To save content items to your account,
please confirm that you agree to abide by our usage policies.
If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account.
Find out more about saving content to .
To save content items to your Kindle, first ensure no-reply@cambridge.org
is added to your Approved Personal Document E-mail List under your Personal Document Settings
on the Manage Your Content and Devices page of your Amazon account. Then enter the ‘name’ part
of your Kindle email address below.
Find out more about saving to your Kindle.
Note you can select to save to either the @free.kindle.com or @kindle.com variations.
‘@free.kindle.com’ emails are free but can only be saved to your device when it is connected to wi-fi.
‘@kindle.com’ emails can be delivered even when you are not connected to wi-fi, but note that service fees apply.
Abstract topological groups were first defined by Schreier in 1926, though the idea was implicit in much earlier work on continuous groups of transformations. The subject has its origins in Klein's programme (1872) to study geometries through the transformation groups associated with them, and in Lie's theory of continuous groups arising from the solution of differential equations. The ‘classical groups’ of geometry (general linear groups, unitary groups, symplectic groups, etc.) are in fact Lie groups, that is, they are analytic manifolds and their group operations are analytic functions. On the other hand, Killing and Cartan showed (1890) that all simple Lie groups are classical groups, apart from a finite number of exceptional groups.
In 1900 Hilbert posed the problem (No. 5 of his famous list) whether every continuous group of transformations of a finite-dimensional real or complex space is a Lie group. The twentieth-century habit of axiomatising everything led to a more abstract formulation of this problem. A topological group is a topological space which is a group with continuous group operations, and the question is: What topological conditions on a topological group will ensure that it has an analytic structure which makes it a Lie group? Since integration was a major tool in the study of Lie groups, especially their representations, it became important to establish the existence of appropriate integrals on general classes of topological groups.
In 1969, and again in 1972, I gave an introductory course on topological groups at the University of London. The audience consisted largely of first-year postgraduate students in algebra or number theory and the course was designed to meet their needs, which I took to be a knowledge of basic facts about various general types of topological groups and enough about the Haar integral to enable them to appreciate its use in such contexts as representation theory and algebraic number theory. Some of the students had little or no background in topology and for this reason topological concepts were developed ab initio, whereas the rudiments of group theory were assumed.
After the 1969 course there was some demand from new students for copies of the notes and so it was decided to produce a duplicated set of notes of the 1972 lectures. I am extremely grateful to Robert Coates, Michael Rutter and Anthony Solomonides for all their hard work in preparing the mimeographed version on which the present notes are based. I have made a number of minor changes and amplified some passages when this seemed advisable for a wider audience. I have also added an informal section on the representation theory of compact groups which I intended to include in the course but for which there was no time. Its purpose is to illustrate one practical application of the Haar integral and to encourage further reading.
We seek to construct an ‘integral’ on a locally compact group. This may be done by a variety of methods; we wish to avoid measure-theoretic methods and so we take as our model the construction of the Riemann integral on (R, +). There we have the set R of all Riemannintegrable functions (vanishing outside some interval), and a map ∫ : R → R defined by
which satisfies:
(i) Linearity: ∫(λf + μg) = μ∫g.
(ii) Positivity: f ≥ 0 ⇒ ∫f ≥ 0.
(iii) Translation-invariance: if for some fixed a ∈ R and all x ∈ R, g(x) = f (x + a) then
∫g = ∫f.
These three properties actually characterize the Riemann integral up to a scalar multiple. (Exercise.) The same is true if we consider only continuous functions on R, and this suggests that we should try to construct, for more general groups, an integral with similar properties for realvalued continuous functions.
From now on we shall only consider locally compact spaces and groups, and we shall always assume that they are Hausdorff.
For a space X, K(X) denotes the set of all continuous functions X → R with compact support, where
We use programmes for the Todd-Coxeter coset enumeration algorithm and the modified Todd-Coxeter coset enumeration algorithm to investigate a class of generalised Fibonacci groups. In particular we use these techniques to discover a finite non-metacyclic Fibonacci group and to study its structure.
1. In this paper we study the asymptotic behaviour of solutions of algebraic equations with real functions as coefficients, using mainly algebraic properties of the class to which the coefficients belong. To that end we introduce the notion of an m-group of functions and prove the main theorem by a procedure originated in [1]. As a corollary we obtain sufficient conditions for a class F of functions to possess the property that solutions of algebraic equations with coefficients in F are again members of F. We conclude by applying these results to the classical Hardy's logarithmico-exponential class ℋ [2]
As is well known, the deficiency indices of the minimal symmetric differential operator of even order 2m with real coefficients on the half-line lie within the limits m and 2m, and are equal. I. M. Glazman [6] first showed, by examples, that for such operators the deficiency indices can actually take all the intermediate values m ≦ P ≦ 2m. Subsequently fresh examples of operators with real coefficients, whose deficiency indices take all possible values, were constructed by various authors (S. A. Orlov [11], M. V. Fedoryuk [4], and others).
Although integral equations and relations for ellipsoidal wave functions have been known for some time, it had previously been impossible to obtain asymptotic estimates for these integrals, with large wave parameter, as the available asymptotic expansions for the integrand were non-uniform. However, uniform asymptotic expansions have recently been calculated for the functions occurring in the integrand, and these expansions are now used to determine asymptotic expansions for ellipsoidal wave functions of the third kind. A different type of normalisation is proposed for ellipsoidal wave functions and this is compared with previous normalisations by evaluating asymptotically a double integral.
Conjugate points are defined in terms of solutions of a linear fourth-order differential equation satisfying two homogeneous boundary conditions at x = α and either u(β) = u′(β) = 0 or u′(γ) = u″(γ) = 0. The smallest β > α and γ > α such that these boundary conditions are satisfied by a non-trivial solution of the equation are denoted by η(α) and ῆ-(α), respectively. Upper bounds are established for min [η(α), ῆ(α)] relative to the conjugate points of a self-adjoint differential equation which is majorised by the more general equation under study.
An analogue of full-range Fourier series is introduced in the Sturm-Liouville setting and a theorem generalising Wiener's theorem for functions with absolutely convergent Fourier series is proved. The Banach algebra structure of the theory is examined. Use is made of second-order asymptotic formulae for the Sturm-Liouville eigenfunctions.
Concavity arguments have been used by Knops, Levine and Payne [1] to discuss evolutionary properties of weak solutions to an abstract non-linear differential equation in a Hilbert space. These authors demonstrate that provided the non-linearity is suitably restricted and for specified initial data, the norm of the solution becomes unbounded in a finite time. In other words, the solution possesses a finite escape time.