote by
$N_K(A)$
and
$C_K(A)$
the normalizer and centralizer of A in K, respectively. The Weyl group
$\mathcal W$
is given by
$N_K(A)/C_K(A)$
. Consider the real vector space
$\mathsf E^*=\mathsf X(A)\otimes_\mathbb Z \mathbb R$
, where
$\mathsf X(A)$
is the group of all real characters of A and let
$\mathsf E$
be its dual. Denote by (,) a
$\mathcal W$
-invariant inner product on
$\mathsf E$
. We denote by
$\{\omega_{\alpha}:\alpha\in \Pi\}$
the (restricted) fundamental weights of
$\Phi$
defined by
where
$c_\alpha=1$
if
$2\alpha\notin \Phi$
and
$c_\alpha=2$
otherwise.
Fix an element
$w_0\in N_K(A) $
of order 2 representing the longest Weyl element so that
$\operatorname{{\rm Ad}}_{w_0}\mathfrak a^+= -\mathfrak a^+$
. The map
is called the opposition involution. It induces an involution of
$ \Phi$
preserving
$\Pi$
, for which we use the same notation i, so that
${\rm i} (\alpha ) = \alpha \circ {\rm i}$
for all
$\alpha\in \Phi$
.
Henceforth, we fix a non-empty subset
$\theta$
of
$ \Pi$
. Let
\begin{align*}\mathfrak {a}_\theta &=\bigcap_{\alpha \in \Pi-\theta} \ker \alpha,\quad \mathfrak a_\theta^+ =\mathfrak a_\theta\cap \mathfrak a^+, \\A_{\theta} &= \exp \mathfrak a_{\theta} \quad \text{and} \quad A_{\theta}^+ = \exp \mathfrak a_{\theta}^+.\end{align*}
Let
denote the projection invariant under all
$w\in \mathcal W$
fixing
$\mathfrak a_\theta$
pointwise.
Let
$ P_\theta$
denote a standard parabolic subgroup of G corresponding to
$\theta$
; that is,
$P_{\theta}=L_\theta N_\theta$
, where
$L_\theta$
is the centralizer of
$A_\theta$
and
$N_\theta$
is the unipotent radical of
$P_\theta$
such that
$\log N_\theta$
is generated by root subgroups associated to all positive roots that are not
$\mathbb Z$
-linear combinations of
$\Pi-\theta$
.
We set
$M_{\theta} = K \cap P_{\theta}=C_K(A_\theta)$
. The Levi subgroup
$L_\theta$
can be written as
$L_{\theta} = A_{\theta}S_{\theta}$
, where
$S_{\theta}$
is an almost direct product of a connected semisimple real algebraic subgroup and a compact center. Letting
$B_\theta=S_\theta \cap A$
and
$B_\theta^+=\{b\in B_\theta: \alpha (\log b)\ge 0 \text{ for all }\},$
we have the Cartan decomposition of
$S_\theta$
:
Note that
$A=A_\theta B_\theta$
and
$ A^+\subset A_\theta^+ B_\theta^+.$
The space
$\mathfrak a_\theta^*=\operatorname{Hom}(\mathfrak a_\theta, \mathbb R)$
can be identified with the subspace of
$\mathfrak a^*$
consisting of
$p_\theta$
-invariant linear forms:
Hence, for
$\theta_1\subset \theta_2$
, we have
When
$\theta=\Pi$
, we will omit the subscript. So
$P=P_\Pi$
is a minimal parabolic subgroup and
$P=MAN$
.
2.1 Cartan projection
Recall the Cartan decomposition
$G = KA^+ K$
, which means that for every
$g\in G$
, there exists a unique element
$\mu(g)\in \mathfrak a^+$
such that
$g\in K \exp \mu(g) K$
. The map
$G\to \mathfrak a^+$
given by
$g\mapsto \mu(g)$
is called the Cartan projection. We have
Let
$X = G/K$
be the associated Riemannian symmetric space and set
$o = [K] \in X$
. Fix a K-invariant norm
$\| \cdot \|$
on
$\mathfrak g$
and a Riemannian distance d on X, induced from the Killing form on
$\mathfrak g$
, so that
for any
$g, h \in G$
. For
$p \in X$
and
$R \gt 0$
, let B(p, R) denote the metric ball
$ \{x \in X : d(x, p) \lt R\}$
.
Lemma 2.1 [Reference BenoistBen97, Lemma 4.6]. For any compact subset
$Q \subset G$
, there exists a constant
$C=C_Q\gt 0$
such that for all
$g \in G$
,
We then write
In view of (2.3), we have
$\psi\circ \mu_\theta=\psi \circ \mu$
for all
$\psi\in \mathfrak a_\theta^*$
.
2.2 The
$\theta$
-boundary
$\mathcal F_\theta$
We set
Let
denote the canonical projection map given by
$gP\mapsto gP_\theta$
,
$g\in G$
. We set
By the Iwasawa decomposition
$G=KP=KAN$
, the subgroup K acts transitively on
$\mathcal F_\theta$
, and hence
$\mathcal F_\theta\simeq K/ M_\theta.$
We consider the following notion of convergence of a sequence in G (or in X) to an element of
$\mathcal F_\theta$
. For a sequence
$g_i \in G$
, we say
$g_i \to \infty$
$\theta$
-regularly if
$\min_{\alpha\in \theta} \alpha(\mu(g_i)) \to \infty$
as
$i \to \infty$
.
Definition 2.2. For a sequence
$g_i\in G$
and
$\xi\in \mathcal F_\theta$
, we write
$\lim_{i\to \infty} g_i=\lim g_i o =\xi$
and say
$g_i $
(or
$g_io \in X$
) converges to
$\xi$
if:
-
–
$g_i \to \infty$
$\theta$
-regularly; and -
–
$\lim_{i\to\infty} \kappa_{i}\xi_\theta= \xi$
in
$\mathcal F_\theta$
for some
$\kappa_{i}\in K$
such that
$g_i\in \kappa_{i} A^+ K$
.
2.3 Points in general position
Let
$P_\theta^+$
be the standard parabolic subgroup of G opposite to
$P_\theta$
such that
$P_\theta\cap P_\theta^+=L_\theta$
. We have
$P_\theta^+ =w_0 P_{{\rm i}(\theta)}w_0^{-1}$
and hence
For
$g\in G$
, we set
as we fix
$\theta$
in the entire paper, we write
$g^{\pm}=g_\theta^{\pm}$
for simplicity when there is no room for confusion. Hence, for the identity
$e\in G$
,
$(e^+, e^-)=(P_\theta, P_\theta^+)=(\xi_\theta, w_0\xi_{{\rm i}(\theta)})$
. The G-orbit of
$(e^+, e^-)$
is the unique open G-orbit in
$G/P_\theta\times G/P_\theta^+$
under the diagonal G-action. We set
Two elements
$\xi\in \mathcal F_\theta$
and
$\eta\in \mathcal F_{{\rm i}(\theta)}$
are said to be in general position (or antipodal) if
$(\xi, \eta)\in \mathcal F_\theta^{(2)}$
.
2.4 Busemann maps and Gromov products
The
$\mathfrak a$
-valued Busemann map
$\beta: \mathcal F\times G \times G \to\mathfrak a $
is defined as follows: for
$\xi\in \mathcal F$
and
$g, h\in G$
,
where
$\sigma(g^{-1},\xi)\in \mathfrak a$
is the unique element such that
$g^{-1}k \in K \exp (\sigma(g^{-1}, \xi)) N$
for any
$k\in K$
with
$\xi=kP$
. For
$(\xi,g,h)\in \mathcal F_\theta\times G\times G$
, we define
this is well-defined independent of the choice of
$\xi_0$
(see [Reference QuintQui02b, Lemma 6.1]). We also have
$\|\beta_\xi^{\theta}(g, h)\|\le d(go, ho)$
for all
$g, h\in G$
(see [Reference QuintQui02b, Lemma 8.9]). The Busemann map has the following properties: for all
$\xi \in \mathcal F_{\theta}$
and
$g_1, g_2, g_3\in G$
,
$$\begin{aligned} \text{(Invariance)} \quad & \beta_{\xi}^{\theta}(g_1, g_2) = \beta_{g_3 \xi}^{\theta}(g_3 g_1, g_3 g_2);\\ \text{(Cocycle property)} \quad & \beta_{\xi}^{\theta}(g_1, g_2) = \beta_{\xi}^{\theta}(g_1, g_3) + \beta_{\xi}^{\theta}(g_3, g_2).\end{aligned}$$
For
$p, q \in X$
and
$\xi \in \mathcal F_{\theta}$
, we set
$\beta_{\xi}^{\theta}(p, q) := \beta_{\xi}^{\theta}(g, h)$
where
$g, h \in G$
satisfies
$go = p$
and
$ho=q$
. It is easy to check that this is well-defined.
Definition 2.3.
For
$(\xi, \eta) \in \mathcal F_{\theta}^{(2)}$
, we define the
$\theta$
-Gromov product as
where
$g \in G$
satisfies
$(g^+, g^-) = (\xi, \eta)$
. This does not depend on the choice of g (see [Reference Kim, Oh and WangKOW25b, Lemma 9.11]).
3. Classification of Patterson–Sullivan measures by tangent forms
Let G be a connected semisimple real algebraic group. We fix a non-empty subset
$\theta$
of the set
$\Pi$
of all simple roots. Throughout this section, let
$\Gamma$
be a discrete subgroup of G. When
$\Gamma$
is
$\theta$
-Anosov, we have a complete classification of all linear forms
$\psi\in \mathfrak a_\theta^*$
admitting a
$(\Gamma, \psi)$
-Patterson–Sullivan measure [Reference Lee and OhLO23, Reference SambarinoSam24, Reference Kim, Oh and WangKOW25b]. The goal of this section is to review this classification, in addition to recalling some basic notions such as the limit cone and the growth indicator of
$\Gamma$
. For a more detailed discussion of the material of this section, we refer to [Reference Kim, Oh and WangKOW25b].
The
$\theta$
-limit set of
$\Gamma$
is defined as follows:
where
$\lim \gamma_i$
is defined as in Definition 2.2. If
$\Gamma \lt G$
is Zariski dense, then the limit set
$\Lambda_{\theta}$
is the unique
$\Gamma$
-minimal subset of
$\mathcal F_{\theta}$
(see [Reference BenoistBen97, § 3.6] and [Reference QuintQui02b, Theorem 7.2]). Furthermore, if we set
$\Lambda=\Lambda_\Pi$
, then
$ \pi_{\theta}(\Lambda) = \Lambda_{\theta}$
. For
$\psi \in \mathfrak a_{\theta}^*$
, a Borel probability measure
$\nu$
on
$\mathcal F_{\theta}$
is called a
$(\Gamma, \psi)$
-conformal measure if for all
$\gamma \in \Gamma$
and
$\xi \in \mathcal F_{\theta}$
,
where
$\gamma_*\nu(B) = \nu(\gamma^{-1} B)$
for any Borel
$B \subset \mathcal F_{\theta}$
. A
$(\Gamma, \psi)$
-conformal measure is called a
$(\Gamma, \psi)$
-Patterson–Sullivan measure if it is supported on
$\Lambda_{\theta}$
.
In order to discuss which linear forms
$\psi$
admit a Patterson–Sullivan measure, we need the definitions of the
$\theta$
-limit cones and growth indicators.
The
$\theta$
-limit cone
$\mathcal L_{\theta}=\mathcal L_\theta(\Gamma)$
of
$\Gamma$
is defined as the asymptotic cone of
$\mu_{\theta}(\Gamma)$
in
$\mathfrak a_{\theta}$
; that is,
$u\in \mathcal L_\theta$
if and only if
$u=\lim t_i \mu_\theta(\gamma_i)$
for some sequences
$t_i\to 0$
and
$\gamma_i\in \Gamma$
. If
$\Gamma$
is Zariski dense,
$\mathcal L_\theta$
is a convex cone with non-empty interior by [Reference BenoistBen97, § 1.2]. Recalling the convention of dropping the subscript
$\theta$
when
$\theta=\Pi$
, we write
$\mathcal L=\mathcal L_\Pi$
. We then have
$p_\theta(\mathcal L)=\mathcal L_\theta$
.
3.1 Growth indicators
We say that
$\Gamma$
is
$\theta$
-discrete if the restriction
$\mu_\theta|_{\Gamma}:\Gamma \to \mathfrak a_\theta^+$
is proper. The
$\theta$
-discreteness of
$\Gamma$
implies that
$\mu_\theta(\Gamma)$
is a closed discrete subset of
$\mathfrak a_\theta^+$
. Indeed,
$\Gamma$
is
$\theta$
-discrete if and only if the counting measure on
$\mu_\theta(\Gamma)$
weighted with multiplicity is a Radon measure on
$\mathfrak a_\theta^+$
.
Definition 3.1 (
$\theta$
-growth [Reference QuintQui02a, Reference Kim, Oh and WangKOW25b]). For a
$\theta$
-discrete subgroup
$\Gamma\lt G$
, the
$\theta$
-growth indicator
$\psi_\Gamma^{\theta}:\mathfrak a_\theta\to [-\infty, \infty] $
is defined as follows: if
$u \in \mathfrak a_\theta$
is non-zero,
where
$\mathcal C\subset \mathfrak a_\theta$
ranges over all open cones containing u, and
$\psi_{\Gamma}^{\theta}(0) = 0$
. Here,
$-\infty\le \tau^{\theta}_{\mathcal C}\le \infty$
denotes the abscissa of convergence of the series
${\mathcal P}^{\theta}_{\mathcal C}(s)=\sum_{\gamma\in \Gamma, \mu_\theta(\gamma)\in \mathcal C} e^{-s\|\mu_\theta(\gamma)\|}$
. As mentioned, we simply write
$\psi_{\Gamma} := \psi_{\Gamma}^{\Pi}$
.
This definition is independent of the choice of a norm on
$\mathfrak a_\theta$
. It has been proved in [Reference QuintQui02a, Theorem 1.1.1] and [Reference Kim, Oh and WangKOW25b, Theorem 3.3] that
where
$\operatorname{{\rm int}}\mathcal L_\theta$
denotes the interior of
$\mathcal L_\theta$
in the relative topology of
$\mathfrak a_{\theta}$
. Moreover,
$\psi_\Gamma^\theta$
is upper semi-continuous and concave. When
$\theta={\rm i}(\theta)$
, it follows from (2.5) that
$\psi_\Gamma^\theta$
is i-invariant.
We say that a linear form
$\psi$
is tangent to
$\psi_\Gamma^\theta$
(at
$u\in \mathfrak a_\theta-\{0\}$
) if
$\psi\ge \psi_\Gamma^\theta$
and
$\psi(u)=\psi_\Gamma^\theta(u)$
. For any
$u\in \operatorname{{\rm int}} \mathcal L_\theta$
, there exists
$\psi\in \mathfrak a_\theta^*$
tangent to
$\psi_\Gamma^\theta$
at u. Moreover, for any
$\psi\in \mathfrak a_\theta^*$
tangent to
$\psi_\Gamma^\theta$
at an interior direction of
$\mathfrak a_\theta^+$
, there exists a
$(\Gamma, \psi)$
-Patterson–Sullivan measure (see [Reference QuintQui02b, Theorem 8.4] and [Reference Kim, Oh and WangKOW25b, Proposition 5.9]).
For
$\theta$
-Anosov subgroups, we have a more precise classification of Patterson–Sullivan measures in terms of tangent forms.
Definition 3.2
A finitely generated subgroup
$\Gamma\lt G$
is
$\theta$
-Anosov if there exists a constant
$C \gt 1$
such that for all
$\alpha \in \theta$
and
$\gamma\in \Gamma$
, we have
where
$|\cdot|$
denotes a fixed word metric on
$\Gamma$
.
We recall that all
$\theta$
-Anosov subgroups are assumed to be non-elementary in this paper. Define
By the duality lemma (see [Reference QuintQui03a, § 4] and [Reference SambarinoSam14, Lemma 4.8]), the following can be deduced from [Reference SambarinoSam24, Theorem A] (see [Reference Kim, Oh and WangKOW25b, Theorem 13.2]).
Theorem 3.3.
Let
$\Gamma$
be a
$\theta$
-Anosov subgroup.
-
(1) We then have that
$\psi_\Gamma^\theta$
is analytic on
$\operatorname{{\rm int}} \mathcal L_{\theta}$
, strictly concave on
$\mathcal L_{\theta}$
, and vertically tangent.Footnote
5
-
(2) For any
$\psi \in \mathscr T_\Gamma$
, there exists a unique unit vector
$u=u_\psi\in \operatorname{{\rm int}} \mathcal L_\theta$
such that
$\psi(u)=\psi_\Gamma^\theta(u)$
. If
$\Gamma$
is Zariski dense, the map
$\psi\mapsto u_\psi$
is a bijection between
$\mathscr T_\Gamma$
and
$\{u\in \operatorname{{\rm int}} \mathcal L_{\theta}:\|u\|=1\}$
.
The following theorem has been proved in [Reference Lee and OhLO23, Theorem 1.3] for
$\theta=\Pi$
and
$\Gamma$
Zariski dense. The general case follows from [Reference SambarinoSam24, Theorem A] (for a more general discussion on conformal measures, see [Reference Kim, Oh and WangKOW25b, Corollary 1.13]).
Theorem 3.4.
Let
$\Gamma$
be a
$\theta$
-Anosov subgroup. For any
$\psi\in \mathscr T_\Gamma$
, there exists a unique
$(\Gamma, \psi)$
-Patterson–Sullivan measure on
$\Lambda_\theta$
, which we denote by
$\nu_\psi=\nu_{\psi, \theta}$
. The map
is a surjection from
$\mathscr T_\Gamma$
to the space of all
$\Gamma$
-Patterson–Sullivan measures. If
$\Gamma$
is Zariski dense, then the map
$\psi \mapsto \nu_{\psi}$
is bijective. Moreover, if
$\psi_1\ne \psi_2$
in
$\mathscr T_\Gamma$
, then
$\nu_{\psi_1}$
and
$\nu_{\psi_2}$
are mutually singular to each other.
Remark 3.5. One immediate consequence of the last statement of Theorem 3.4 is that at most one Patterson–Sullivan measure can be a Hausdorff measure on
$\Lambda_\theta$
with respect to a fixed metric (e.g., Riemannian metric).
When
$\psi\in \mathfrak a_\theta^*$
is positive on
$\mathcal L_{\theta}-\{0\}$
, the abscissa of convergence of the
$\psi$
-Poincaré series
is a well-defined positive number, which we denote by
$\delta_\psi$
(see [Reference Kim, Oh and WangKOW25b, Lemma 4.3]). Equivalently,
$\delta_\psi$
is also given by (1.3).
Lemma 3.6 [Reference Kim, Oh and WangKOW25b, Lemma 4.5]. If
$\psi\in \mathfrak a_\theta^*$
is positive on
$\mathcal L_\theta-\{0\}$
, then
In particular,
$\psi \in \mathscr T_{\Gamma}$
if and only if
$\delta_{\psi} = 1$
.
Since
$\mu(g^{-1}) = {\rm i}(\mu(g))$
for all
$g \in G$
, we have that
$\Gamma$
is
$\theta$
-Anosov if and only if
$\Gamma$
is
$\theta \cup {\rm i}(\theta)$
-Anosov. If
$\Gamma$
is
$\theta$
-Anosov, then the canonical projection map
$p:\Lambda_{\theta \cup {\rm i}(\theta)} \to \Lambda_{\theta}$
is a
$\Gamma$
-equivariant homeomorphism. Recalling that
$\mathfrak a_\theta^*$
can be considered as a subset of
$\mathfrak a_{\theta\cup{\rm i}(\theta)}^*$
from (2.4), we recall the following, which will be of use.
Lemma 3.7 [Reference Kim, Oh and WangKOW25b, Lemma 9.5]. Let
$\Gamma$
be a
$\theta$
-Anosov subgroup. For any
$\psi \in \mathscr T_\Gamma$
, the measure
$\nu_{\psi,\theta}$
coincides with the push-forward of
$\nu_{\psi, \theta\cup{\rm i}(\theta)}$
by p.
3.2 Gromov hyperbolic space and quasi-isometry
We collect a few basic facts about
$\theta$
-Anosov subgroups that will be used repeatedly.
Recall that a geodesic metric spaceFootnote
6
$(Z, d_Z)$
is called a Gromov hyperbolic space if it satisfies a uniformly thin-triangle property; that is, there exists
$T \gt 0$
such that for any geodesic triangle in Z, one side of the triangle is contained in the T-neighborhood of the union of two other sides. We denote by
$\partial Z$
the Gromov boundary of Z, which is the space of equivalence classes of geodesic rays in Z. For any
$z_1\ne z_2\in Z\cup \partial Z$
, there may be more than one geodesic connecting
$z_1$
and
$z_2$
. By the notation
$[z_1, z_2]$
, we mean ‘a’ geodesic in Z connecting
$z_1$
to
$z_2$
. For
$w\in Z$
, the nearest-point projection of w to a geodesic
$[z_1,z_2]$
is any point
$w'\in [z_1, z_2]$
satisfying
$d_Z(w,w')=\inf \{d_Z(w, z):z\in [z_1, z_2]\}$
. This is coarsely well-defined. We refer to [Reference Bridson and HaefligerBH99] for basics on Gromov hyperbolic spaces. Recall that d denotes the Riemannian distance function on
$X=G/K$
.
Theorem 3.8 (See [Reference Kapovich, Leeb and PortiKLP18, Corollary 1.6] and [Reference Kapovich, Leeb and PortiKLP17, Proposition 5.16, Lemma 5.23]; see also [Reference Guéritaud, Guichard, Kassel and WienhardGGK+17]). Let
$\Gamma$
be a
$\theta$
-Anosov subgroup. Fix a word metric
$\mathsf{d}_\Gamma$
on
$\Gamma$
with respect to a finite symmetric generating set.
-
(1) We have that
$(\Gamma, \mathsf{d}_\Gamma)$
is a Gromov hyperbolic space.Footnote
7
-
(2) Then,
$\mathcal L_\theta-\{0\}$
is contained in the relative interior of
$\mathfrak a_\theta^+$
in
$\mathfrak a_\theta$
. -
(3) The orbit map
$ (\Gamma,\mathsf{d}_\Gamma) \to (\Gamma o, d)$
given by
$ \gamma \mapsto \gamma o $
is a quasi-isometric embedding, i.e., there exist
$Q=Q_\Gamma\ge 1$
such that for all
$\gamma_1, \gamma_2\in \Gamma$
,
$$ Q^{-1}\cdot \mathsf{d}_{\Gamma}(\gamma_1, \gamma_2) -Q \le d(\gamma_1 o, \gamma_2 o) \le Q \cdot \mathsf{d}_{\Gamma}(\gamma_1, \gamma_2) +Q .$$
-
(4) The orbit map
$\Gamma \to \Gamma o$
uniquely extends to a
$\Gamma$
-equivariant continuous map
$f:\Gamma \cup \partial \Gamma \to \Gamma o \cup \Lambda_{\theta}$
and
$f|_{\partial \Gamma}$
is a homeomorphism onto
$\Lambda_\theta$
. For
$\theta={\rm i}(\theta)$
, f maps two distinct points of
$\partial \Gamma$
to points in general position.
We henceforth identity
$\partial \Gamma$
and
$\Lambda_\theta$
using f. For any
$\xi\ne \eta \in \Gamma \cup \partial \Gamma$
, note that
$f([\xi, \eta])=[\xi, \eta] o$
is the image of
$[\xi, \eta]$
under the orbit map.
4. Metric-like functions on
$\Gamma$
-orbits and diamonds
We fix a non-empty subset
$\theta \subset \Pi$
. In this section, we assume that
$\theta$
is symmetric, i.e.,
$\theta = {\rm i}(\theta)$
. Recall the notation
$X=G/K$
and
$o=[K]\in X$
.
For a linear form
$\psi \in \mathfrak a_{\theta}^*$
, define
$\mathsf{d}_{\psi} : X \times X \to \mathbb R$
as follows: for
$g, h \in G$
,
Since the Cartan projection
$\mu$
is bi-K-invariant,
$\mathsf{d}_\psi$
is a well-defined left G-invariant function.
The main goal of this section is to prove the following theorem saying that when
$\Gamma$
is
$\theta$
-Anosov,
$\mathsf{d}_\psi$
behaves like a metric, restricted to the
$\Gamma$
-orbit
$\Gamma o$
for a proper class of
$\psi$
values.
Theorem 4.1 (Coarse triangle inequality) Let
$\Gamma$
be a
$\theta$
-Anosov subgroup. Let
$\psi\in \mathfrak a_\theta^*$
be such that
$\psi\gt 0$
on
$\mathcal L_\theta-\{0\}$
. Then there exists a constant
$D=D_\psi\gt 0$
such that for all
$\gamma_1, \gamma_2,\gamma \in \Gamma$
,
Indeed, we prove Theorem 4.1 in a greater generality where the orbit
$\Gamma o$
is replaced by the image of a uniformly regular quasi-isometric embedding of a geodesic metric space into X.
4.1 Coarse triangle inequalities for uniformly regular quasi-isometric embeddings
We set
$\mathcal W_\theta$
to be the set of all Weyl elements that fix
$\mathfrak a_\theta$
pointwise. We define a closed cone
$\mathcal C$
in
$\mathfrak a^+$
to be
$\theta$
-admissible if the following three conditions hold:
-
(1)
$\mathcal C$
is i-invariant, so
${\rm i}(\mathcal C)=\mathcal C$
; -
(2)
$\mathcal W_\theta \cdot \mathcal C=\bigcup_{w\in \mathcal W_\theta} \operatorname{{\rm Ad}}_w \mathcal C $
is convex; and -
(3)
$\mathcal C\cap (\bigcup_{\alpha\in \theta} \ker \alpha) =\{0\}$
.
For a
$\theta$
-admissible cone
$\mathcal C$
, we say that an ordered pair
$(x_1, x_2)$
of distinct points in X is
$\mathcal C$
-regular if for
$g_1, g_2 \in G$
such that
$g_1 o = x_1$
and
$g_2 o = x_2$
, we have
In this case,
$x_2 = g_2 o \in g_1 K (\exp \mathcal C) o$
and hence for some
$g \in g_1 K$
,
$x_1 = g_1 o = go$
and
$x_2 \in g (\exp \mathcal C) o$
. Note that if
$(x_1, x_2)$
is
$\mathcal C$
-regular, then
$(x_2, x_1)$
is
${\rm i}(\mathcal C)$
-regular and hence
$\mathcal C$
-regular by the i-invariance of
$\mathcal C$
.
Definition 4.2 Let
$(Z, d_Z)$
be a metric space and
$f:Z\to X$
be a map. For a cone
$\mathcal C \subset \mathfrak a^+$
and a constant
$B\ge 0$
, f is called
$(\mathcal C,B)$
-regular if the pair
$(f(z_1),f(z_2))$
is
$\mathcal C$
-regular for all
$z_1, z_2 \in Z$
with
$d_Z(z_1,z_2) \ge B$
. We simply say that f is
$\mathcal C$
-regular if it is
$(\mathcal C, B)$
-regular for some
$B \ge 0$
.
Theorem 4.1 will be deduced as a special case of the following theorem: we write
$\mathcal C_\theta=p_\theta(\mathcal C)$
.
Theorem 4.3.
Let Z be a geodesic metric space and
$\mathcal C\subset \mathfrak a^+$
a
$\theta$
-admissible cone. Let
$f: Z\to X$
be a
$\mathcal C$
-regular quasi-isometric embedding.
Footnote 8
If
$\psi \in \mathfrak a_\theta^*$
is positive on
$\mathcal C -\{0\}$
, then there exists a constant
$D=D_\psi \ge 0$
such that for all
$x_1,x_2,x_3\in f(Z)$
,
We continue to use notation
$\operatorname{{\rm int}}\mathfrak a^+$
and
$\operatorname{{\rm int}}\mathfrak a_\theta^+$
for relative interiors in the topology of
$\mathfrak a$
and
$\mathfrak a_\theta$
, respectively. Unless mentioned otherwise, for any proper cone
$\mathcal C$
in
$\mathfrak a^+$
(respectively,
$\mathfrak a_\theta^+$
), we denote by
$\operatorname{{\rm int}} \mathcal C$
the interior of
$\mathcal C$
in the relative topology of
$\mathfrak a^+$
(respectively,
$\mathfrak a_\theta^+$
).
4.2 Proof of Theorem 4.1 assuming Theorem 4.3
Let
$\psi\in \mathfrak a_\theta^*$
be such that
$\psi\gt 0$
on
$\mathcal L_\theta-\{0\}$
. We will construct a
$\theta$
-admissible cone
$\mathcal C\subset \mathfrak a^+$
such that
$\mathcal L-\{0\}\subset \operatorname{{\rm int}} \mathcal C $
and
$\psi$
is positive on
$\mathcal C -\{0\}$
.
Since
$\theta={\rm i}(\theta)$
by hypothesis, it follows from (2.5) that
${\rm i}|_{\mathfrak a_\theta}$
is an involution preserving
$\mathcal L_\theta$
. Since
$\psi$
is positive on
$\mathcal L_\theta-\{0\}$
and
$\mathcal L_{\theta} - \{0\} \subset \operatorname{{\rm int}} \mathfrak a_{\theta}^+$
(Theorem 3.8(2)), we can choose a closed convex cone
$\mathcal C_0 \subset \mathrm{int}\, \mathfrak a_{\theta}^+ \cup \{0\}$
satisfying:
-
(1)
$\mathcal L_{\theta}-\{0\} \subset \mathrm{int}\, \mathcal C_0$
; -
(2)
${\rm i}(\mathcal C_0)=\mathcal C_0$
; and -
(3)
$\psi\gt 0$
on
$\mathcal C_0 - \{0\}$
.
We observe that
$\mathcal W_\theta \cdot \mathfrak a^+ $
is equal to the union of all Weyl chambers containing
$\mathfrak a_\theta^+$
, and hence is a convex cone by [Reference Kapovich, Leeb and PortiKLP17, Lemma 2.6].
Let
$\alpha\in \theta$
. It follows from (3.2) that
$ \mathcal L\cap \ker \alpha =\{0\}$
. Since
$\ker \alpha \cap \mathfrak a^+$
is contained in the boundary of
$\mathcal W_\theta \cdot \mathfrak a^+$
, it follows from the convexity of
$\mathcal W_\theta\cdot \mathfrak a^+$
that
$\mathcal W_\theta \cdot \mathfrak a^+$
is contained in the half-space
$\{\alpha\ge 0\}$
. Hence, both
$\operatorname{{\rm int}} \mathfrak a_\theta^+$
and
$\mathcal W_\theta \cdot \mathcal L -\{0\}$
are contained in the open half-space
$\{\alpha\gt 0\}$
. Therefore, we can find a linear form
$h_\alpha\in \mathfrak a^*$
such that
Now set
$H:=\bigcap_{\alpha\in \theta, w\in \mathcal W_\theta} \{h_\alpha\circ \operatorname{{\rm Ad}}_{w} \ge 0\}$
, which is clearly a
$\mathcal W_\theta$
-invariant convex cone. By our choice of
$h_\alpha$
,
$\operatorname{{\rm int}} H$
contains
$\mathcal L-\{0\}$
. Since
$\theta={\rm i}(\theta)$
and hence
$\mathcal W_\theta =\mathcal W_{{\rm i}(\theta)}$
, we have that
${\rm i}(H)$
is also a
$\mathcal W_\theta$
-invariant convex cone whose interior contains
$\mathcal L-\{0\}={\rm i}(\mathcal L)-\{0\}$
.
Define
By construction, we have
$ \mathcal C \cap (\bigcup_{\alpha \in \theta} \ker \alpha )= \{0\}$
. In particular,
$\mathcal C$
is a proper closed cone in
$\mathfrak a^+$
. Then,
$\operatorname{{\rm int}} \mathcal C$
contains
$\mathcal L-\{0\}$
. Since
$\psi\gt 0$
on
$\mathcal C_0$
and
$\psi$
is
$p_\theta$
-invariant,
$\psi\gt 0$
on
$\mathcal C$
. Since
${\rm i}(\mathcal C_0)=\mathcal C_0$
, we have
${\rm i}(\mathcal C)=\mathcal C$
. Using the fact that
$p_\theta : \mathfrak a \to \mathfrak a_\theta$
is
$\mathcal W_\theta$
-equivariant, we have that
Since
$p_{\theta}^{-1}(\mathcal C_0)$
,
$\mathcal W_{\theta} \cdot \mathfrak a^+$
, H, and
${\rm i}(H)$
are convex, it follows that
$\mathcal W_\theta\cdot \mathcal C $
is convex.
Therefore,
$\mathcal C$
is
$\theta$
-admissible. Since the orbit map
$ (\Gamma,\mathsf{d}_\Gamma) \to (X, d)$
,
$\gamma \mapsto \gamma o $
, is a quasi-isometric embedding by Theorem 3.8(3) and any open cone containing
$\mathcal L$
contains
$\mu(\Gamma)$
except for finitely many points, Theorem 4.1 follows from Theorem 4.3 once we prove that the orbit map is a
$\mathcal C$
-regular embedding, as below.
Lemma 4.4
Let
$\mathcal C\subset \mathfrak a^+$
be a closed cone such that
$\operatorname{{\rm int}} \mathcal C\supset \mathcal L - \{0\}$
. Then the orbit map
$(\Gamma, \mathsf{d}_{\Gamma}) \to (X, d)$
is
$\mathcal C$
-regular.
Proof. Suppose not. Then there exist two sequences
$\{\gamma_i\}, \{\gamma_i'\} \subset \Gamma$
such that
$\mathsf{d}_{\Gamma}(\gamma_i, \gamma_i')=|\gamma_i^{-1}\gamma_i'| \gt i$
and
$\mu(\gamma_i^{-1} \gamma_i') \not\in \mathcal C$
for all
$i\ge 1$
. Setting
$g_i=\gamma_i^{-1}\gamma_i'\in \Gamma$
, we then have that
${\mu(g_i)}/{\|\mu(g_i)\|} \notin \mathcal C$
for all
$i \ge 1$
. Hence no limit of the sequence
${\mu(g_i)}/{\|\mu(g_i)\|} $
belongs to
$\operatorname{{\rm int}} \mathcal C$
. On the other hand, since
$|g_i|\to \infty$
, we have
$\|\mu(g_i)\|\to \infty$
and hence any limit of the sequence
${\mu(g_i)}/{\|\mu(g_i)\|} $
must belong to the asymptotic cone of
$\mu(\Gamma)$
; that is,
$\mathcal L$
. This yields a contradiction to the hypothesis
$\mathcal L -\{0\} \subset \operatorname{{\rm int}}\mathcal C $
.
The rest of this section is devoted to the proof of Theorem 4.3. We begin by recalling the following theorem; in particular, the metric space Z in Theorem 4.3 is always Gromov hyperbolic.
Theorem 4.5 [Reference Kapovich, Leeb and PortiKLP18, Theorem 1.4]. Let Z and
$ f:Z\to X$
be as in Theorem 4.3. Then Z is Gromov hyperbolic. If Z is proper in addition, then f continuously extends to
where
$\bar Z = Z \cup \partial Z$
is the Gromov compactification and f maps two distinct points in
$\partial Z$
to points in general position.
4.3 Diamonds
The notion of diamonds in X, due to Kapovich, Leeb, and Porti, plays a key role in the proof of Theorem 4.3. We fix
in the following. For a
$\mathcal C$
-regular pair
$(x_1,x_2)$
of points in X, define the
$\mathcal C$
-cone with the tip at
$x_1$
containing
$x_2$
to be
where
$g=g(x_1, x_2) \in G$
is any element such that
$x_1 = go$
and
$x_2 \in g (\exp \mathcal C) o$
; it is easy to check such g always exists and this definition is independent of the choice of g. For any
$h\in G$
, we have
$ hV_{\mathcal C}(x_1,x_2) = V_{\mathcal C}( hx_1, hx_2) $
.
Definition 4.6 (Diamonds) For a
$\mathcal C$
-regular pair
$(x_1,x_2)$
of points in X, the
$\mathcal C$
-diamond with tips at
$x_1$
and
$x_2$
is defined as
The
$\mathcal C$
-cones and
$\mathcal C$
-diamonds are convex subsets of X (see [Reference Kapovich, Leeb and PortiKLP17, Propositions 2.10 and 2.13]). Note also the equivariance property that for
$h\in G$
,
$ h \Diamond_{\mathcal C}(x_1,x_2) = \Diamond_{\mathcal C}(hx_1, hx_2) $
. It follows that for any
$\mathcal C$
-regular pair
$(x_1, x_2)$
, the diamond
$\Diamond_{\mathcal C}(x_1,x_2)$
is of the form
$h \Diamond_{\mathcal C}(o,ao)$
for some
$a\in \exp \mathcal C$
and
$h\in G$
. Therefore, the following example describes all diamonds up to translations.
Example 4.7. For
$a \in \exp \mathcal C$
, the diamond
$\Diamond_{\mathcal C}(o, a o)$
can be explicitly described as follows. First note that as we can take
$g(o, ao) =e$
, we have
$V_{\mathcal C}(o, a o) = M_{\theta}(\exp \mathcal C) o.$
Recalling that
${\rm i}=-\operatorname{{\rm Ad}}_{w_0}$
, we also have
$a o = a w_0 o $
and
$ o = (aw_0) (w_0^{-1} a^{-1} w_0) o \in aw_0 (\exp \mathcal C) o .$
So we can take
$g(ao, o)=aw_0$
. Since
$w_0 M_{\theta} w_0^{-1} = M_{\theta}$
and
$w_0 (\exp \mathcal C) w_0^{-1} = \exp (-\mathcal C)$
, we have
$V_{\mathcal C}(a o, o) = a w_0 M_{\theta} (\exp \mathcal C) o = a M_{\theta} \exp (- \mathcal C) o$
. Therefore,
(see Figure 4.7).
A diamond drawn in
$\mathfrak a$
.

Lemma 4.8 (Simultaneous nesting property) If
$(x_1, x_2)$
is
$\mathcal C$
-regular, then for any
$x \in \Diamond_{\mathcal C}(x_1, x_2)$
, there exist
$g \in G$
and
$a \in \exp \mathcal C$
such that
Proof. We may first assume that
$x_1 = o$
. By the
$\mathcal C$
-regularity of the pair
$(x_1, x_2)$
, we have
$x_2 \in K (\exp \mathcal C) o$
. By multiplying an element of K to
$x_1$
and
$x_2$
, we may also assume that
$x_1 = o$
and
$x_2 \in (\exp \mathcal C) o$
, and hence
$x \in M_{\theta} (\exp \mathcal C) o$
. We again multiply an element of
$M_{\theta}$
to
$x_1, x_2$
, and x if necessary so that we have
$x_1 = o$
,
$x_2 \in M_{\theta}(\exp \mathcal C) o$
, and
$x = ao$
for some
$a \in \exp \mathcal C$
. Then it suffices to show that
$x_2 = a k a' o$
for some
$k \in M_{\theta}$
and
$a' \in \exp \mathcal C$
. We write
$x_2 = m a_0 o$
for
$m \in M_{\theta}$
and
$a_0 \in \exp \mathcal C$
. We then have
$ o \in V_{\mathcal C}(x_2, o) = m a_0 k_0 M_{\theta} (\exp \mathcal C) o$
for some
$k_0 \in K$
. Hence, we have
This implies that
$k_0^{-1} \in M_{\theta} w_0$
and hence
$k_0 \in w_0 M_{\theta}$
. Since
$a o \in V_{\mathcal C}(x_2, o)$
as well, we now have
$a o \in m a_0 w_0 M_{\theta} (\exp \mathcal C) o$
. Then, for some
$k \in K$
, we have
Hence, for some
$a' \in \exp \mathcal C$
, we have
Looking at
$G/P_{\theta}$
, we have
$ k P_{\theta} = a^{-1} m a_0 M_{\theta} a'^{-1} P_{\theta} = P_{\theta}$
. Therefore,
$k \in M_{\theta}$
. Since
$x_2 = m a_0 o = aka' o$
, the claim follows.
Lemma 4.9.
For any
$\mathcal C$
-regular pair
$(g_1 o, g_2 o)$
with
$g_1, g_2\in G$
and for any
$ go \in \Diamond_{\mathcal C}(g_1 o, g_2 o)$
with
$g\in G$
,
Proof. By Lemma 4.8, there exists
$h\in G$
,
$a, \tilde{a}, a' \in \exp \mathcal C$
and
$\tilde{k}, k \in M_\theta $
such that
$g_1o=ho$
,
$go=hao$
, and
$g_2o= h \tilde{k} \tilde{a} o = ha k a'o$
. Without loss of generality, we may assume that
$h=e$
in proving (4.2).
We write
We then have
Since
$a_2 k a_2' \in S_{\theta}$
, we can write its Cartan decomposition
$a_2 k a_2' = m b m' \in M_{\theta}B_{\theta}^+M_{\theta}$
, and hence
Let
$w \in \mathcal W$
be a Weyl element such that
$b a_1 a_1' \in w A^+ w^{-1}$
. Since
$\tilde{a} = \exp \mu(aka')$
, we must have
$b a_1 a_1' = w \tilde{a} w^{-1}$
. Hence we have
On the other hand, we also have
$g_2 o = \tilde{k} \tilde{a} o,$
where
$\tilde{k} \in M_{\theta}$
. This implies that
$mw \in M_{\theta}$
; and, in particular,
$w \in M_{\theta}$
. Therefore
$\tilde{a} = w^{-1} b a_1 a_1' w = (w^{-1} b w)(a_1 a_1') \in B_{\theta}A_{\theta}^+$
, which implies that
Since
this finishes the proof.
As an immediate corollary, we obtain that
$\mathsf{d}_{\psi}$
is additive on each diamond for any
$\psi\in \mathfrak a_\theta^*$
.
Lemma 4.10 (Additivity of
$\mathsf{d}_\psi$
on diamonds) Let
$\psi \in \mathfrak a_{\theta}^*$
. For any
$\mathcal C$
-regular pair
$(x_1, x_2)$
and for any
$x\in \Diamond_{\mathcal C}(x_1, x_2)$
, we have
4.4 KLP Morse lemma
The Morse lemma due to Kapovich, Leeb, and Porti, which we will call the KLP Morse lemma, is stated as follows [Reference Kapovich, Leeb and PortiKLP18, Theorem 5.16, Corollary 5.28]: the image of an interval in
$\mathbb R $
under a Q-quasi-isometry is called a Q-quasi-geodesic.
Theorem 4.11 (KLP Morse lemma) Let
$\mathcal C,\mathcal C' \subset \mathfrak a^+$
be
$\theta$
-admissible closed cones such that
$\operatorname{{\rm int}} \mathcal C'$
contains
$ \mathcal C-\{0\}$
(see Figure 2). Let
$Q, B\ge 1$
be constants. There exists a constant
$D_0 = D_0(\mathcal C,\mathcal C', Q, B) \ge 0$
so that the following holds: let
$I \subset \mathbb R$
be an interval and
$c : I \to X$
a
$(\mathcal C, B)$
-regular Q-quasi-geodesic.
The choice of
$\mathcal C'$
viewed on the unit sphere of
$\mathfrak a^+$
.

-
(1) If
$I = [a, b]$
with
$b - a \ge B$
, then the image c(I) is contained in the
$D_0$
-neighborhood of the diamond
$\Diamond_{\mathcal C'}(c(a),c(b))$
. -
(2) If
$I = [a, \infty)$
for some
$a \in \mathbb R$
, then c(I) is contained in the
$D_0$
-neighborhood of the cone
$g M_{\theta}(\exp \mathcal C') o,$
where
$g \in G$
is such that
$g o = c(a)$
and
$g^+ = c(\infty) \in \mathcal F_{\theta}$
. -
(3) If
$I = \mathbb R$
, then c(I) is contained in the
$D_0$
-neighborhood of the parallel set
$g M_{\theta} A o,$
where
$g \in G$
is such that
$g^{\pm} = c(\pm \infty) \in \mathcal F_{\theta}$
.
We note that the above applies for an interval in
$\mathbb Z$
, as any
$\mathcal C$
-regular quasi-isometric embedding
$c:I\cap \mathbb Z \to X$
can be extended to a
$\mathcal C$
-regular quasi-geodesic
$I\to X$
simply by setting
$c(t) := c( \lfloor t \rfloor)$
where
$\lfloor t \rfloor$
is the largest integer not bigger than t.
As an application of Theorem 4.11, we obtain the following.
Corollary 4.12
Given
$\mathcal C, \mathcal C', Q, B\ge 1$
as in Theorem 4.11 and
$\psi\in \mathfrak a_\theta^*$
, there exists a constant
$D_1 = D_1(\mathcal C,\mathcal C', Q, B,\psi) \ge 0$
so that the following holds: let
$I \subset \mathbb R$
be an interval and
$c : I \to X$
a
$(\mathcal C, B)$
-regular Q-quasi-geodesic. Then, for all
$a \le t \le b$
in I, we have
Proof. Suppose that
$b - a \ge B$
. Since c is
$(\mathcal C, B)$
-regular, the pair (c(a), c(b)) is
$\mathcal C$
-regular. Applying Theorem 4.11, we obtain that the image of
$ c : [a,b] \to X$
lies in the
$D_0$
-neighborhood of
$\Diamond_{\mathcal C'}(c(a), c(b))$
. For each
$a \lt t \lt b$
, choose
$x_t\in \Diamond_{\mathcal C'}(c(a), c(b))$
so that
$d(x_t, c(t)) \le D_0$
. Hence, by Lemma 4.10,
For each
$a \le t \le b$
, write
$c(t)=g_t o$
and
$x_t=h_t o$
for
$g_t, h_t\in G$
. We then have
$\| \mu(h_t^{-1} g_t)\|\le D_0$
. By applying Lemma 2.1 to a compact subset
$\{g \in G : \|\mu(g)\|\le D_0\}$
, we have, for all
$a\lt t\lt b$
,
where
$C\gt 0$
is a uniform constant depending only on
$\psi$
and
$D_0$
. Similarly, we have
$|\mathsf{d}_\psi (x_t, c(b)) - \mathsf{d}_\psi (c(t), c(b)) |\le C $
. By (4.5), this implies that
Setting
$D_1= 2C + 3 \|\psi\|(QB + Q)$
, where
$\|\psi\|$
is the operator norm of
$\psi$
, we have shown that (4.4) holds whenever
$b-a\ge B$
. If
$b - a \lt B$
, then the image of c([a, b]) has diameter smaller than
$Q(b-a) + Q \lt QB + Q$
. Then,
for all
$t_1, t_2 \in [a, b]$
, and hence the left-hand side of (4.4) is bounded above by
$ 3\|\psi\| (QB + Q)\le D_1$
. This completes the proof.
We are ready to give the following proof.
4.5 Proof of Theorem 4.3
Let
$f : Z \to X$
be as in Theorem 4.3. Let
$\psi \in \mathfrak a_{\theta}^*$
be such that
$\psi \gt 0$
on
$ \mathcal C - \{0\}$
. Choose a
$\theta$
-admissible cone
$\mathcal C' \subset \mathfrak a^+$
such that
$\operatorname{{\rm int}} \mathcal C'$
contains
$\mathcal C-\{0\}$
and such that
$\psi\gt 0$
on
$\mathcal C'-\{0\}$
. Let
$x_1, x_2, x_3 \in f(Z)$
be a triple of distinct points. We choose
$z_1, z_2, z_3 \in Z$
such that
$x_i = f(z_i)$
for
$i = 1,2, 3$
. Choose geodesics
$c_1$
and
$c_2$
in Z connecting
$z_1$
to
$z_2$
and
$z_2$
to
$z_3$
, respectively. By Theorem 4.5,
$(Z, d_Z)$
is Gromov hyperbolic. We denote by z the nearest-point projection of
$z_2$
to a geodesic segment connecting
$z_1$
and
$z_3$
. Then, by the Gromov hyperbolicity of
$(Z, d_Z)$
, there exists a uniform constant
$\delta \gt 0$
so that the
$\delta$
-neighborhood of z intersects both geodesics
$c_1$
and
$c_2$
. We choose two points
$y_1 \in c_1$
and
$y_2 \in c_2$
that are
$\delta$
-close to z. We concatenate the segment of
$c_1$
connecting
$z_1$
and
$y_1$
, a geodesic connecting
$y_1$
and
$y_2$
, and the segment of
$c_2$
connecting
$y_2$
and
$z_3$
, and denote the concatenated path by c. We can parameterize
$c : [0, b] \to Z$
so that c is a q-quasi-geodesic for some
$b \gt 0$
and uniform
$q \ge 1$
by the Gromov hyperbolicity of
$(Z, d_Z)$
and the choice of
$y_1$
and
$y_2$
.
Since f is a
$\mathcal C$
-regular quasi-isometric embedding, so is
$f \circ c$
. Hence, we obtain
where
$D_1$
is the constant given by Corollary 4.12. Applying Corollary 4.12 to the restriction of
$f \circ c$
to the interval
$[c^{-1}(y_1), b]$
again, we have
Since
$d_Z(y_1, y_2) \le 2 \delta$
, combining (4.6) and (4.7) yields
where
$D_1':= \sup \{\mathsf{d}_\psi(f(w_1), f(w_2)) :{d_Z(w_1, w_2) \le 2 \delta} \} + 2 D_1\lt \infty $
.
Since f is
$\mathcal C$
-regular and
$\psi \gt 0$
on
$\mathcal C - \{0\}$
, there exists
$D_2 \gt 0$
such that
for all
$w_1, w_2 \in Z$
; indeed, if f is
$(\mathcal C, B)$
-regular for some
$B\ge0$
, then
$\mathsf{d}_{\psi}(f(w_1), f(w_2)) \ge 0$
whenever
$d_Z(w_1, w_2)\ge B$
, and
$\sup \{|\mathsf{d}_\psi (f(w_1), f(w_2))| :d_Z(w_1, w_2)\lt B\} $
is bounded by a uniform constant depending only on B, the quasi-isometry constant of f, and
$\|\psi\|$
.
Hence, applying (4.9) and Corollary 4.12 to
$f ( c_1 )$
, we have
Similarly, we also obtain
Combining (4.8), (4.10), and (4.11), we obtain
This completes the proof of Theorem 4.3.
We state the following consequence of the KLP Morse lemma applied to Anosov subgroups.
Theorem 4.13 (Morse lemma for Anosov subgroups) Let
$\theta={\rm i}(\theta)$
. Let
$\Gamma$
be a
$\theta$
-Anosov subgroup and let
$f : \Gamma \cup \partial \Gamma \to \Gamma o \cup \Lambda_{\theta}$
be the extension of the orbit map
$\gamma \mapsto \gamma o$
given in Theorem 3.8(4). Then there exist a cone
$\mathcal C \subset \mathfrak a^+$
and constants
$B, D_0 \ge 1$
such that for any geodesic
$[\xi, \eta]$
in
$\Gamma$
, the following hold.
-
(1) If
$\xi, \eta \in \Gamma$
and
$\mathsf{d}_{\Gamma}(\xi, \eta) \ge B$
, then
$f([\xi, \eta])$
is contained in the
$D_0$
-neighborhood of the diamond
$\Diamond_{\mathcal C}(f(\xi), f(\eta))$
. -
(2) If
$\xi \in \Gamma$
and
$\eta \in \partial \Gamma$
, then
$f([\xi, \eta])$
is contained in the
$D_0$
-neighborhood of
$g M_{\theta} (\exp \mathcal C) o$
, where
$g \in G$
is such that
$g o = \xi$
and
$g P_{\theta} = f(\eta)$
. -
(3) If
$\xi, \eta \in \partial \Gamma$
, then
$f([\xi, \eta])$
is contained in the
$D_0$
-neighborhood of
$g M_{\theta} A o$
, where
$g \in G$
is such that
$g P_{\theta} = f(\xi)$
and
$g w_0 P_{\theta} = f(\eta)$
.
Moreover, the cone
$\mathcal C$
can be taken arbitrarily close to
$\mathcal L$
as long as its interior contains
$\mathcal L - \{0\}$
.
Proof. Let
$\mathcal C\subset \mathfrak a^+$
be the
$\theta$
-admissible cone as in the proof of Theorem 4.1, and choose a
$\theta$
-admissible cone
$\mathcal C' \subset \mathfrak a^+$
whose interior in
$\mathfrak a^+$
contains
$\mathcal C-\{0\}$
. Then, by Lemma 4.4 and Theorem 3.8(3), the orbit map
$f|_{\Gamma}$
is a
$(\mathcal C, B) $
-regular Q-quasi-isometry between
$(\Gamma, \mathsf{d}_\Gamma)$
and
$(\Gamma o, d)$
for some
$B, Q\ge 1$
. Let
$D_0=D_0(\mathcal C, \mathcal C', Q, B)$
be as given by Theorem 4.11.
Now note that any geodesic
$[\xi,\eta]$
in
$(\Gamma, \mathsf{d}_\Gamma)$
can be written as
$[\xi, \eta]=\{\gamma_i:i\in I\}$
for an interval I in
$\mathbb Z$
, and
$\iota: i\mapsto \gamma_i$
is an isometry between I and
$[\xi, \eta]$
. Since
$c:=f \circ \iota $
is a
$(\mathcal C, B)$
-regular Q-quasi-geodesic, we can apply Theorem 4.11, which implies the above claims (1)–(3), where the cone
$\mathcal C$
in the statement is given by
$\mathcal C'$
in this proof. Note from the proof of Theorem 4.1 that the cone
$\mathcal C'$
can be taken arbitrarily close to the limit cone
$\mathcal L$
of
$\Gamma$
as long as
$\operatorname{{\rm int}} \mathcal C'$
contains
$\mathcal L - \{0\}$
.
5. Conformal premetrics on limit sets
Let
$\Gamma$
be a
$\theta$
-Anosov subgroup of a connected semisimple real algebraic group G. We assume that
$\theta = {\rm i}(\theta)$
in this section. Fix a linear form
$\psi \in \mathfrak a_\theta^*$
positive on
$\mathcal L_{\theta} - \{0\}$
. The goal of this section is to define a premetric
$d_\psi$
on the limit set
$\Lambda_\theta$
, which is conformal, almost symmetric and satisfies almost triangle inequality with bounded multiplicative error. We also discuss how this definition can be extended to non-symmetric
$\theta$
at the end of the section.
Recall the definition of the Gromov product from Definition 2.3. The
$\theta$
-Anosov property of
$\Gamma$
implies that any two distinct points in
$\Lambda_\theta$
are in general position: if
$\xi\ne \eta$
in
$\Lambda_\theta$
, then
$(\xi, \eta)\in \mathcal F_\theta^{(2)}$
. Therefore, the following premetric on
$\Lambda_\theta$
is well-defined.
Definition 5.1.
For
$\xi, \eta \in \Lambda_{\theta}$
, we set
\begin{equation}d_{\psi}(\xi, \eta) =\begin{cases}e^{-\psi( \mathcal G^{\theta}(\xi, \eta))} & \text{if } \xi \neq \eta,\\0 &\text {if } \xi = \eta.\end{cases} \end{equation}
We first observe the following
$\Gamma$
-conformal property of
$d_\psi$
.
Lemma 5.2.
For
$\gamma \in \Gamma$
and
$\xi, \eta \in \Lambda_{\theta}$
, we have
Proof. Let
$\xi \neq \eta$
, and
$g \in G$
be such that
$g^+ = \xi$
and
$g^- = \eta$
. Then, for any
$\gamma\in \Gamma$
,
$$\begin{aligned} 2 \mathcal G^{\theta}(\gamma^{-1} \xi, \gamma^{-1} \eta) & = \beta_{\gamma^{-1} \xi}^{\theta}(e, \gamma^{-1} g ) + {\rm i}(\beta_{\gamma^{-1} \eta}^{\theta}(e, \gamma^{-1} g )) \\ & = 2 \mathcal G^{\theta}(\xi, \eta) +\beta_{\xi}^{\theta}(\gamma , e) + {\rm i}(\beta_{\eta}^{\theta}(\gamma , e)) \\ & = 2 \mathcal G^{\theta}(\xi, \eta) - \beta_{\xi}^{\theta}(e, \gamma) - {\rm i}(\beta_{\eta}^{\theta}(e, \gamma)). \end{aligned}$$
The claim now follows from the definition of
$d_{\psi}$
.
Recall that
$\mathcal G^{\theta}(\xi, \eta)={\rm i} (\mathcal G^{\theta}( \eta,\xi))$
for all
$\xi,\eta\in \Lambda_\theta$
. Hence if
$\psi$
is i-invariant, then
$d_\psi$
is symmetric. We have the following in general.
Proposition 5.3 (Metric-like properties of
$d_\psi$
)
-
(1) There exists
$R=R(\psi)\gt 1$
such that for all
$\xi, \eta \in \Lambda_{\theta}$
,
$$R^{-1} d_\psi(\eta,\xi)\le d_\psi(\xi, \eta) \le R\; d_\psi (\eta, \xi) .$$
-
(2) There exists
$N=N(\psi) \gt 0$
such that for all
$\xi_1, \xi_2, \xi_3 \in \Lambda_{\theta}$
,
$$d_{\psi}(\xi_1, \xi_3) \le N (d_{\psi}(\xi_1, \xi_2) + d_{\psi}(\xi_2, \xi_3)).$$
The second property was obtained in [Reference Lee and OhLO23, Lemma 6.11] and the same proof can be repeated for a general
$\theta$
in verbatim. The first property follows from Lemma 5.4 below. For
$x\ne y$
in the Gromov boundary
$\partial \Gamma$
and a bi-infinite geodesic [x, y] in
$\Gamma$
, we denote by
$\gamma_{x, y} \in [x, y]$
the nearest-point projection of the identity e to [x,y] in
$(\Gamma, \mathsf{d}_\Gamma)$
; that is,
$\gamma_{x, y} \in [x, y]$
is an element such that
$\mathsf{d}_\Gamma (e, \gamma_{x,y})=\inf\{\mathsf{d}_\Gamma (e, g):g\in [x,y]\}$
, which is coarsely well-defined. Recall the map
$f : \Gamma \cup \partial \Gamma \to \Gamma o \cup \Lambda_{\theta}$
from Theorem 3.8(4). The following was proved in [Reference Lee and OhLO23, Lemma 6.6] for
$\theta=\Pi$
and the same proof works for a general
$\theta$
.
Lemma 5.4
There exists
$C_1 \gt 0$
such that for any
$x \neq y \in \partial \Gamma$
,
In particular, for
$\xi \neq \eta \in \Lambda_{\theta}$
, we have
5.1 Symmetrization
Consider the following symmetrization of
$\psi\in \mathfrak a_\theta^*$
:
Since we are assuming that
$\theta={\rm i}(\theta)$
, we have
$\bar\psi\in \mathfrak a_\theta^*$
as well. Since
$\mathcal L_{\theta}$
is i-invariant, we have
$\bar \psi \gt 0$
on
$\mathcal L_{\theta} - \{0\}$
. Lemma 5.4 implies that
$d_{\bar \psi}$
and
$d_{\psi}$
are Lipschitz equivalent.
Proposition 5.5.
There exists
$R \ge 1$
such that for any
$\xi, \eta \in \Lambda_{\theta}$
, we have
Proof. Since
$\mathcal G^{\theta}(\eta, \xi) = {\rm i} ( \mathcal G^{\theta}(\xi, \eta))$
for all
$\eta \ne \xi$
in
$\Lambda_\theta$
, it follows from Lemma 5.4 with the constant
$C_1$
therein that
It suffices to set
$R = e^{\|\psi\| C_1}$
to finish the proof.
We also record the following Vitali covering type lemma, which is a standard consequence of Proposition 5.3(2) (cf. [Reference Lee and OhLO23]): here,
$B_\psi(\xi, r)=\{\eta\in \Lambda_\theta: d_\psi(\xi, \eta)\lt r\}$
.
Lemma 5.6 [Reference Lee and OhLO23, Lemma 6.12]. There exists
$N_0 = N_0(\psi) \ge 1$
satisfying the following: for any finite collection
$B_{\psi}(\xi_1, r_1), \ldots, B_{\psi}(\xi_n, r_n)$
with
$\xi_i \in \Lambda_{\theta}$
and
$r_i \gt 0$
for
$i = 1, \ldots, n$
, there exists a disjoint subcollection
$B_{\psi}(\xi_{i_1}, r_{i_1}), \ldots, B_{\psi}(\xi_{i_k}, r_{i_k})$
such that
$$\bigcup_{i = 1}^n B_{\psi}(\xi_i, r_i) \subset \bigcup_{j = 1}^k B_{\psi}(\xi_{i_j}, N_0 r_{i_j}).$$
Remark 5.7. Recall that the canonical projection
$p : \Lambda_{\theta \cup {\rm i}(\theta)} \to \Lambda_{\theta}$
is a
$\Gamma$
-equivariant homeomorphism and that
$\mathfrak a_\theta^*\subset \mathfrak a_{\theta\cup {\rm i}(\theta)}^*$
. Using this homeomorphism, we can also define a function
$d_{\psi}$
on
$\Lambda_{\theta}$
even when
$\theta$
is not symmetric, so that
$p : (\Lambda_{\theta \cup {\rm i}(\theta)}, d_{\psi}) \to (\Lambda_{\theta}, d_\psi)$
is an isometry:
for all
$\xi, \eta \in \Lambda_{\theta}$
. In this regard, the above discussion is still valid without the symmetric hypothesis on
$\theta$
.
6. Compatibility of shadows and
$d_{\psi}$
-balls
As before, let
$\Gamma$
be a
$\theta$
-Anosov subgroup of a connected semisimple real algebraic group G. We fix a word metric
$\mathsf{d}_{\Gamma}$
on
$\Gamma$
. Fix a linear form
that is positive on
$\mathcal L - \{0\}$
and
$\psi = \psi \circ {\rm i}$
. Recall the premetric
$\mathsf{d}_\psi$
on
$\Gamma o$
defined in (4.1) and the conformal premetric
$d_\psi$
on
$\Lambda_\theta$
defined by (5.1).
Lemma 6.1.
Both
$(\Gamma o, \mathsf{d}_\psi)$
and
$(\Lambda_\theta, d_\psi)$
are symmetric.
Proof. For
$g_1, g_2\in G$
, we have
The second claim follows similarly, since
$\mathcal G^{\theta \cup {\rm i}(\theta)}(\xi, \eta)= {\rm i} \mathcal G^{\theta \cup {\rm i}(\theta)}(\eta, \xi)$
for all
$\xi, \eta\in \mathcal F_{\theta \cup {\rm i}(\theta)}$
in general position.
Shadows play a basic role in studying the metric property of
$(\Lambda_\theta, d_\psi)$
in relation with the geometry of the symmetric space X, as in the original work of Sullivan. We recall the definition of shadows in
$\mathcal F_{\theta}$
. For
$p, q \in X$
, the shadow
$O_R^{\theta}(p, q)$
of the Riemannian ball B(q, R) viewed from p is defined as
For the basic properties of these shadows, we refer to [Reference Kim, Oh and WangKOW25a] and [Reference Kim, Oh and WangKOW25b].
The main technical ingredient of this paper is the following theorem, which says that shadows in
$\Lambda_\theta$
are comparable with
$d_{\psi}$
-balls.
Theorem 6.2.
Let
$\psi \in \mathfrak a_{\theta}^*$
be such that
$\psi \gt 0$
on
$\mathcal L- \{0\}$
and
$\psi = \psi \circ {\rm i}$
. Then there exist constants
$c, R_0 \gt 0$
such that for any
$R \gt R_0$
, there exists
$c' = c'_R \gt 0$
so that the following holds: for any
$\xi \in \Lambda_{\theta}$
and any
$g \in \Gamma$
on a geodesic ray
$[e,\xi]$
in
$\Gamma$
, we have
Since the proof of this theorem is quite lengthy, we will prove the first inclusion in this section and the second inclusion in the next section. The rest of this section is devoted to the proof of the first inclusion. In view of Remark 5.7, we assume that
Strictly speaking,
$\mathsf{d}_\psi$
is not a metric on the
$\Gamma$
-orbit
$\Gamma o$
. Nevertheless, we still employ terminologies for the metric space on
$(\Gamma o, \mathsf{d}_\psi)$
for convenience. For instance, for a subset
$B\subset \Gamma o$
,
$\mathsf{d}_\psi( g o, B)= \inf_{ho\in B} \mathsf{d}_\psi (go, ho)$
and the R-neighborhood of B is given by
$\{go\in \Gamma o: \mathsf{d}_\psi( g o, B)\lt R\}$
, etc.
Two main ingredients of the proof of the first inclusion of (6.1) are the following, which allow us to treat
$(\Gamma o, \mathsf{d}_\psi) $
almost like a Gromov hyperbolic space:
-
(1)
$(\Gamma o, \mathsf{d}_\psi)$
satisfies a triangle inequality up to an additive error (Theorem 4.1); and -
(2) the
$\psi$
-Gromov product
$\psi(\mathcal G(\xi, \eta))$
is equal to the premetric
$\mathsf{d}_\psi (o, [\xi, \eta] o)$
up to an additive error (Proposition 6.7).
In the rank-one case, property (2) is a well-known consequence of a uniform thin-triangle property and the Morse lemma of the rank-one symmetric space. Higher-rank symmetric spaces have neither of these properties. Our proof of property (2) is based on the KLP Morse lemma using diamonds as well as a uniform thin-triangle property of the orbit
$(\Gamma o, \mathsf{d}_{\psi})$
.
We begin with the following.
Proposition 6.3.
The orbit map
$(\Gamma, \mathsf{d}_{\Gamma}) \to (\Gamma o, \mathsf{d}_{\psi})$
,
$\gamma \mapsto \gamma o$
, is a quasi-isometry, i.e., there exists
$Q_{\psi} \ge 1$
such that for any
$\gamma_1, \gamma_2 \in \Gamma$
,
In particular, the images of geodesic triangles in
$\Gamma$
under the orbit map are uniformly thin; that is, there exists
$T_{\psi}\gt 0$
such that for any
$\xi_1, \xi_2, \xi_3 \in \Gamma \cup \partial \Gamma$
, the image
$[\xi_1, \xi_{3}]o$
is contained in the
$T_{\psi}$
-neighborhood of
$([\xi_1, \xi_2] \cup [\xi_2, \xi_3])o$
with respect to
$\mathsf{d}_{\psi}$
.
Proof. The second part follows since
$(\Gamma,\mathsf{d}_\Gamma)$
is a Gromov hyperbolic space (Theorem 3.8(1)), and hence it has a uniform thin-triangle property that is a quasi-isometry invariance. Since the orbit map
$(\Gamma, \mathsf{d}_{\Gamma}) \to (\Gamma o, d)$
is a quasi-isometry (Theorem 3.8(3)), the first part of the above proposition follows from the following claim that the identity map
$(\Gamma o, d)\to (\Gamma o, \mathsf{d}_\psi)$
is a quasi-isometry: there exists
$C_\psi\ge 1$
such that for all
$\gamma_1, \gamma_2 \in \Gamma$
, we have
We can take a cone
$\mathcal C$
whose relative interior in
$\mathfrak a^+$
contains
$\mathcal L - \{0\}$
in
$\mathfrak a^+$
such that
$\psi \gt 0$
on
$\mathcal C - \{0\}$
. Hence, we can choose
$C_1\gt 1$
so that
On the other hand,
$\mu(\gamma) \in \mathcal C$
for all but finitely many
$\gamma \in \Gamma$
(Lemma 4.4), and hence
$C_2:=\max\{| \psi (\mu(\gamma))|:\mu(\gamma)\notin \mathcal C\}\lt \infty$
. If we set
$C=C_1+C_2$
, then
Since both d and
$\mathsf{d}_\psi$
are left
$\Gamma$
-invariant, this implies the claim.
We use the Morse property to obtain that the image of a geodesic ray under the orbit map has a uniform progression.
Lemma 6.4 (Uniform progression lemma) For any
$r\gt 0$
, there exists
$n_r\gt 0$
such that for any geodesic ray
$\{\gamma_0 = e,\gamma_1,\gamma_2, \ldots\}$
in
$(\Gamma,\mathsf{d}_\Gamma)$
,
for all
$i\in \mathbb N$
and all
$n\ge n_r$
.
Proof. Fix
$r\gt 0$
. By Theorem 4.13, there exist a cone
$\mathcal C \subset \mathfrak a^+$
and
$B, D_0 \ge 0$
so that for all
$n \ge B$
and
$i \ge 0$
, the sequence
$o, \gamma_1 o, \ldots, \gamma_{i+n} o$
is contained in the
$D_0$
-neighborhood of the diamond
$\Diamond_{\mathcal C}( o,\gamma_{i+n} o)$
in (X, d). We may also assume that
$\psi \gt 0$
on
$\mathcal C - \{0\}$
as
$\mathcal C$
can be arbitrarily close to
$\mathcal L$
. For each
$i \ge 0$
, choose a point
$x_i \in \Diamond_{\mathcal C}(o, \gamma_{i + n} o)$
that is
$D_0$
-close to
$\gamma_i o$
. Applying Lemma 4.10, we obtain that
Since the orbit map
$(\Gamma, \mathsf{d}_\Gamma)\to (\Gamma o, d)$
is a
$Q_{\psi}$
-quasi-isometry by Proposition 6.3, we obtain that for all
$i \ge 0$
,
By applying Lemma 2.1 to a compact subset
$\{g\in G: \|\mu(g)\| \le D_0\}$
, we have
where C depends only on
$D_0$
and
$\|\psi\|$
. Putting (6.3), (6.4), and (6.5) together, we obtain
\begin{align*} \mathsf{d}_\psi( o, \gamma_{i+n} o) &= \mathsf{d}_\psi( o, x_i)+ \mathsf{d}_\psi(x_i, \gamma_{i+n} o)\\ &\ge \mathsf{d}_\psi( o, \gamma_i o) + \mathsf{d}_\psi( \gamma_i o, \gamma_{i+n} o) - 2 C \\ &\ge \mathsf{d}_\psi( o, \gamma_i o) + (Q_{\psi}^{-1}n -Q_{\psi}) - 2 C . \end{align*}
Hence, setting
$n_r = B + Q_{\psi}(r + 2 C + Q_{\psi})$
finishes the proof.
Lemma 6.5 (Small inscribed triangle) There exists
$C \gt 0$
satisfying the following property: Let
$[\xi, \eta]$
be a bi-infinite geodesic in
$(\Gamma, \mathsf{d}_{\Gamma})$
. If
$\gamma o $
is the nearest-point projection of o to
$[\xi, \eta] o$
in the
$\mathsf{d}_\psi$
-metric, i.e.,
$\gamma \in [\xi, \eta]$
is such that
$\mathsf{d}_{\psi}(o, \gamma o) = \mathsf{d}_{\psi}(o, [\xi, \eta]o)$
, then there exist
$u \in [e, \xi]$
and
$v \in [e, \eta]$
so that
$\{uo, v o, \gamma o\}$
has
$\mathsf{d}_\psi$
-diameter less than C (see Figure 3
).
A small inscribed triangle.

Proof. Recall from Proposition 6.3 that there exists
$T_\psi \gt 0$
so that every triangle in
$\Gamma o$
, obtained as the image of a geodesic triangle in
$(\Gamma, \mathsf{d}_{\Gamma})$
under the orbit map, is
$T_{\psi}$
-thin in the
$\mathsf{d}_\psi$
-metric. By the
$T_{\psi}$
-thinness of
$(\Gamma o, \mathsf{d}_\psi)$
, we have either
$\mathsf{d}_{\psi} (\gamma o, [e, \xi] o)\le T_{\psi}$
or
$\mathsf{d}_{\psi} (\gamma o, [e, \eta] o) \le T_{\psi}$
. We assume the latter case; the other case can be treated similarly. We write
$[e, \eta] = \{v_i\}_{i \ge 0}$
. We then can choose j so that
$j = \min \{i \ge 0: \mathsf{d}_\psi( \gamma o, v_io)\le T_{\psi} + D\}$
where D is given in Theorem 4.1. Let
$n' = n_{3 T_{\psi} {+3D}}$
be the constant from Lemma 6.4. If
$j\lt n'$
, then we set
$u=v=e$
and note that
where
$Q_\psi$
is given by Proposition 6.3. Hence the triangle
$\{uo, vo, \gamma o\}=\{o, o, \gamma o\}$
has
$\mathsf{d}_\psi$
-diameter at most
$D_1$
.
Now suppose that
$j\gt n'$
. We claim that
Indeed, otherwise,
$\mathsf{d}_\psi(v_{j - n'}o, \gamma'o) \le T_{\psi}$
for some
$\gamma' \in [\xi, \eta]$
, and hence we have
$$\begin{aligned} \mathsf{d}_{\psi}(o, \gamma' o) & \le \mathsf{d}_{\psi}(o, v_{j - n'} o) + \mathsf{d}_{\psi}( v_{j - n'} o, \gamma' o) {+ D} \\ & \le (\mathsf{d}_{\psi}(o, v_{j} o) - 3 T_{\psi} {- 3 D}) + T_{\psi} {+ D}\\ & = \mathsf{d}_{\psi}(o, v_{j} o) - 2 T_{\psi} {-2 D}\\ & \le \mathsf{d}_{\psi}(o, v_{j} o) - {\mathsf{d}_{\psi}(\gamma o, v_{j}o)} - T_{\psi} {- D}\\ & \le \mathsf{d}_{\psi}(o, \gamma o) - T_{\psi},\end{aligned}$$
where the first and the last inequalities follow from Theorem 4.1 and the second is from Lemma 6.4. This yields a contradiction to the minimality of
$\mathsf{d}_{\psi}(o, \gamma o)$
, proving the claim.
Since the triangle consisting of the sides
$[\xi, \eta]o$
,
$[e, \xi]o$
, and
$[e, \eta] o = \{v_i o\}_{i \ge 0}$
is
$T_{\psi}$
-thin, the above claim implies that
$v_{j - n'} o$
lies in the
$T_{\psi}$
-neighborhood of
$[e, \xi] o$
. Hence, there exists
$u \in [e, \xi]$
such that
$\mathsf{d}_\psi(v_{j-n'} o, u o)\le T_{\psi}$
(see Figure 4). Since
$\mathsf{d}_{\psi}(v_j, v_{j - n'}) \le Q_{\psi} n' + Q_{\psi}$
, we have so far obtained:
-
–
$\mathsf{d}_{\psi}(\gamma o, v_j o) \le T_\psi + D $
; -
–
$\mathsf{d}_{\psi}(v_j o, u o) \le Q_{\psi} n' + Q_{\psi} + T_{\psi} + D$
; and -
–
$\mathsf{d}_{\psi}(\gamma o, u o) \le Q_{\psi} n' + Q_{\psi} + 2T_{\psi} + 3D$
.
The choice of
$\gamma o$
,
$v_j o$
,
$v_{j-n'} o$
and
$u_k o$
.

Therefore, the triangle
$\{uo, v_j o, \gamma o\}$
has
$\mathsf{d}_\psi$
-diameter at most
$D_2 = Q_{\psi} n' + Q_{\psi} + 2T_{\psi} + 3D$
. It remains to set
$C=\max (D_1, D_2)$
.
The following has been shown for
$\theta = \Pi$
in [Reference Lee and OhLO23, Lemma 5.7], which directly implies the statement for general
$\theta$
.
Lemma 6.6.
There exists
$\kappa \gt 0$
such that for any
$g, h \in G$
and
$R\gt 0$
, we have
We now prove that the
$\psi$
-Gromov product
$\psi(\mathcal G(\xi, \eta))$
behaves like the distance
$\mathsf{d}_\psi (o, [\xi, \eta] o)$
up to an additive error.
Proposition 6.7 (Comparison between
$\psi$
-Gromov product and
$\mathsf{d}_{\psi}$
-distance) There exists
$C_1 \gt 0$
such that for any
$\xi\ne \eta \in \Lambda_{\theta}=\partial \Gamma$
, we have
Proof. Let
$\gamma\in [\xi, \eta]$
be such that
$\mathsf{d}_{\psi}(o, \gamma o) = \mathsf{d}_{\psi}(o, [\xi, \eta] o)$
. Consider geodesic rays
$[e, \xi] $
and
$[e, \eta] $
in
$(\Gamma, \mathsf{d}_\Gamma)$
. Let
$k, \ell \in K$
and
$h \in G$
be such that
$kP_{\theta} = \xi$
,
$\ell P_{\theta} = \eta$
,
$h P_{\theta}=\xi$
and
$h w_0 P_{\theta} = \eta$
. For the constant
$D_0$
given by Theorem 4.13, we have
\begin{equation} \begin{aligned} \sup_{u \in [e, \xi]} d(u o, kM_{\theta}A^+ o) &\le D_0; \\ \sup_{v \in [e, \eta]} d(v o, \ell M_{\theta}A^+ o) &\le D_0; \\ \sup_{g \in [\xi, \eta]} d (g o, hM_{\theta} A o) &\le D_0. \end{aligned} \end{equation}
Since
$\gamma\in [\xi, \eta]$
by the choice, the third inequality implies that
$d (\gamma o, hM_\theta A o) \le D_0$
. We may assume that h satisfies that
$d(h o, \gamma o) \le D_0$
, by replacing h with an element of
$hM_{\theta}A$
if necessary.
We first claim that for some uniform
$R \gt 0$
depending only on
$\Gamma$
and
$\psi$
,
To show the claim, let
$C \gt 0$
be the constant given by Lemma 6.5 and choose
$u \in [e, \xi]$
and
$v \in [e, \eta]$
so that the triangle
$\{u o, v o, \gamma o\}$
has
$\mathsf{d}_{\psi}$
-diameter smaller than C (see Figure 5). Hence, for the constant
$C' := C_{\psi}(C + C_{\psi})$
, where
$C_{\psi}$
is given in (6.2), the Riemannian diameter of the triangle
$\{u o, v o, \gamma o\}$
is less than C’. It then follows from the first two inequalities of (6.7) that
Since
$k P_{\theta} = \xi$
and
$\ell P_{\theta} = \eta$
, we have
showing the claim with
$R = D_0 + C'$
Therefore, by Lemma 6.6, we obtain
Since
$\beta_{\xi}^{\theta}(o, \gamma o) = \beta_{\xi}^{\theta}(o, ho) + \beta_{\xi}^{\theta}(ho, \gamma o)$
and
$\|\beta_{\xi}^{\theta}(ho, \gamma o) \| \le d(ho, \gamma o) \le D_0$
, we have
and, similarly,
Recalling the definition
$\mathcal G^{\theta}(\xi, \eta) =({1}/{2})(\beta_{\xi}^{\theta}(o, ho) + {\rm i}(\beta_{\eta}^{\theta}(o, ho)))$
, and using
$\psi = \psi \circ {\rm i}$
, we obtain that
as desired.
The dotted triangle is of diameter less than C and the gray ball has radius R.

We are now ready to prove the first inclusion in Theorem 6.2, which we formulate again as follows.
Proposition 6.8.
There exist constants
$c, R_0 \gt 0$
such that for any
$\xi \in \Lambda_{\theta}$
and
$g \in [e,\xi]$
in
$\Gamma$
, we have
Proof. Let
$C_1, D \gt 0$
be the constants given by Proposition 6.7 and Theorem 4.1, respectively. Recall the constant
$T_{\psi}$
in Proposition 6.3; the image of any geodesic triangle in
$(\Gamma, \mathsf{d}_{\Gamma})$
under the orbit map, is
$T_{\psi}$
-thin in the
$\mathsf{d}_\psi$
-metric. We now claim that (6.8) holds with
$c := e^{- (2 T_{\psi} + C_1 + D)} $
. Fix
$\xi \in \Lambda_{\theta}$
and an element
$g\in [e, \xi]$
. Let
$\eta \in B_{\psi}(\xi, c e^{-\mathsf{d}_{\psi}(o, go)} )$
; that is,
Let
$\gamma \in [\xi, \eta]$
be chosen so that
$\mathsf{d}_{\psi}(o, \gamma o) = \mathsf{d}_{\psi}(o, [\xi, \eta] o)$
. By Proposition 6.7, we have
Hence, by (6.9),
Let
$g' \in [\xi, \eta]$
be such that
$\mathsf{d}_{\psi}(go, g' o) = \mathsf{d}_{\psi}(go, [\xi, \eta] o)$
. By Theorem 4.1, we also have
Together with (6.10), this implies
Since the triangle
$[e, \xi]o \cup [\xi, \eta]o \cup [e, \eta ]o$
is
$T_{\psi}$
-thin in
$\mathsf{d}_{\psi}$
-metric, go is contained in the
$T_{\psi}$
-neighborhood of
$[\xi, \eta]o \cup [e, \eta ]o$
. Since
$\mathsf{d}_{\psi}(g o, [\xi, \eta] o) \gt 2 T_{\psi}$
by (6.11), we must have
$\mathsf{d}_{\psi}(g o, [e, \eta] o) \le T_{\psi} $
(see Figure 6). For the constant
$T' := C_{\psi}(T_{\psi} + C_{\psi})$
, where
$C_{\psi}$
is as in (6.2), we have
With the constant
$D_0$
given in Theorem 4.13, there exists
$\ell \in K$
so that
$\ell P_{\theta} = \eta$
and
$[e, \eta] o$
is contained in the
$D_0$
-neighborhood of
$\ell M_{\theta}A^+ o$
in the Riemannian distance d. This implies that
This completes the proof with
$R_0=T'+D_0$
.
go is far from
$[\xi, \eta]o$
and hence close to
$[e, \eta]o$
; so
$\eta$
lies in the shadow
$O^{\theta}_{T' + D_0}(o, go)$
.

7. Shadows inside balls: the second inclusion in Theorem 6.2
We continue the setup from § 6. Hence,
${\rm i}(\theta)=\theta$
and
$\psi\in \mathfrak a_\theta^*$
is a linear form such that
$\psi\gt 0$
on
$\mathcal L-\{0\}$
and
$\psi=\psi \circ {\rm i}$
. In this section, we prove the second inclusion of Theorem 6.2, which can be stated as follows.
Proposition 7.1.
For any
$r \gt 0$
, there exists
$c' = c'_r \gt 0$
such that for any
$\xi \in \Lambda_{\theta}$
and any
$g \in [e,\xi]$
in
$\Gamma$
, we have
In addition to the coarse triangle inequality of
$\mathsf{d}_\psi$
(Theorem 4.1) and the uniform progression lemma (Lemma 6.4), we will use the property that the shadows in
$(\Gamma, \mathsf{d}_\Gamma)$
are comparable to shadows in
$\Lambda_\theta$
(Proposition 7.2) and that the half-spaces spanned by shadows of balls in
$(\Gamma, \mathsf{d}_{\Gamma})$
stay deeper than the balls from the viewpoints (see Figure 7 and Lemma 7.4).
A pictorial description of Lemma 7.4.

In the Gromov hyperbolic space
$(\Gamma,\mathsf{d}_\Gamma)$
, for
$R\gt 0$
and
$\gamma_1, \gamma_2\in \Gamma$
, the shadow
$O_R^{\Gamma}(\gamma_1, \gamma_2)$
is defined as the set of all
$\xi\in \partial \Gamma$
such that a geodesic ray
$[\gamma_1, \xi]$
intersects the R-ball centered at
$\gamma_2$
:
Clearly, shadows are
$\Gamma$
-equivariant in the sense that for any
$\gamma\in \Gamma$
, we have
$\gamma O_R^{\Gamma}(\gamma_1, \gamma_2)=O_R^{\Gamma}(\gamma \gamma_1, \gamma \gamma_2)$
.
The following proposition states that shadows in
$\partial \Gamma$
and shadows in
$\Lambda_{\theta}$
are compatible via the boundary map
$f : \partial \Gamma \to \Lambda_{\theta}$
: recall that the orbit map
$(\Gamma, \mathsf{d}_{\Gamma}) \to (\Gamma o, d)$
is a Q-quasi-isometry for some
$Q \ge 1$
(Theorem 3.8(3)) and let
$R_0 := Q + D_0 + 1$
, where
$D_0$
is given in Theorem 4.13.
Proposition 7.2.
For any
$R\gt R_0$
, there exists
$R_1, R_2 \gt 0$
such that for any
$\gamma_1, \gamma_2 \in \Gamma$
,
In proving this proposition, we also need to consider shadows whose viewpoints are on the boundary
$\mathcal F_\theta$
. For
$\eta\in \mathcal F_\theta$
,
$p\in X$
, and
$R\gt 0$
, the
$\theta$
-shadow
$O_R^{\theta}(\eta, p)$
is defined as follows:
We need the following proposition on continuity of shadows.
Proposition 7.3 (Continuity of shadows on viewpoints [Reference Kim, Oh and WangKOW25a, Proposition 3.4]). Let
$p \in X$
,
$\eta \in \mathcal F_{\theta}$
and
$r\gt 0$
. If a sequence
$q_i \in X$
converges to
$ \eta $
as
$i \to \infty$
as in Definition 2.2, then for any
$0\lt \varepsilon\lt r$
, we have
7.1 Proof of Proposition 7.2
Let
$R\gt R_0$
. By the
$\Gamma$
-equivariance of f as well as of shadows, we may assume that
$\gamma_1 = e$
and write
$\gamma_2 = \gamma$
. By applying Theorem 4.13(2), we obtain that for any
$\xi \in \partial \Gamma$
and
$k\in K$
with
$kP_{\theta} =f(\xi)$
, the image
$[e, \xi]o$
is contained in the
$D_0$
-neighborhood of
$kM_\theta (\exp \mathcal C) o\subset k M_{\theta} A^+ o$
in the symmetric space (X, d). Since
$R\gt R_0=Q+D_0+1 $
, we can choose
$R_1\gt 0$
so that
$ Q R_1+ Q+D_0 \lt R$
. Now if
$\xi\in O^\Gamma_{R_1}(e, \gamma)$
, and hence
$[e, \xi]$
intersects the ball
$\{g\in \Gamma: \mathsf{d}_\Gamma( \gamma , g)\lt R_1\}$
, then
$kM_{\theta}A^+ o$
intersects the
$ Q R_1+ Q+D_0 $
-neighborhood of
$\gamma o$
, and hence the R-neighborhood of
$\gamma o$
. Therefore,
$f(\xi) \in O_{R}^{\theta}(o, \gamma o)$
. This shows the first inclusion.
To prove the second inclusion, suppose that the claim does not hold for some
$R\gt R_0$
. Then, for each
$i \ge 1$
, there exists
$\gamma_i \in \Gamma$
such that
in other words, there exists
$x_i \in \partial \Gamma - O_i^{\Gamma}(e, \gamma_i)$
such that
$f(x_i) \in O_R^{\theta}(o, \gamma_i o)$
. By the
$\Gamma$
-equivariance of f, it follows that
After passing to a subsequence, we may assume that
$\gamma_i^{-1} \to y \in \partial \Gamma$
and
$\gamma_i^{-1}x_i \to x$
as
$i \to \infty$
. By Theorem 3.8(4), we deduce
$\gamma_i^{-1} o \to f(y)$
as
$i \to \infty$
. Applying Proposition 7.3 to
$q_i = \gamma_i^{-1} o$
,
$p = o$
and
$\eta = f(y)$
, we have for some
$\varepsilon \gt 0$
that
Since
$f(\gamma_i^{-1} x_i) \in O_{R}^{\theta}(\gamma_i^{-1}o, o)$
for all
$i \ge 1$
and
$f(\gamma_i^{-1} x_i) $
converges to f(x) as
$i \to \infty$
, we have
This implies that f(x) is in general position with f(y), i.e.,
$(f(x), f(y))\in \mathcal F_\theta^{(2)}$
, and in particular
$f(x) \neq f(y)$
. On the other hand, since
$\gamma_i^{-1}x_i \notin O_i^{\Gamma}(\gamma_i^{-1}, e)$
for all
$i \ge 1$
, the sequence of geodesics
$[\gamma_i^{-1} x_i, \gamma_i^{-1}]$
escapes any large ball centered at e. This implies that two sequences
$\gamma_i^{-1} x_i$
and
$\gamma_i^{-1}$
must have the same limit, and hence
$x = y$
, which is a contradiction. Therefore, the claim follows.
The Gromov product in
$(\Gamma, \mathsf{d}_{\Gamma})$
is defined as follows: for
$\alpha, \beta, \gamma \in \Gamma$
,
and for
$x, y \in \partial \Gamma$
,
where the supremum is taken over all sequences
$\{x_i\}, \{y_j\}$
in
$\Gamma$
such that
$\lim_{i \to \infty} x_i = x$
and
$\lim_{j \to \infty} y_j = y$
. The Gromov product for a pair of a point in
$\Gamma$
and a point in
$\partial \Gamma$
is defined similarly. The Gromov product
$(x, y)_{\gamma}$
is known to measure distance from
$\gamma$
and to a geodesic [x, y] up to a uniform additive error (for basic properties of Gromov hyperbolic spaces, see [Reference Bridson and HaefligerBH99]).
The following lemma says that the half-space spanned by the shadow is opposite to the light; more precisely, for any
$x\in \partial \Gamma$
and
$\gamma\in [e,x]$
, the half-space spanned by all geodesics connecting x and
$O^\Gamma_R(e,\gamma)$
lies farther than
$\gamma$
, viewed from e.
Lemma 7.4.
Given
$R \gt 0$
, there exists
$r = r_R \gt 0$
such that for any
$x\in \partial \Gamma$
,
$\gamma\in [e,x]$
, and
$y \in O_R^{\Gamma}(e, \gamma)$
, we have
where
$\gamma_{x,y}\in [x, y]$
denotes the nearest-point projection of e to a geodesic [x,y].
Proof. Let
$[e, x] = \{\gamma_i\}_{i \ge 0}$
. We fix
$\gamma := \gamma_i$
and
$y \in O_R^{\Gamma}(e, \gamma)$
. In terms of the Gromov product, we have
$(e, y)_{\gamma} \lt R + \delta / 2$
for some uniform
$\delta \gt 0$
depending only on
$\Gamma$
. On the other hand, the hyperbolicity of
$\Gamma$
also implies that we can take
$\delta$
large enough so that
and that every geodesic triangle in
$\Gamma \cup \partial \Gamma$
is
$\delta$
-thin. Therefore
First, consider the case when
$(\gamma_{x,y}, y)_{\gamma} \lt R + \delta$
. Then, for some constant
$\delta_1$
depending on
$R + \delta$
, there exists
$\gamma' \in [\gamma_{x,y}, y]$
such that
$\mathsf{d}_{\Gamma}(\gamma', \gamma) \lt \delta_1$
. Consider the geodesic triangle with vertices
$x, \gamma, \gamma'$
. Since this triangle is
$\delta$
-thin and
$\gamma_{x,y} \in [x, \gamma']$
, the
$\delta$
-neighborhood of
$\gamma_{x,y}$
intersects
$[x, \gamma] \cup [\gamma, \gamma']$
. Hence it follows from
$\mathsf{d}_{\Gamma}(\gamma, \gamma') \lt \delta_1$
that the
$(\delta + \delta_1)$
-neighborhood of
$\gamma_{x,y}$
intersects the geodesic
$[x, \gamma]$
. Namely,
Now consider the case that
$(e, \gamma_{x,y})_{\gamma} \lt R + \delta$
. Since
$\gamma_{x,y}$
is the nearest-point projection of e to [x, y], there exists a constant
$\delta_2$
depending only on
$\Gamma$
such that the
$\delta_2$
-neighborhood of
$\gamma_{x,y}$
intersects both geodesic rays [e, x] and [e, y]. In particular, there exists
$\gamma_{k}\in [e, x]$
such that
$\mathsf{d}_{\Gamma}(\gamma_{x,y}, \gamma_{k}) \lt \delta_2$
. This implies
Since both
$\gamma =\gamma_i $
and
$ \gamma_{k}$
lie on the geodesic [e, x], this implies that
${k} \ge i - (R + \delta + \delta_2)$
. Let j be the unique integer such that
$k + R + \delta + \delta_2 \le j \le k + R + \delta + \delta_2 + 1$
. Note that since
$k \ge i - (R + \delta + \delta_2)$
, we have
$j \ge i$
, and hence
$\gamma_j \in [\gamma, x]$
. Then,
\begin{align*} \mathsf{d}_{\Gamma}(\gamma_{x,y}, [\gamma, x] ) &\le \mathsf{d}_{\Gamma}(\gamma_{x,y}, \gamma_j) \\ &\le \mathsf{d}_{\Gamma}(\gamma_{x, y}, \gamma_k) + \mathsf{d}_{\Gamma}(\gamma_k, \gamma_j) \\ &\le \delta_2 + (j-k)\le R + \delta + 2 \delta_2 + 1 . \end{align*}
Therefore, it remains to set
$r = R + \delta + \delta_1 + 2 \delta_2 + 1$
.
We are new ready to prove Proposition 7.1.
7.2 Proof of Proposition 7.1
Let
$\xi \in \Lambda_\theta=\partial\Gamma$
and
$g\in [e,\xi]$
in
$\Gamma$
. Fix
$r\gt 0$
, and let
$\eta \in O_r^{\theta}(o, g o) \cap \Lambda_{\theta}$
distinct from
$\xi$
. We will continue to use the convention of identifying
$\Lambda_\theta$
and
$\partial \Gamma$
in this proof. As in Lemma 7.4, we let
$\gamma_{\xi,\eta}$
be the nearest-point projection of e to a bi-infinite geodesic
$[\xi, \eta]$
in
$(\Gamma, \mathsf{d}_\Gamma)$
. By Proposition 7.2, there exists
$R\gt 0$
, depending only on r, such that
$\eta \in O_R^{\Gamma}(e, g)$
. Write the geodesic ray
$[e,\xi]$
as a sequence
$\{g_k\}_{k \ge 0}$
with
$g_0=e$
. Since
$g\in [e,\xi]$
by the hypothesis, we have
$g_i = g$
for some
$i \ge 0$
. Then, for
$r_R \gt 0$
given in Lemma 7.4, there exists
$j \ge i$
such that
Let
$n_1 \ge 0$
and
$D \ge 0$
be given by Lemma 6.4 (uniform progression lemma) and Theorem 4.1 (coarse triangle inequality), respectively. We then have
Since
$g = g_i$
, we have
$\mathsf{d}_{\psi}(g_{i - n_1} o, go) \le Q_{\psi}(n_1 + 1)$
, where
$Q_{\psi}$
is the constant in Proposition 6.3. Hence we deduce by setting
$D' := Q_{\psi}(n_1 + 1) + D$
that
On the other hand, applying the coarse triangle inequality (Theorem 4.1) again, we have
Since
$\mathsf{d}_{\Gamma}(\gamma_{\xi,\eta}, g_j) \le r_R$
, we have
$\mathsf{d}_{\psi}(\gamma_{\xi,\eta} o, g_j o) \le Q_{\psi}(r_R + 1)$
by Proposition 6.3, and hence
Since we have
$|\psi( \mathcal G^{\theta}(\xi, \eta)) - \mathsf{d}_{\psi}(o, \gamma_{\xi,\eta} o) | \lt \|\psi\|C_1$
with
$C_1$
given by Lemma 5.4,
Setting
$c' := e^{D' + Q_{\psi}(r_R + 1) + D + \|\psi\|C_1}$
, we have
Hence
$\eta \in B_\psi (\xi, c' e^{{-\mathsf{d}_{\psi}(o, go)}}) $
as desired.
7.3 Comparing Gromov products
Lemma 7.5.
Let
$\psi \in \mathfrak a_{\theta}^*$
be such that
$\psi \gt 0$
on
$\mathcal L - \{0\}$
. Then there exists
$c \gt 0$
, depending only on
$\psi$
, such that for all
$x, y\in \partial\Gamma$
,
where
$Q_{\bar\psi}$
is as given in Proposition 6.3.
Proof. Let
$x \neq y \in \partial \Gamma$
and set
$\gamma_{x, y} \in \Gamma$
the nearest-point projection of e to [x, y] in
$(\Gamma, \mathsf{d}_{\Gamma})$
. By Lemma 5.4, we have
where
$C_1$
is given in Lemma 5.4. As in the proof of Proposition 5.5,
Since
by Proposition 6.3 with
$Q_{\bar \psi} \ge 1$
therein, we now have that
where
$c' := Q_{\bar \psi} + C_1 (1 + \|\psi\|)$
. Since
$(\Gamma, \mathsf{d}_{\Gamma})$
is Gromov hyperbolic, we have that
$|(x, y)_e - \mathsf{d}_{\Gamma}(e, \gamma_{x, y})|$
is uniformly bounded. Hence, the claim follows.
8. Ahlfors regularity of Patterson–Sullivan measures
As before, let
$\Gamma$
be a
$\theta$
-Anosov subgroup of a connected semisimple real algebraic group G. Recall from Theorem 3.4 that the space of
$\Gamma$
-Patterson–Sullivan measures on
$\Lambda_\theta$
is parameterized by the set
We continue to use the notation
$\nu_\psi$
for the unique
$(\Gamma, \psi)$
-Patterson–Sullivan measure on
$\Lambda_{\theta}$
. Recall that
$d_\psi $
is the premetric on
$\Lambda_\theta$
defined by
$d_\psi(\xi, \eta)=e^{-\psi(\mathcal G(\xi, \eta))}$
for all
$\xi\ne \eta$
in
$\Lambda_\theta$
and
$B_{\psi}(\xi, r)=\{\eta\in \Lambda_\theta: d_\psi(\xi, \eta)\lt r\}$
.
The Ahlfors regularity is an important notion in fractal geometry.
Definition 8.1.
A premetric space (Z, d) is called Ahlfors s-regular if there exist a Borel measure
$\nu$
on Z and
$C\ge 1$
so that for all
$z\in Z$
and
$r\in [0, \operatorname{{\rm diam}} Z)$
,
where
$B(z, r)=\{w\in Z: d(z,w)\lt r\}$
. Such a measure
$\nu$
is also called Ahlfors s-regular.
The goal of this section is to deduce the following from Theorem 6.2.
Theorem 8.2.
For any symmetric
$\psi \in \mathscr T_\Gamma$
, the measure
$\nu_\psi$
is Ahlfors one-regular on
$(\Lambda_\theta, d_\psi)$
.
Remark 8.3. When
$\Gamma$
is a convex cocompact subgroup of
$G=\operatorname{{\rm SO}}^\circ (n,1)$
,
$\mathscr T_\Gamma$
is a singleton consisting of the critical exponent
$\delta_\Gamma$
(more precisely, the multiplication by
$\delta_\Gamma$
on
$\mathbb R$
), and the metric
$d_{\delta_\Gamma}$
is the
$\delta_\Gamma$
-power of a K-invariant Riemannian metric on
$\mathbb S^{n-1}$
. Hence Theorem 8.2 is equivalent to Sullivan’s theorem [Reference SullivanSul79, Theorem 7] that the Patterson–Sullivan measure of a Riemannian ball of radius r is comparable to
$r^{\delta_\Gamma}$
.
We use the higher-rank version of Sullivan’s shadow lemma. The following is a special case of [Reference Kim, Oh and WangKOW25b, Lemma 7.2].
Lemma 8.4 (Shadow lemma) Let
$\Gamma \lt G$
be a non-elementary
$\theta$
-Anosov subgroup. For all large enough
$R \gt 0$
, there exists
$c_0 = c_0 (\psi, R) \ge 1$
such that for all
$\gamma \in \Gamma$
,
8.1 Proof of Theorem 8.2
By Lemma 3.7 and Remark 5.7, it suffices to consider the case of
$\theta = {\rm i}(\theta)$
. Let c and
$R_0$
be the constants as in Theorem 6.2. Fix
$\xi \in \Lambda_{\theta}$
and
$0\lt r \lt \operatorname{{\rm diam}}(\Lambda_\theta, d_\psi)$
. Write the geodesic ray
$[e, \xi] $
as
$\{\gamma_k\}_{k \ge 0}$
in
$(\Gamma, \mathsf{d}_\Gamma)$
. Setting
Theorem 6.2 implies that for any
$R \gt R_0$
,
By Lemma 8.4, we obtain
By the coarse triangle inequality of
$\mathsf{d}_\psi$
(Theorem 4.1), we have
where D is as in Theorem 4.1. Since
$\mathsf{d}_{\psi}(\gamma_i o, \gamma_{i + 1} o) \le 2 Q_{\psi}$
with
$Q_{\psi}$
in Proposition 6.3, we have
where
$D' = D + 2 Q_{\psi}$
. This implies that
where the last inequality follows from the definition of
$i = i_r$
in (8.1). Hence, we deduce from (8.2) that
Now let
$c' = c'_R \gt 0$
be given by Theorem 6.2 and set
By Theorem 6.2, we have
and hence applying Lemma 8.4 yields
By the minimality of
$j = j_r$
as defined in (8.3) and the coarse triangle inequality of
$\mathsf{d}_\psi$
(Theorem 4.1), we have
Recalling that
$\mathsf{d}_{\psi}(\gamma_{j-1} o, \gamma_j o) \le 2 Q_{\psi}$
and
$D' = D + 2 Q_{\psi}$
, we have
and hence
Therefore, the theorem is proved with
$c_1= \max (c_0e^{D'} c^{-1}, c_0 c' e^{D'})$
.
9. Hausdorff measures on limit sets
Let
$\Gamma \lt G$
be a
$\theta$
-Anosov subgroup, where G is a connected semisimple real algebraic group. For a linear form
$\psi \in \mathfrak a_\theta^*$
that is positive on
$\mathcal L -\{0\}$
, consider the associated conformal premetric
$d_\psi$
on
$\Lambda_\theta$
. For
$s\gt 0$
, we denote by
$\mathcal H_{\psi}^s$
the associated Hausdorff measure of dimension s; that is, for any subset
$B \subset \Lambda_{\theta}$
, let
where
$\operatorname{{\rm diam}}_{\psi} U =\sup_{\xi, \eta\in U} d_\psi(\xi, \eta)$
. This is an outer measure which induces a Borel measure on
$\Lambda_\theta$
(see [Reference FalconerFal14] and [Reference Dey and KapovichDK22, Appendix A]). For
$s=1$
, we simply write
$\mathcal H_\psi$
for
$\mathcal H_\psi^1$
. Recall that
$\mathscr T_{\Gamma}$
is the space of all linear forms tangent to the growth indicator
$\psi_\Gamma^\theta$
. In this section, we first deduce the following two theorems from Theorem 8.2. Together with Theorem 9.12, they imply Theorems 1.1 and 1.3. We also prove Theorem 1.4.
Theorem 9.1.
For any symmetric
$\psi\in \mathscr T_\Gamma$
, the associated Patterson–Sullivan measure
$\nu_\psi$
coincides with the one-dimensional Hausdorff measure
$\mathcal H_{\psi}$
, up to a constant multiple. In other words,
$\mathcal H_\psi$
is the unique
$(\Gamma, \psi)$
-conformal measure on
$\Lambda_\theta$
(up to a constant multiple).
We also show that the symmetric hypothesis is necessary.
Theorem 9.2.
If
$\psi\in \mathscr T_\Gamma$
is not symmetric and
$\Gamma$
is Zariski dense, then
$\nu_\psi$
is not comparable to
$\mathcal H_{\psi}^s$
for any
$s \gt 0$
.
Remark 9.3. If
$\psi\in \mathfrak a_\theta^*$
is positive on
$\mathcal L -\{0\}$
, then
$\delta_\psi \psi\in \mathscr T_\Gamma$
. Since
$\mathcal H_{ \delta_\psi \psi}=\mathcal H_{\psi}^{\delta_\psi}$
, Theorem 9.1 says that if
$\psi$
is symmetric in addition,
Remark 9.4. For a special class of symmetric
$\psi$
whose gradient lies in the interior of
$\mathfrak a_\theta^+$
, Dey and Kapovich [Reference Dey and KapovichDK22, Corollary 4.8] have shown that
$(\Gamma o, \mathsf{d}_\psi)$
is a Gromov hyperbolic space and they have proved Theorem 9.1 relying upon the work of Coornaert [Reference CoornaertCoo93], which gives the positivity and finiteness of
$\mathcal H_\psi$
for the Gromov hyperbolic space. In our generality,
$(\Gamma o, \mathsf{d}_\psi)$
is not even a metric space, and hence their approach cannot be extended.
The main work is to establish the positivity and the finiteness of
$\mathcal H_\psi$
and the key ingredient is the Ahlfors regular property of
$\nu_\psi$
obtained in Theorem 8.2. For example, positivity of
$\mathcal H_\psi$
is a standard consequence of the Ahlfors regularity of
$(\Lambda_\theta, d_\psi)$
. However, we cannot conclude finiteness of
${\mathcal H}_\psi$
directly from Ahlfors regularity due to the lack of the triangle inequality.
Proposition 9.5 (Positivity) For any symmetric
$\psi\in \mathscr T_\Gamma$
, we have
Proof. Fix
$\varepsilon \gt 0$
and a countable cover
$\{U_i\}_{i \in \mathbb N}$
such that
$\operatorname{{\rm diam}}_{\psi} U_i \le \varepsilon$
for all
$i \in \mathbb N$
. For each
$i \in \mathbb N$
, we choose
$\xi_i \in U_i$
. By Theorem 8.2, we have
where the constant
$C\gt 0$
depends only on
$\psi$
. Since
$\Lambda_{\theta} \subset \bigcup_{i \in \mathbb N} U_i \subset \bigcup_{i \in \mathbb N} B_{\psi}(\xi_i, \operatorname{{\rm diam}}_{\psi} U_i)$
, it follows that
$\sum_{i \in \mathbb N} \operatorname{{\rm diam}}_{\psi} U_i \ge C \cdot \nu_{\psi} (\Lambda_{\theta}) = C.$
Since
$\{U_i\}_{i \in \mathbb N}$
is an arbitrary countable cover, it follows that
$\mathcal H_{\psi, \varepsilon}(\Lambda_{\theta}) \ge C$
. Since
$\varepsilon\gt 0$
is arbitrary and C is independent of
$\varepsilon\gt 0$
, we have
$\mathcal H_\psi (\Lambda_\theta)\gt 0$
.
Proposition 9.6 (Finiteness) For any symmetric
$\psi\in \mathscr T_\Gamma$
, we have
Proof. Let
$N=N(\psi)$
and
$N_0=N_0(\psi)$
be the constants given in Proposition 5.3 and Lemma 5.6 respectively. Fix
$\varepsilon \gt 0$
. Since
$\Lambda_{\theta}$
is compact, we have a finite cover
$\Lambda_{\theta}$
by
$ \bigcup_{i = 1}^n B_{\psi}(\xi_i, {\varepsilon}/{2NN_0})$
for some finite set
$\xi_1, \ldots, \xi_n \in \Lambda_{\theta}$
. Applying the Vitali covering type lemma (Lemma 5.6), there exists a disjoint subcollection
$B_{\psi}(\xi_{i_1}, {\varepsilon}/{2NN_0}), \ldots, B_{\psi}(\xi_{i_k}, {\varepsilon}/{2NN_0})$
such that
$$\Lambda_{\theta} \subset \bigcup_{j = 1}^k B_{\psi}\left(\xi_{i_j}, \frac{\varepsilon}{2N}\right)\!.$$
Since
$\operatorname{{\rm diam}}_{\psi} B_{\psi}(\xi_{i_j}, {\varepsilon}/{2N}) \le \varepsilon$
for each
$1 \le j \le k$
by Proposition 5.3(2), we have
$$\mathcal H_{\psi,\varepsilon}(\Lambda_{\theta}) \le \sum_{j = 1}^k \operatorname{{\rm diam}}_{\psi} B_{\psi}\left(\xi_{i_j}, \frac{\varepsilon}{2N}\right) \le k \cdot \varepsilon.$$
Applying Theorem 8.2, we obtain that for some constant
$C\gt 0$
depending only on
$\psi$
,
$$ k \cdot \varepsilon \le C \sum_{j = 1}^k \nu_{\psi}\bigg(B_{\psi}\bigg(\xi_{i_j}, \frac{\varepsilon}{2NN_0}\bigg)\bigg) = C \cdot \nu_{\psi} \bigg(\bigcup_{j = 1}^k B_{\psi}\bigg(\xi_{i_j}, \frac{\varepsilon}{2NN_0}\bigg)\bigg) \le C \cdot \nu_{\psi}(\Lambda_{\theta}) = C, $$
where the equality follows from the disjointness. This implies
$\mathcal H_{\psi, \varepsilon}(\Lambda_{\theta}) \le C$
. Since
$\varepsilon$
is arbitrary, we have
$\mathcal H_{\psi}(\Lambda_{\theta}) \le C$
.
Hence
$\mathcal H_\psi$
is a non-trivial measure on
$\Lambda_\theta$
. It is also
$(\Gamma, \psi)$
-conformal.
Lemma 9.7 (Conformality) For any symmetric
$\psi\in \mathscr T_\Gamma$
, we have
for all
$\gamma \in \Gamma$
and
$\xi \in \Lambda_{\theta}$
.
Proof. Since
$d_{\psi}$
is invariant under the
$\Gamma$
-equivariant homeomorphism
$p : \Lambda_{\theta\cup{\rm i}(\theta)} \to \Lambda_\theta$
by the definition of
$d_{\psi}$
(Remark 5.7), the measure
$(\mathcal H_\psi,\Lambda_\theta)$
is the push-forward of the Hausdorff measure
$(\mathcal H_\psi, \Lambda_{\theta\cup {\rm i} (\theta)})$
via p. Therefore, it suffices to prove this lemma assuming that
$\theta = {\rm i}(\theta)$
. We simply write
$\beta^{\theta} = \beta$
in this proof to ease the notation.
Fix
$\gamma \in \Gamma$
and
$\xi \in \Lambda_{\theta}$
. Let
$U \subset \Lambda_{\theta}$
be a small open neighborhood of
$\xi$
. To estimate
$\gamma_* \mathcal H_{\psi}(U)$
in terms of
$\mathcal H_{\psi}(U)$
, we fix
$\varepsilon \gt 0$
and take any cover
$\{U_i \}_{i \in \mathbb N}$
of U such that
$\operatorname{{\rm diam}}_{\psi} U_i \le \varepsilon$
and that
$U \cap U_i \neq \emptyset$
for all
$i \in \mathbb N$
.
For simplicity, we write
$s_{\xi, R} (\gamma) := \sup_{\eta \in B_{\psi}(\xi, R)} e^{\psi(\beta_{\eta}(e, \gamma))}$
. By Lemma 5.2 and Proposition 5.3 with
$N=N(\psi) \gt 0$
therein, we have that for each
$i \ge 1$
,
where
$R_{\varepsilon} =R_\varepsilon(U)= N\cdot (\operatorname{{\rm diam}}_{\psi} U + \varepsilon)$
. We then have for
$\tilde{\varepsilon} := s_{\xi, R_{\varepsilon}}(\gamma) \varepsilon$
,
Since
$\{U_i\}_{i \in \mathbb N}$
is an arbitrary countable open cover of U, the above inequality implies that
Taking
$\varepsilon \to 0$
, we have
$\tilde{\varepsilon} = s_{\xi, R_\varepsilon}( \gamma) \varepsilon \to 0$
and
$R_{\varepsilon} \to R_U := N \cdot \operatorname{{\rm diam}}_{\psi} U$
. Therefore,
Applying (9.3) after replacing U with
$\gamma^{-1} U$
, and
$\gamma$
by
$\gamma^{-1}$
, we have
If we set
$c = \sup_{\zeta \in \Lambda_{\theta}} e^{\psi(\beta_{\zeta}(e, \gamma^{-1} ))}$
, then for any
$\eta \in B_{\psi}(\gamma^{-1} \xi, R_{\gamma^{-1}U})$
, it follows from Lemma 5.2 that
This implies that
$$ \begin{aligned} s_{\gamma^{-1} \xi, R_{\gamma^{-1} U}}(\gamma^{-1}) & = \sup_{\eta \in B_{\psi}(\gamma^{-1} \xi, R_{\gamma^{-1} U})} e^{ \psi(\beta_{\eta}(e, \gamma^{-1}))} \\ & \le \sup_{\eta \in B_{\psi}(\xi, c R_{\gamma^{-1} U})} e^{\psi(\beta_{\gamma^{-1} \eta}(e, \gamma^{-1}))} = \sup_{\eta \in B_{\psi}(\xi, c R_{\gamma^{-1} U})} e^{\psi(\beta_{\eta}(\gamma, e))}. \end{aligned}$$
Hence, we obtain from (9.4) that
Together with (9.3), we deduce
Now shrinking
$U \to \xi$
, we have
$R_U, R_{\gamma^{-1} U} \to 0$
and, hence, both sides in the above inequality converge to
$e^{ \psi(\beta_{\xi}(e, \gamma))}$
, by the continuity of the Busemann map
$\beta_{\eta}(e, \gamma )$
on the
$\eta$
-variable. Therefore,
as desired.
9.1 Proof of Theorem 9.1
By Propositions 9.5 and 9.6, we have
$\mathcal H_{\psi}(\Lambda_{\theta}) \in (0, \infty)$
. Moreover, it follows from Lemma 9.7 that
${1}/{\mathcal H_{\psi}(\Lambda_{\theta})}\mathcal H_{\psi}$
is a
$(\Gamma, \psi)$
-Patterson–Sullivan measure. Since there exists a unique
$(\Gamma, \psi)$
-Patterson–Sullivan measure on
$\Lambda_{\theta}$
(Theorem 3.4), this completes the proof.
9.2 Proof of Theorem 9.2
By Lemma 3.7, we may assume that
$\theta = {\rm i}(\theta)$
. Since
$\psi\ne \psi \circ {\rm i}$
, two linear forms
$\psi$
and
$\bar \psi$
are not proportional. Since
$d_{\psi}$
and
$d_{\bar \psi}$
are bi-Lipschitz by Proposition 5.5,
$\mathcal H_{\psi}^s$
is in the same measure class as
$\mathcal H_{\bar \psi}^s$
for all
$s \gt 0$
. Hence, it follows from Theorem 9.1 (see also Remark 9.3) that
$\mathcal H_{\psi}^s(\Lambda_{\theta}) = 0$
or
$\infty$
if
$s \neq \delta_{\bar \psi}$
. It now suffices to show that
$\nu_\psi$
is not comparable to
$\mathcal H_{\psi}^{\delta_{\bar \psi}}$
. Since
$\psi$
and
$\bar \psi$
are not proportional,
$\psi$
and
$\delta_{\bar \psi} \bar \psi$
are two different forms tangent to
$\psi_{\Gamma}^{\theta}$
. By Theorem 3.4, it follows that
$\nu_\psi $
is mutually singular to
$\nu_{\delta_{\bar \psi} \bar \psi}$
. Since the latter is proportional to
$\mathcal H_{\bar \psi}^{\delta_{\bar \psi}}$
by Theorem 9.1,
$\nu_\psi$
is singular to
$\mathcal H_{\bar \psi}^{\delta_{\bar \psi}}$
and hence singular to
$\mathcal H_{\psi}^{\delta_{\bar \psi}}$
as well. This finishes the proof.
Remark 9.8. In fact, without the Zariski dense hypothesis, it has been shown in [Reference SambarinoSam24, Theorem A] that for
$\psi_1, \psi_2 \in \mathscr T_{\Gamma}$
,
$\nu_{\psi_1}$
and
$\nu_{\psi_2}$
are mutually singular unless
$\psi_1 = \psi_2$
on
$\mathcal L_{\theta}$
. Hence, Theorem 9.2 holds provided that
$\psi$
and
$\psi \circ {\rm i}$
are not identical on
$\mathcal L_{\theta}$
.
9.3 Critical exponents and Hausdorff dimensions
The Hausdorff dimension of
$\Lambda_{\theta}$
with respect to
$d_{\psi}$
is defined as
As a corollary of Theorem 9.1, we obtain the following (Theorem 1.4).
Corollary 9.9.
For any
$\psi \in \mathfrak a_{\theta}^*$
positive on
$\mathcal L -\{0\}$
, we have
where
$ \bar \psi = {\psi + \psi \circ {\rm i}}/{2}.$
Proof. By Proposition 5.5, we have
$\dim_{\psi} \Lambda_{\theta} = \dim_{\bar \psi} \Lambda_{\theta}$
. Applying Theorem 9.1 to
$\delta_{\bar\psi} \bar \psi$
(see Remark 9.3), we have
$\mathcal H_{\bar \psi}^{\delta_{\bar \psi}}(\Lambda_{\theta}) \in (0, \infty)$
, which implies that
$\dim_{\bar \psi} \Lambda_{\theta} = \delta_{\bar \psi}$
. This shows the claim.
For
$\psi$
non-symmetric,
$\dim_{\psi} \Lambda_{\theta}$
is not in general equal to
$\delta_\psi$
.
Proposition 9.10.
For
$\psi \in \mathfrak a_{\theta}^*$
positive on
$\mathcal L - \{0\}$
, we have
If
$\Gamma$
is Zariski dense, then the equality holds if and only if
$\psi = \psi \circ {\rm i}$
.
Proof. As before, we may assume that
$\theta = {\rm i}(\theta)$
. Suppose that
$\psi \neq \psi \circ {\rm i}$
. Note that
$\delta_{\psi}=\delta_{\psi \circ {\rm i}}$
and hence both
$\delta_{\psi}\psi$
and
$ \delta_{\psi} (\psi\circ {\rm i})$
are tangent to the
$\theta$
-growth indicator
$\psi_{\Gamma}^{\theta}$
(see [Reference Kim, Minsky and OhKMO24, Theorem 2.5] and [Reference Kim, Oh and WangKOW25b, Lemma 4.5]). We then have
$\psi_\Gamma^\theta \le \delta_{\psi}\psi$
and
$\psi_{\Gamma}^{\theta} \le\delta_{\psi} (\psi\circ {\rm i}) $
. Hence,
$\psi_\Gamma^\theta \le \delta_{\psi} \bar\psi$
. Since
$\delta_{\bar\psi}\bar\psi$
is tangent to
$\psi_\Gamma^\theta$
, it follows that
$\delta_{\bar \psi}\le \delta_{\psi} $
.
Now suppose that
$\Gamma$
is Zariski dense and that
$\psi\ne \psi\circ {\rm i}$
. By Theorem 3.3, there exists a unique unit vector
$u=u_{\delta_\psi \psi} \in \operatorname{{\rm int}} \mathcal L_\theta$
such that
$\psi_\Gamma^{\theta}(u)= \delta_\psi \psi(u)$
. Since
$\psi_\Gamma^\theta$
is i-invariant, it implies that
$\psi_\Gamma^{\theta}({\rm i}(u))= \delta_\psi (\psi \circ {\rm i}) ({\rm i} (u))$
. On the other hand,
$u \neq {\rm i}(u)$
by Theorem 3.3. Hence the inequality
$\psi_{\Gamma}^{\theta} \le \delta_{\psi} \psi$
and
$\psi_{\Gamma}^{\theta} \le \delta_{\psi} ( \psi \circ {\rm i})$
cannot become equalities simultaneously at the same vector. This implies that
$\psi_{\Gamma}^{\theta} \lt \delta_{\psi} \bar{\psi}$
and hence
$\delta_{\bar{\psi}} \lt \delta_{\psi}$
.
By Corollary 9.9 and Proposition 9.10, we obtain the following.
Corollary 9.11.
Let
$\Gamma$
be Zariski dense in G. For any
$\psi\in \mathscr T_\Gamma$
, we have
$\dim_\psi \Lambda_\theta\le 1$
and the equality holds if and only if
$\psi$
is symmetric.
We now prove the Ahlfors regularity of
$(\Lambda_\theta, d_\psi)$
for general
$\psi \in \mathscr T_{\Gamma}$
.
Theorem 9.12.
Let
$\Gamma$
be a
$\theta$
-Anosov subgroup. For any
$\psi\in \mathscr T_\Gamma$
, the premetric space
$(\Lambda_\theta, d_\psi)$
is Ahlfors s-regular for some
$0 \lt s \le 1$
. Moreover, if
$\Gamma$
is Zariski dense, we have
$s = 1$
if and only if
$\psi$
is symmetric.
Proof. Let
$\psi \in \mathscr T_{\Gamma}$
. By Proposition 5.5, the identity map
$(\Lambda_{\theta}, d_{\psi}) \to (\Lambda_{\theta}, d_{\bar \psi})$
is bi-Lipschitz. Noting that
$\delta_{\bar \psi} \bar \psi \in \mathscr T_{\Gamma}$
by Lemma 3.6, we denote by
$\nu := \nu_{\delta_{\bar \psi} \bar \psi}$
the
$(\Gamma, \delta_{\bar \psi}\bar \psi)$
-Patterson–Sullivan measure on
$\Lambda_{\theta}$
. By Theorem 8.2, for any
$\xi \in \Lambda_{\theta}$
and
$r \in [0, \operatorname{{\rm diam}}_{\bar \psi} \Lambda_{\theta})$
, we have
for some constant
$c\ge 1$
depending only on
$\psi$
. Since
$B_{\delta_{\bar \psi} \bar \psi}(\xi, r^{\delta_{\bar \psi}}) = B_{\bar \psi}(\xi, r)$
and the identity map
$(\Lambda_{\theta}, d_{\psi}) \to (\Lambda_{\theta}, d_{\bar \psi})$
is bi-Lipschitz by Proposition 5.5, (9.5) implies that for some
$C \ge 1$
depending only on
$\psi$
, we have
Recall
$\delta_{\psi} = 1$
for
$\psi \in \mathscr T_{\Gamma}$
(Lemma 3.6). Hence
$\delta_{\bar\psi}\lt 1$
for
$\psi$
non-symmetric and
$\Gamma$
Zariski dense by Proposition 9.10. This finishes the proof.
9.4 Analyticity of Hausdorff dimensions
For a hyperbolic group
$\Sigma$
, a representation
$\sigma : \Sigma \to G$
is called
$\theta$
-Anosov if
$\sigma$
has a finite kernel and its image
$\sigma(\Sigma)$
is a
$\theta$
-Anosov subgroup of G. For a given
$\psi \in \mathfrak a_{\theta}^*$
that is non-negative on
$\mathfrak a_{\theta}^+$
, the
$\psi$
-critical exponents
$\delta_{\psi}(\sigma(\Sigma))$
vary analytically on analytic families of
$\theta$
-Anosov representations
$\sigma$
in the variety
$\operatorname{Hom}(\Sigma, G)$
by Bridgeman, Canary, Labourie, and Sambarino [Reference Bridgeman, Canary, Labourie and SambarinoBCL+15, Proposition 8.1] (see also [Reference Chow and SarkarCS23, § 4.4]). Hence the following is an immediate consequence of Corollary 9.9.
Corollary 9.13.
Let
$\Sigma$
be a non-elementary
Footnote 9
hyperbolic group and let
$\psi \in \mathfrak a_{\theta}^*$
be non-negative on
$\mathfrak a_{\theta}^+$
. Let
$\mathcal D \subset \operatorname{Hom}(\Sigma, G)$
be an analytic family of
$\theta$
-Anosov representations. Then
is analytic on
$ \mathcal D$
.
9.5 (p,q)-Hausdorff dimensions
Let
$\Sigma$
be a non-elementary convex cocompact subgroup of
$\operatorname{{\rm SO}}^\circ(n, 1)= \operatorname{{\rm Isom}}^+(\mathbb H^n)$
,
$n\ge 2$
. Let
$\operatorname{{\rm CC}}(\Sigma) $
denote the space
where the equivalence relation is given by conjugations. As in the introduction, for
$\sigma \in \operatorname{{\rm CC}}(\Sigma)$
, we denote by
$\Lambda_{\sigma} \subset \mathbb S^{n-1} \times \mathbb S^{n-1}$
the limit set of the self-joining subgroup
$\Sigma_{\sigma} := (\operatorname{{\rm id}} \times \sigma)(\Sigma) \lt \operatorname{{\rm SO}}^\circ(n, 1) \times \operatorname{{\rm SO}}^\circ(n, 1)$
, which is well-defined up to translations. The Hausdorff dimension of
$\Lambda_{\sigma}$
with respect to a Riemannian metric on
$\mathbb S^{n-1}\times \mathbb S^{n-1}$
is equal to
$\max (\dim \Lambda_\Sigma, \dim \Lambda_{\sigma(\Sigma)} )$
, where
$\Lambda_{\Sigma} \subset \mathbb S^{n-1}$
and
$\Lambda_{\sigma(\Sigma)}\subset \mathbb S^{n-1}$
are limit sets of
$\Sigma$
and
$\sigma(\Sigma)$
, respectively, and Hausdorff dimensions are computed with respect to a Riemannian metric on
$\mathbb S^{n-1}$
(see [Reference Kim, Minsky and OhKMO23, Theorem 1.1]).
For a pair (p, q) of positive real numbers, let
$d_{p, q}$
be the premetric on
$\mathbb S^{n-1} \times \mathbb S^{n-1}$
defined as
where
$\xi = (\xi_1, \xi_2), \eta = (\eta_1, \eta_2) \in \mathbb S^{n-1} \times \mathbb S^{n-1}$
and
$d_{\mathbb S^{n-1}}$
is a Riemannian metric on
$\mathbb S^{n-1}$
. We also denote by
$\dim_{p, q}$
the Hausdorff dimension with respect to
$d_{p, q}$
. Let
$\delta_{p,q}(\sigma)$
denote the critical exponent of the series
We deduce the following.
Corollary 9.14.
Let
$\Sigma$
be a non-elementary convex cocompact subgroup of
$\operatorname{{\rm SO}}^\circ(n, 1)$
,
$n\ge 2$
. Let p,q be positive real numbers.
-
(1) For any
$\sigma \in \operatorname{{\rm CC}}(\Sigma)$
, we have
$$\dim_{p, q}\Lambda_{\sigma} =\delta_{p,q}(\sigma).$$
-
(2) For any
$\sigma \in \operatorname{{\rm CC}}(\Sigma)$
, we have and the equality holds if and only if
$$\dim_{p, q} \Lambda_{\sigma} \le \left( \frac{p}{\dim \Lambda_{\Sigma}} + \frac{q}{\dim \Lambda_{\sigma(\Sigma)}} \right)^{-1}$$
$\rho = \operatorname{{\rm id}}$
.
-
(3) Moreover, the map
is an analytic function on any analytic subfamily of
$$\sigma \mapsto\dim_{p, q}\Lambda_{\sigma} $$
$\operatorname{{\rm CC}}(\Sigma)$
. In particular, for
$n=2,3$
, it is analytic on
$\operatorname{{\rm CC}}(\Sigma)$
.
Proof. Identifying the Cartan subspace
$\mathfrak a$
of
$\operatorname{{\rm SO}}^\circ(n, 1) \times \operatorname{{\rm SO}}^\circ(n, 1)$
with
$\mathbb R^2$
and
$\mathfrak a^+$
with
$\mathbb R_{\ge 0}^2$
, consider the linear form
$\Psi\in \mathfrak a^*$
defined by
$\Psi(u_1, u_2)= pu_1+ q u_2$
. Since
$d_{\mathbb S^{n-1}}(\xi, \eta)=e^{-\mathcal G(\xi, \eta)}$
is a
$\operatorname{{\rm SO}}(n)$
-invariant metric and hence a Riemannian metric, where
$\mathcal G$
is the Gromov product on
$\mathbb S^{n-1}\simeq\partial \mathbb H^n$
, we have
$d_{\Psi} = d_{p, q}$
, where
$d_{\Psi}$
is defined in (5.1). Since the opposition involution i is trivial for
$\operatorname{{\rm SO}}^\circ(n, 1) \times \operatorname{{\rm SO}}^\circ(n, 1)$
, the linear form
$\Psi$
is symmetric and hence claims (1) and (3) follow from Corollaries 9.9 and 9.13, respectively, applied to any analytic subfamily of
$ \{(\operatorname{{\rm id}}\times \sigma):\Sigma \to \operatorname{{\rm SO}}^\circ(n, 1) \times \operatorname{{\rm SO}}^\circ(n, 1) : \sigma \in \operatorname{{\rm CC}}(\Sigma)\}$
. For
$n=2,3$
,
$\operatorname{{\rm CC}}(\Sigma)$
is known to be analytic (cf. [Reference BersBer70], [Reference MardenMar74, Theorem 10.8], and [Reference Imayoshi and TaniguchiIT92]). Hence, the last part of claim (3) follows. Claim (2) follows from claim (1) and the following Theorem 9.15.
The following theorem is due to Bishop and Steger [Reference Bishop and StegerBS93, Theorem 2] for
$n=2$
and to Burger [Reference BurgerBur93, Theorem 1(a)] in general. We denote by
$\delta_{\Sigma}$
the critical exponent of
$\Sigma$
, the abscissa of convergence of the Poincaré series
$s \mapsto \sum_{\gamma \in \Sigma} e^{-s d_{\mathbb H^n}(o, \gamma o)}$
.
Theorem 9.15.
For each
$\sigma \in \operatorname{{\rm CC}}(\Sigma)$
, we have
and the equality holds if and only if
$\sigma = \operatorname{{\rm id}}$
.
Proof. We explain how to deduce this from [Reference BurgerBur93, Theorem 1(a)]. We again identify the Cartan subspace
$\mathfrak a$
of
$\operatorname{{\rm SO}}^\circ(n, 1) \times \operatorname{{\rm SO}}^\circ(n, 1)$
with
$\mathbb R^2$
. For each
$i=1,2$
, denote by
$\delta_i$
the
$\alpha_i$
-critical exponent of
$\Sigma_{\sigma} = (\operatorname{{\rm id}} \times \sigma)(\Sigma),$
where
$\alpha_i : \mathfrak a \to \mathbb R$
,
$(u_1, u_2) \mapsto u_i$
. Then,
$\delta_1=\delta_\Sigma$
and
$\delta_{2} = \delta_{\sigma(\Sigma)}$
. If we set
$\alpha_i':= \delta_i \alpha_i$
, then
$\delta_{\alpha_i'}=1$
for each
$i=1,2$
and hence Burger’s theorem [Reference BurgerBur93, Theorem 1(a)] implies that the critical exponent of any convex combination of
$\alpha_1'$
and
$\alpha_2'$
is at most one and is equal to one only when
$\sigma=\operatorname{{\rm id}}$
.
Since
where
$\Psi_0 := ({({p}/{\delta_{1}}) \alpha_1' + ({q}/{\delta_{2}}) \alpha_2'})/({{p}/{\delta_{1}} + {q}/{\delta_{2}}})$
is a convex combination of
$\alpha_1'$
and
$ \alpha_2'$
, we obtain
and the equality holds if and only if
$\sigma = \operatorname{{\rm id}}$
.
Remark 9.16 We remark that in Corollary 9.14, the hypothesis
$p, q\gt 0$
was imposed to be able to consider all
$\sigma \in \operatorname{{\rm CC}}(\Sigma)$
. If we replace
$\operatorname{{\rm CC}}(\Sigma)$
by a subset
$\mathcal D \subset \operatorname{{\rm CC}}(\Sigma)$
, then Corollary 9.14 holds for any
$p, q \in \mathbb R$
such that
$p u_1 + q u_2 \gt 0$
for all non-zero
$(u_1, u_2) \in \mathcal L(\Sigma_\sigma)$
and all
$\sigma \in \mathcal D$
.
10. Hausdorff dimensions with respect to Riemannian metrics
Let G be a connected semisimple real algebraic group. As before, let
$\theta$
be a non-empty subset of the set
$\Pi$
of simple roots of
$(\mathfrak g, \mathfrak a)$
. We denote by
the Hausdorff dimension of
$\Lambda_{\theta}$
with respect to a Riemannian distance
$d_{\rm Riem}$
on
$\mathcal F_{\theta}$
. As any two Riemannian metrics are bi-Lipschitz,
$\dim \Lambda_\theta$
is well-defined independent of the choice of a Riemannian metric. In this section, we present an estimate on
$\dim \Lambda_\theta$
.
10.1 Tits representations and the sum of Tits weights
Let
$\mathbf G$
be the semisimple algebraic group defined over
$\mathbb R$
such that
$G=\mathbf G(\mathbb R)^\circ$
. There exists an exact sequence
$\tilde{\mathbf G}\to_{\tilde p} \mathbf G\to_{\bar p} \bar{\mathbf G},$
where
$\tilde {\mathbf G}$
and
$\bar{\mathbf G}$
are, respectively, simply connected and adjoint semisimple
$\mathbb R$
-groups and
$\tilde p$
and
$\bar p$
are central
$\mathbb R$
-isogenies (see [Reference Borel and TitsBT65] and [Reference MargulisMar91, Proposition 1.4.11]).
Recall that for
$\alpha \in \Pi$
,
$\omega_\alpha$
denotes the (restricted) fundamental weight associated to
$\alpha$
as defined in (2.1). The first part of the following theorem immediately follows as a special case of a theorem of Tits [Reference TitsTit71], and the second part is remarked in [Reference BenoistBen97] and proved in [Reference SmilgaSmi18].
Theorem 10.1 (See [Reference TitsTit71, Theorem 7.2] and [Reference SmilgaSmi18, Lemma 2.13]). For each
$\alpha\in \Pi$
, there exists an irreducible
$\mathbb R$
-representation
${\tilde{\rho}}_{\alpha}: \tilde{\mathbf{G}}\to \operatorname{GL} (\mathbf V_{\alpha}) $
whose highest (restricted) weight
$\chi_{\alpha}$
is equal to
$k_\alpha \omega_\alpha$
for some positive integer
$k_\alpha$
and whose highest-weight space is one-dimensional. Moreover, all weights of
$\tilde\rho_{\alpha}$
are
$\chi_\alpha$
,
$\chi_\alpha-\alpha$
, and weights of the form
$\chi_{\alpha} - \alpha - \sum_{\beta \in \Pi} n_{\beta} \beta$
with
$n_\beta$
non-negative integers.
For each
$\alpha\in \Pi$
, we fix once and for all a representation
$\tilde\rho_\alpha:\tilde{\mathbf{G}}\to \operatorname{GL} (\mathbf V_\alpha)$
as in Theorem 10.1 with minimal
$k_\alpha$
. Since
$\tilde p$
and
$\bar p$
are central isogenies and
$\tilde p(\tilde{\mathbf G}(\mathbb R))=G$
, the representation
$\tilde\rho_\alpha$
induces a projective representation
where
$V_\alpha=\mathbf V_\alpha(\mathbb R)$
. Since the restriction of
$\tilde \rho_\alpha$
to
$\tilde{\mathbf G}(\mathbb R)$
and
$\rho_\alpha$
induce the same representation of the Lie algebra
$\mathfrak g$
to
$\mathfrak {gl}(V_\alpha)$
, their restricted weights are the same. We call
the Tits representation and the Tits weight associated to
$\alpha$
, respectively.
Let
$\rho$
denote the half-sum of all positive roots for
$(\mathfrak g, \mathfrak a)$
counted with multiplicity:
$2\rho =\sum_{\alpha\in \Phi^+} (\dim \mathfrak g^{\alpha} ) \alpha$
. In terms of the restricted fundamental weights
$\omega_\alpha$
, we then have
where
$c_\alpha = \dim \mathfrak g^{\alpha}$
if
$2\alpha$
is not a root, and
$c_\alpha = ({1}/{2})(\dim \mathfrak g^{\alpha} + 2 \dim \mathfrak g^{2 \alpha}) $
otherwise (cf. [Reference BourbakiBou02]). If G is split over
$\mathbb R$
, we have
$\chi_\alpha=\omega_\alpha$
for all
$\alpha\in \Pi$
and hence
$ \sum_{\alpha \in \Pi} \chi_{\alpha}=\rho$
. In general, we do not have this identity, which motivates the following definition.
Definition 10.2.
Define
${\mathsf c}_\theta$
to be the minimum number
$c\ge 0$
such that
We also set
$\mathsf{c}_G := \mathsf{c}_{\Pi}$
.
It is easy to check that
$0\lt \mathsf{c}_{\theta} \le \mathsf{c}_G$
, and, moreover, if
$\theta \cap {\rm i}(\theta) = \emptyset$
, then
$\mathsf{c}_{\theta} \le {\mathsf{c}_G}/{2}$
. By our choice of the Tits representation of G, note that
${\mathsf c}_G$
depends only on the Lie algebra
$\mathfrak g$
; hence, we sometimes write
${\mathsf c}_G=\mathsf{c}_{\mathfrak g}$
. The proof of the following lemma was provided by I. Smilga.
Lemma 10.3.
We have
$\sum_{\alpha\in \Pi} \chi_\alpha \le \rho,$
and hence
Proof. Let
$\mathfrak g_\mathbb C$
be the complexification of
$\mathfrak g=\operatorname{Lie}G$
and
$\mathfrak {h}$
be a Cartan subalgebra of
$\mathfrak g_\mathbb C$
containing
$\mathfrak a$
. Since
$\mathfrak a\subset \mathfrak {h}$
, we have a natural restriction map
$\pi : \mathfrak {h}^* \to \mathfrak a^*$
. Recall the restricted fundamental weights
$\omega_1, \ldots, \omega_s$
defined in (2.1), where
$s=\dim \mathfrak a $
; they form a basis of
$\mathfrak a^*$
. We denote by
$\bar \omega_1, \ldots, \bar \omega_r$
the fundamental weights of
$(\mathfrak g_{\mathbb C}, \mathfrak {h})$
, where
$r=\dim \mathfrak {h}$
, which have been chosen compatibly with
$\omega_j$
values so that
$\pi$
sends each
$\bar \omega_j$
to some linear combination
$\sum_{i} c_{j, i} \omega_i$
, where the
$c_{j, i}$
are non-negative integers. They form a basis of
$\mathfrak {h}^*$
.
Set
$\rho_\mathbb C=\sum_{i=1}^r \bar \omega_i$
, which is equal to the half-sum of all positive roots of
$(\mathfrak g_\mathbb C, \mathfrak {h})$
. Then,
where
$d_i=\sum_j c_{j, i}\in \mathbb N$
. For the Tits weights
$\chi_i=\kappa_i \omega_i$
for
$i=1,\ldots ,s$
, recall that
$\kappa_i$
is the smallest positive integer
$\kappa$
such that
$\kappa \omega_i$
is proximal; that is, its highest-weight space is one-dimensional. In view of the Killing form, we may consider
$\mathfrak a^*$
as a subset of
$\mathfrak {h}^*$
. We have the following facts:
-
– a representation with the highest weight
$\chi\in \mathfrak {h}^*$
is proximal if and only if
$\chi$
actually lies in
$\mathfrak a^*$
(see [Reference Abels, Margulis and SoiferAMS95, Theorem 6.3]); and -
– each coefficient
$\kappa_i$
is either 1 or 2 (see [Reference BenoistBen00, § 2.3]).
We now claim that
$\kappa_i\le d_i$
for all
$1\le i\le s$
; this implies that
$\sum_{i} \chi_i=\sum_i \kappa_i \omega_i\le \rho$
. This is clear if
$\kappa_i=1$
, since
$d_i\ge 1$
. Thus, suppose that
$\kappa_i=2$
and let us show that
$d_i\ge 2$
. Then,
$\chi_i=2 \omega_i$
lies in
$\mathfrak a^*$
and is an integral weight; hence it is equal to some linear combination
$\sum_j c_j \bar \omega_j$
with non-negative integer coefficients
$c_j$
. Moreover, the sum
$\sum_j c_j$
cannot exceed 2, because
$\pi$
has to map
$\sum_j c_j \bar \omega_j$
to
$2 \omega_i$
, and it maps each
$\bar \omega_j$
to some non-zero sum of the
$\omega_k$
. We are left with three cases:
-
(a)
$2 \omega_i = \bar \omega_j$
for some j; -
(b)
$2 \omega_i = \bar \omega_j + \bar \omega_{k}$
for some distinct j and k; and -
(c)
$2 \omega_i = 2 \bar \omega_j$
for some j.
We can rule out case (c), because then
$\omega_i = \bar \omega_j$
would be proximal, which contradicts
$\kappa_i = 2$
. In case (a), we obtain that
$c_{j, i}=2$
and hence
$d_i$
is at least 2. In case (b), applying
$\pi$
on both sides, we necessarily have
$\pi(\bar \omega_j) = \pi(\bar \omega_{k}) = \omega_i$
, so
$c_{j, i} = c_{k, i} = 1$
and hence
$d_i$
is also at least 2.
The bound on
$\mathsf c_{G}$
can be improved in certain cases. For example, for
$\mathfrak g=\mathfrak {so}(n,1)$
,
$n\ge 2$
, we have
$\Pi=\{\alpha\}$
,
$\rho=(({n-1})/{2}) \alpha$
and
$\chi_\alpha=\omega_\alpha={\alpha}/{2}$
; hence
$\mathsf c_{\mathfrak g}={2}/({n-1})$
.
10.2 Riemannian metric on
$\mathcal F_\theta$
For each
$\alpha \in \Pi$
, we denote by
$V_{\alpha}^+$
the highest-weight space of
$\rho_{\alpha}$
and by
$V_{\alpha}^{\lt }$
its unique complementary A-invariant subspace in
$V_{\alpha}$
. Then, the map
$g \in G \mapsto (\rho_{\alpha}(g)V_{\alpha}^+)_{\alpha \in \theta}$
factors through a proper immersion
Let
$\langle \cdot, \cdot \rangle_{\alpha}$
be a K-invariant inner product on
$V_{\alpha}$
with respect to which A is symmetric, so that
$V_{\alpha}^+$
is perpendicular to
$V_{\alpha}^{\lt }$
. We denote by
$\| \cdot \|_{\alpha}$
the norm on
$V_{\alpha}$
induced by
$\langle \cdot, \cdot \rangle_{\alpha}$
. We also use the notation
$\| \cdot \|_{\alpha}$
for a bi-
$\rho_{\alpha}(K)$
-invariant norm on
$\operatorname{GL}(V_{\alpha})$
. The angle
$\angle (E, F)$
between a line E and a subspace F is defined as the minimum of all angles between all non-zero
$v\in E$
and non-zero
$w\in F$
.
We write
$g V_{\alpha}^+ := \rho_{\alpha}(g) V_{\alpha}^+$
and
$g V_{\alpha}^{\lt } := \rho_{\alpha}(g) V_{\alpha}^{\lt }$
for
$g \in G$
and
$\alpha \in \Pi$
. Up to a Lipschitz equivalence, the Riemannian distance
$d_{\rm Riem}$
on
$\mathcal F_\theta=G/P_\theta$
satisfies that for all
$g_1, g_2 \in G$
,
$$d_{\rm Riem}(g_1P_{\theta}, g_2 P_{\theta}) = \sqrt{\sum_{\alpha \in \theta} \sin^2 \angle (g_1 V_{\alpha}^+, g_2 V_{\alpha}^+)}.$$
The Gromov product
$\mathcal G$
on
$\mathcal F^{(2)}$
can be expressed in terms of angles between appropriate subspaces as follows.
Lemma 10.4 (See [Reference QuintQui02b, Lemma 6.4] and [Reference Lee and OhLO23, Lemma 3.11]). For
$(\xi, \eta) \in \mathcal F^{(2)}$
, we have that for any
$\alpha\in \Pi$
,
where
$g\in G$
is such that
$\xi=gP$
and
$\eta=gw_0P$
.
We then have the following estimates on the Riemannian distance using Gromov products and Tits weights.
Lemma 10.5.
There exists a constant
$C\gt 0$
such that for all
$g \in G$
,
$$d_{\rm Riem}(gP_\theta , gw_0P_\theta) \ge C \bigg(\sum_{\alpha \in\theta} e^{-4\chi_\alpha (\mathcal G (g P, g w_0 P))}\bigg)^{\!\!1/2}.$$
Proof. We first note that for each
$\alpha\in \Pi$
,
$w_0 V_{\alpha}^+ \subset V_{\alpha}^{\lt }$
; to see this, recall that
$V_\alpha^\lt $
is the sum of all weight subspaces of
$V_\alpha$
whose weight is not equal to
$\chi_{\alpha}$
. On the other hand,
$w_0 V_{\alpha}^+$
is a weight space with the weight given by
$\chi_{\alpha} \circ \operatorname{{\rm Ad}}_{w_0} = - \chi_{\alpha} \circ {\rm i}$
. Since
$- \chi_{\alpha} \circ {\rm i} (\mathfrak a^+) \le 0$
while
$\chi_{\alpha}(\mathfrak a^+) \ge 0$
, we have
$\chi \circ \operatorname{{\rm Ad}}_{w_0} \neq \chi_{\alpha}$
, which shows
$w_0 V_{\alpha}^+ \subset V_{\alpha}^{\lt }$
.
Therefore, for all
$g\in G$
,
Hence, up to a Lipschitz constant, we have that for all
$g \in G$
,
\begin{align*}d_{\rm Riem}(g P_{\theta}, g w_0 P_{\theta}) & = \sqrt{\sum_{\alpha \in \theta} \sin^2 \angle (g V_{\alpha}^+, gw_0 V_{\alpha}^+)} \\& \ge \sqrt{\sum_{\alpha \in \theta} \sin^2 \angle (g V_{\alpha}^+, gV_{\alpha}^\lt )}\\&= \bigg(\sum_{\alpha \in \theta} e^{-4\chi_\alpha (\mathcal G (g P, g w_0 P))}\bigg)^{\!1/2},\end{align*}
where the last equality follows from Lemma 10.4.
10.3 Lower bounds
In the rest of this section, we assume that
Since the Tits weights
$ \{\chi_{\alpha} : \alpha \in \theta \}$
form a basis of
$\mathfrak a_{\theta}^*$
, each linear form
$\psi \in \mathfrak a_{\theta}^*$
can be uniquely written as
$\psi = \sum_{\alpha \in \theta} \kappa_{\psi, \alpha} \chi_{\alpha}$
with
$\kappa_{\psi, \alpha}\in \mathbb R$
. We consider the following height of
$\psi$
:
Denote by
$\mathsf{E}_{\theta}$
the collection of all linear forms that are non-negative linear combinations of
$\{\chi_{\alpha} :\alpha \in \theta\}$
. That is,
Since
$\chi_\alpha \gt 0$
on
$\operatorname{{\rm int}} \mathfrak a_\theta^+$
for all
$\alpha\in \theta$
, each non-zero
$\psi\in \mathsf{E}_\theta$
is positive on
$\operatorname{{\rm int}} \mathfrak a_{\theta}^+$
. Since
$\mathcal L_\theta - \{0\} \subset \operatorname{{\rm int}}\mathfrak a_\theta^+$
by Theorem 3.8(2), each non-zero
$\psi\in \mathsf{E}_\theta$
is positive on
$\mathcal L_\theta-\{0\}$
and hence we have the corresponding conformal premetric
$d_\psi$
on
$\Lambda_\theta$
discussed in § 5.
Lemma 10.6.
For any non-zero
$\psi \in \mathsf{E}_{\theta}$
, the identity map
$(\Lambda_{\theta}, d_{\rm Riem}) \to (\Lambda_{\theta}, d_{\psi})$
is bi-Hölder. More precisely, we have for some
$c_1, c_2 \gt 0$
so that
where
$r_{\Gamma, \psi} \gt 0$
is defined in (10.6).
Proof. By [Reference Bridgeman, Canary, Labourie and SambarinoBCL+15, Theorem 6.1], there exists
$c, h_{\Gamma} \gt 0$
such that
$d_{\rm Riem}(\xi, \eta) \le c e^{-h_{\Gamma} ( \xi, \eta )_e}$
for all
$\xi\ne \eta\in \Lambda_\theta\simeq \partial \Gamma$
. Together with Lemma 7.5, this implies the first inequality with
For each
$\xi \neq \eta \in \Lambda_{\theta}$
, there exists
$g \in G$
such that
$\xi = g P_{\theta}$
and
$\eta = g w_0 P_{\theta}$
(Theorem 3.8(4)). By Lemma 10.5, we have that for each
$\alpha \in \theta$
, up to a Lipschitz constant,
\begin{equation} d_{\rm Riem}(\xi, \eta) \ge \bigg(\sum_{\alpha \in \theta} e^{-4\chi_\alpha (\mathcal G (g P, g w_0 P))}\bigg)^{\!1/2} \ge e^{-2\chi_\alpha (\mathcal G (g P, g w_0 P))}. \end{equation}
Recalling
and writing
$\psi=\sum_{\alpha\in \theta} \kappa_{\psi, \alpha}\chi_\alpha\in \mathsf{E}_\theta$
, since all
$\kappa_{\psi, \alpha}$
are non-negative, (10.7) implies that
up to a Lipschitz constant. Hence, the second inequality follows.
Remark 10.7. Since
$d_{\psi}$
and
$d_{\bar \psi}$
are bi-Lipschitz (Proposition 5.5), Proposition 6.8 and the above lemma imply that there exist
$c, R \gt 0$
such that for any
$\xi \in \Lambda_{\theta}$
and
$g \in [e,\xi]$
in
$\Gamma$
, the shadow
$O_{R}^{\theta}(o, g o) \cap \Lambda_{\theta}$
contains the Riemannian ball of center
$\xi$
and of radius
$c e^{-{2}/{\kappa_{\psi}}\mathsf{d}_{\psi}(o, go)}$
.
Theorem 10.8.
For any non-zero
$\psi \in \mathsf{E}_{\theta}$
, we have
In particular,
Proof. It follows from Lemma 10.6 and a standard property of Hausdorff dimension that we obtain
Since
$\dim_{\psi}\Lambda_\theta= \delta_{\bar \psi}$
by Corollary 9.9, the claim follows.
Applying Theorem 10.8 to each
$\chi_{\alpha}$
,
$\alpha\in \theta$
, we obtain the following uniform lower bound on the Hausdorff dimension of all non-elementary
$\theta$
-Anosov subgroups.
Corollary 10.9. We have
Example 10.10. For
$G = \operatorname{{\rm PSL}}_n(\mathbb R)$
, we have
$\Pi = \{\alpha_1, \ldots, \alpha_{n-1} \},$
where
Let
$1\le p\le n-1$
. Since
$\chi_{\alpha_p}$
is equal to the fundamental weight
$\omega_p,$
which is given by
$\omega_p(\operatorname{{\rm diag}}(a_1, \ldots, a_n))= a_1 + \cdots + a_p$
, we deduce from Corollary 10.9 that for all non-elementary
$\alpha_p$
-Anosov subgroups of
$\operatorname{{\rm PSL}}_n(\mathbb R)$
, we have
When
$p = 1$
, this lower bound is obtained in [Reference Dey and KapovichDK22, Theorem 10.1].
The following upper bound in Proposition 10.11 was obtained in [Reference Pozzetti, Sambarino and WienhardPSW23, Theorem B] and [Reference Canary, Zhang and ZimmerCZZ26, Theorem 1.2] for
$G = \operatorname{{\rm PSL}}_n(\mathbb R)$
and
$\theta$
is a singleton.
Proposition 10.11. We have
Proof. Via the proper immersion of
$\mathcal F_{\theta}$
into
$\prod_{\alpha \in \theta} \mathbb{P}(V_{\alpha})$
as discussed in (10.4), we may consider the following metric on
$\mathcal F_{\theta}$
: for
$g_1, g_2 \in G$
,
where
$d_{\mathbb{P}(V_{\alpha})}$
is the metric on
$\mathbb{P}(V_{\alpha})$
given by
$d_{\mathbb{P}(V_{\alpha})}(v_1, v_2) = \sin \angle (v_1, v_2)$
. Then,
$d_{\mathcal F_{\theta}}$
is Lipschitz equivalent to the Riemannian distance on
$\mathcal F_\theta$
and hence we can use
$d_{\mathcal F_{\theta}}$
to compute
$\dim \Lambda_{\theta}$
.
Fix
$\alpha\in \theta$
and consider the Tits representation
$(\rho_\alpha, V_\alpha)$
. We write
$V_\alpha=\mathbb R^{n_\alpha}$
and
$\operatorname{{\rm PGL}}(V_{\alpha})=\operatorname{{\rm PGL}}_{n_\alpha}(\mathbb R)$
by fixing a basis. We denote by
$\beta_{1,\alpha}$
the simple root of
$\operatorname{{\rm PGL}}_{n_\alpha}(\mathbb R)$
given by
$\beta_{1,\alpha}(\operatorname{{\rm diag}}(u_1, \ldots, u_{n_\alpha}))=u_1-u_2.$
Since the highest weight of
$\rho_\alpha$
is
$\chi_{\alpha}$
and the second highest weight is
$\chi_{\alpha}-\alpha $
by Theorem 10.1, we have that for all
$\gamma\in \Gamma$
,
Since
$\Gamma$
is an
$\{\alpha\}$
-Anosov subgroup of G, there exists
$C\gt 1$
such that for all
$\gamma \in \Gamma$
,
$\alpha(\mu(\gamma)) \ge C^{-1}|\gamma|-C $
, and hence
$\beta_{1,\alpha}(\mu(\rho_{\alpha}(\gamma))) \ge C^{-1}|\gamma|-C$
. Therefore,
$\rho_\alpha (\Gamma)$
is a
$\{\beta_{1, \rho}\}$
-Anosov subgroup of
$\operatorname{{\rm PGL}}_{n_\alpha}(\mathbb R)$
.
We denote by
$f_{\alpha} : \partial \Gamma \to \mathbb{P}(V_{\alpha})$
the
$\rho_{\alpha}(\Gamma)$
-equivariant embedding obtained as the extension of the orbit map of
$\rho_{\alpha}(\Gamma)$
(Theorem 3.8(4)). It is shown in [Reference Pozzetti, Sambarino and WienhardPSW23, Proposition 3.5, Proposition 3.8] that there exists a constant
$C_{\alpha} \gt 0$
such that for each
$\gamma \in \Gamma$
, there exists a ball
$\mathcal {B}_{\alpha}(\gamma)$
of radius
$C_{\alpha} e^{-\beta_{1, \rho}(\mu(\rho_{\alpha}(\gamma)))}$
in
$\mathbb{P}(V_{\alpha})$
so that for any
$x \in \partial \Gamma$
such that
$\gamma \in [e, x]$
in
$\Gamma$
, we have
$f_{\alpha}(x) \in \mathcal {B}_{\alpha}(\gamma)$
. In particular, for every
$k \ge 1$
, the collection
covers the limit set of
$\rho_{\alpha}(\Gamma)$
in
$\mathbb{P}(V_{\alpha})$
. Hence,
$\Lambda_{\theta}$
is covered by the collection
$$\bigg\{\prod_{\alpha \in \theta} \mathcal {B}_{\alpha}(\gamma) : \gamma \in \Gamma, |\gamma| = k \bigg\}$$
via the immersion
$\mathcal F_{\theta} \to \prod_{\alpha \in \theta} \mathbb{P}(V_{\alpha})$
. Since
$\prod_{\alpha \in \theta} \mathcal {B}_{\alpha}(\gamma)$
has
$d_{\mathcal F_\theta}$
-diameter at most
where
$C = \max_{\alpha \in \theta} C_{\alpha}$
by (10.8), we have that for each
$s \gt 0$
, the s-dimensional Hausdorff measure
$\mathcal H^s(\Lambda_\theta)$
with respect to
$d_{\mathcal F_\theta}$
satisfies
Therefore, denoting by
$\delta_{\min_{\alpha \in \theta} \alpha}$
the abscissa of convergence of the series
$s \mapsto \sum_{\gamma \in \Gamma} e^{-s \min_{\alpha \in \theta} \alpha(\mu(\gamma))}$
, if
$s \gt \delta_{\min_{\alpha \in \theta} \alpha}$
, we have
$ \mathcal H^s(\Lambda_\theta)=0$
and hence
On the other hand, we have
$$\frac{1}{\# \theta} \sum_{\alpha \in \theta} \sum_{\gamma \in \Gamma} e^{- s \alpha(\mu(\gamma))} \le \sum_{\gamma \in \Gamma} e^{-s \min_{\alpha \in \theta} \alpha(\mu(\gamma))} \le \sum_{\alpha \in \theta} \sum_{\gamma \in \Gamma} e^{-s \alpha(\mu(\gamma))}.$$
The first inequality implies
$\max_{\alpha \in \theta} \delta_{\alpha} \le \delta_{\min_{\alpha \in \theta} \alpha}$
and the second gives
$\delta_{\min_{\alpha \in \theta} \alpha} \le \max_{\alpha \in \theta} \delta_{\alpha}$
. Hence,
$\delta_{\min_{\alpha \in \theta} \alpha} = \max_{\alpha \in \theta} \delta_{\alpha}$
, which completes the proof.
Theorem 1.7 is a combination of Corollary 10.9 and Proposition 10.11.
11. Growth indicator bounds and applications to the
$L^2$
-spectrum
As before, let
$\Gamma\lt G$
be a
$\theta$
-Anosov subgroup where G is a connected semisimple real algebraic group. In this final section, we deduce bounds on the growth indicator
$\psi_\Gamma^\theta:\mathfrak a_\theta\to [0, \infty)\cup\{-\infty\}$
of
$\Gamma$
(see Definition 3.1) from Corollary 10.9. Recall Tits weights
$\chi_\alpha$
,
$\alpha\in \Pi$
, of G from (10.2). We have the following (Corollary 1.8).
Corollary 11.1. We have
Moreover,
Proof. For any linear form
$\psi\in \mathfrak a_{\theta \cup {\rm i}(\theta)}^*$
positive on
$\mathcal L_{\theta \cup {\rm i}(\theta)} - \{0\}$
, the scaled linear from
$\delta_{\psi} \psi$
is tangent to the growth indicator (Lemma 3.6). Hence it follows from Corollary 10.9 that for each
$\alpha \in \theta$
, we have
Therefore, taking the minimum among
$\alpha \in \theta$
finishes the proof of (11.1).
By [Reference Kim, Oh and WangKOW25b, Lemma 3.12], we have
Hence, by (11.1), we have
Since the linear form
$\chi_{\alpha} + \chi_{{\rm i}(\alpha)} \in \mathfrak a_{\theta \cup {\rm i}(\theta)}^*$
is
$p_{\theta \cup {\rm i}(\theta)}$
-invariant for each
$\alpha \in \theta$
, (11.2) follows.
Observing
Corollary 11.1 implies the following.
Corollary 11.2.
For any
$\theta$
-Anosov subgroup of G, we have
Remark 11.3. We remark that our proof shows that
${{\mathsf c}_\theta }/{\# \theta }$
in the above corollary can be replaced by the minimum
$c\ge 0$
such that
$\min_{\alpha \in \theta} ( \chi_{\alpha} + \chi_{{\rm i}(\alpha)} ) \le c \cdot \rho $
on the limit cone
$\mathcal L$
.
Define the real number
$\lambda_0(\Gamma\backslash X) \in [0,\infty)$
as follows:
\begin{equation} \lambda_0(\Gamma\backslash X):= \inf\left\lbrace \frac{\int_{\Gamma\backslash X}\|\text{grad} \, f \|^2\,d\operatorname{Vol}}{\int_{\Gamma\backslash X}|f|^2\,d\operatorname{Vol}}\,:\,f\in C^\infty_c(\Gamma\backslash X),\; f\neq 0 \right\rbrace\!.\end{equation}
This number is equal to the bottom of the
$L^2$
-spectrum of
$\Gamma \backslash X$
of the Laplace–Beltrami operator [Reference SullivanSul87, Theorem 2.2]. The following was proved in [Reference Edwards and OhEO23, Theorem 1.6] for
$\Pi$
-Anosov subgroups and in [Reference Lutsko, Weich and WolfLWW24, Corollary 3] in general.
Theorem 11.4.
If
$\Gamma\lt G$
is a torsion-free discrete subgroup of G with
$\psi_\Gamma \le \rho$
, then
$L^2(\Gamma \backslash G)$
is tempered and
$\lambda_0(\Gamma\backslash X) = \| \rho\|^2$
.
Applying Theorem 11.4, we obtain the following (Corollary 1.9) from (11.3).
Corollary 11.5.
Let
$\Gamma$
be a torsion-free
$\theta$
-Anosov subgroup. If
$ \dim \Lambda_{\theta} \le {\# \theta}/{{\mathsf c}_\theta}$
, then
$L^2(\Gamma \backslash G)$
is tempered and
$\lambda_0(\Gamma\backslash X) = \| \rho\|^2$
.
Moreover,
$\lambda_0$
is not an
$L^2$
-eigenvalue [Reference Edwards and OhEO23, Reference Edwards, Fraczyk, Lee and OhEFL+24] (see also [Reference Weich and WolfWW23, Corollary 5.2] for the absence of any principal joint
$L^2$
-eigenvalues as well).
Remark 11.6. Indeed, it is shown in [Reference Lutsko, Weich and WolfLWW24, Theorem 11] that if
$\psi_\Gamma \le (2-{2}/{p}) \rho$
for some
$p \ge 1$
, then
$L^2(\Gamma\backslash G)$
is strongly
$L^{p+\varepsilon}$
-integrable for all
$\varepsilon\gt 0$
; that is, for a dense subset of vectors, the associated matrix coefficients belong to
$L^{p+\varepsilon}(G)$
. Hence, if
$ \dim \Lambda_{\theta} \le (2- {2}/p) {\# \theta}/{{\mathsf c}_\theta}$
, we obtain that
$L^2(\Gamma\backslash G)$
is strongly
$L^{p+\varepsilon}$
-integrable for all
$\varepsilon\gt 0$
.
Remark 11.7. Using that
$\mathsf c_G = {2}/({n-1})$
for
$G = \operatorname{{\rm SO}}^\circ(n, 1)$
, Corollary 11.5 says that for a Zariski dense convex cocompact
$\Gamma \lt \operatorname{{\rm SO}}^\circ(n, 1)$
, if
$\dim \Lambda \le ({n-1})/{2}$
, then
$L^2(\Gamma \backslash \operatorname{{\rm SO}}^\circ(n, 1))$
is tempered and
$\lambda_0(\Gamma \backslash \mathbb H^n) = {(n-1)^2}/{4}$
, as shown by Sullivan [Reference SullivanSul87, Theorem 2.21].
Acknowledgement
We would like to thank Ilia Smilga for providing the proof of Lemma 10.3.
Conflicts of interest
None.
Financial support
Oh is partially supported by the NSF grant no. DMS-1900101 and 2450703.
Journal information
Compositio Mathematica is owned by the Foundation Compositio Mathematica and published by the London Mathematical Society in partnership with Cambridge University Press. All surplus income from the publication of Compositio Mathematica is returned to mathematics and higher education through the charitable activities of the Foundation, the London Mathematical Society and Cambridge University Press.
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