Hostname: page-component-76d6cb85b7-pn7tm Total loading time: 0 Render date: 2026-07-17T06:48:55.089Z Has data issue: false hasContentIssue false

Dynamics of proteins in solution

Published online by Cambridge University Press:  13 June 2019

Marco Grimaldo
Affiliation:
Institut Max von Laue - Paul Langevin, 71 avenue des Martyrs, 38042 Grenoble, France Institut für Angewandte Physik, Universität Tübingen, Auf der Morgenstelle 10, 72076 Tübingen, Germany
Felix Roosen-Runge*
Affiliation:
Institut Max von Laue - Paul Langevin, 71 avenue des Martyrs, 38042 Grenoble, France Division for Physical Chemistry, Lund University, Naturvetarvägen 14, 22100 Lund, Sweden
Fajun Zhang
Affiliation:
Institut für Angewandte Physik, Universität Tübingen, Auf der Morgenstelle 10, 72076 Tübingen, Germany
Frank Schreiber
Affiliation:
Institut für Angewandte Physik, Universität Tübingen, Auf der Morgenstelle 10, 72076 Tübingen, Germany
Tilo Seydel*
Affiliation:
Institut Max von Laue - Paul Langevin, 71 avenue des Martyrs, 38042 Grenoble, France
*
Author for correspondence: Felix Roosen-Runge, E-mail: felix.roosen-runge@fkem1.lu.se; Tilo Seydel, E-mail: seydel@ill.eu
Author for correspondence: Felix Roosen-Runge, E-mail: felix.roosen-runge@fkem1.lu.se; Tilo Seydel, E-mail: seydel@ill.eu
Rights & Permissions [Opens in a new window]

Abstract

The dynamics of proteins in solution includes a variety of processes, such as backbone and side-chain fluctuations, interdomain motions, as well as global rotational and translational (i.e. center of mass) diffusion. Since protein dynamics is related to protein function and essential transport processes, a detailed mechanistic understanding and monitoring of protein dynamics in solution is highly desirable. The hierarchical character of protein dynamics requires experimental tools addressing a broad range of time- and length scales. We discuss how different techniques contribute to a comprehensive picture of protein dynamics, and focus in particular on results from neutron spectroscopy. We outline the underlying principles and review available instrumentation as well as related analysis frameworks.

Information

Type
Review
Creative Commons
Creative Common License - CCCreative Common License - BYCreative Common License - NCCreative Common License - ND
This is an Open Access article, distributed under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives licence (http://creativecommons.org/licenses/by-nc-nd/4.0/), which permits non-commercial re-use, distribution, and reproduction in any medium, provided the original work is unaltered and is properly cited. The written permission of Cambridge University Press must be obtained for commercial re-use or in order to create a derivative work.
Copyright
Copyright © The Author(s) 2019
Figure 0

Fig. 1. Sketch of different types of protein dynamics. Left: The rotation and translation of the entire protein occurs on timescales of nanoseconds to seconds and lengthscales from nanometers to micrometers. Domain fluctuations occur on timescales of several nanoseconds to milliseconds with amplitudes from some Ångströms to about a nanometer. Right: Localized and confined diffusive relaxations occurring on a timescale of picoseconds to nanoseconds and a subnanometer length scale, as well as vibrations occurring on the femto- to pico-second timescale with amplitudes up to a few Ångströms are depicted. The IgG protein (Harris et al., 1997) was rendered using Mathematica (Wolfram Research, Inc.) and the figure was produced using Mathematica (Wolfram Research, Inc.) and Gimp (Spencer Kimball and the GIMP Development Team).

Figure 1

Fig. 2. Sketch of the diffusive MSD W(t) as a function of time. For very short times, W(t) ~ t2. For tB < t < tI, $W\lpar t \rpar \sim D_{\rm s}^{\lpar {\rm s} \rpar } \,t$, and for t ≫ tI, $W\lpar t \rpar \sim D_l^{\lpar {\rm s} \rpar } \,t$. τI is the typical interaction time, i.e. the time on which proteins collide.

Figure 2

Table 1. Comparison between several techniques in the context of dynamics of proteins in solution

Figure 3

Fig. 3. Accessible length- and time-scales of typical scattering techniques.

Figure 4

Fig. 4. Schematic representation of a scattering event. An incoming neutron with initial wavevector ${\bf k}_i$ interacts with an atomic nucleus and is scattered at an angle 2θ. After the event, its wavevector is ${\bf k}_f$. The scattering vector ${\bf q}$ is defined as the difference between ${\bf k}_f$ and ${\bf k}_i$. Figure rendered using Mathematica (Wolfram Research, Inc.).

Figure 5

Table 2. Coherent (σcoh), incoherent (σinc) and absorption (σa) neutron cross-sections in barns of the elements comprising proteins and common salts in biological environments (Sears, 1992)

Figure 6

Fig. 5. Sketch of the scattering function of elastic, quasi-elastic and inelastic neutron scattering near room temperature, in the absence of so-called detailed-balance effects. Elastic scattering gives a very sharp peak centered at ω = 0. QENS yields a broader peak centered at ω = 0, while the scattering function of inelastic scattering is characterized by peaks centered at ω ≠ 0. Figure rendered using Mathematica (Wolfram Research, Inc.).

Figure 7

Fig. 6. Simplified schematic representation of a TOF spectrometer at a reactor neutron source: a continuous ‘white’ neutron beam enters from the far left, passing a series of chopper disks (marked by the numbers 1–3). The total of six choppers in the chosen example setup are, from left, a pair of counter-rotating pulse choppers (1) chopping the continuous neutron beam into short pulses, the so-called contamination order and frame overlap choppers (2), and the pair of counter-rotating monochromator choppers (3). Each chopper carries a slit with an opening on its circumference that has an open area equal to the neutron guide cross-section area. The remainder of the chopper disk area absorbs neutrons. The counter-rotating chopper pairs serve to minimize the opening and closing times, thus enhancing the energy resolution. The sample (small red cylinder, 4) is located close to the last downstream chopper (3), typically tens of meters away from the pulse choppers. The detectors (long cyan cylindrical tubes, 5) cover a large solid angle at a neutron flight distance of several meters from the sample to simultaneously detect neutrons at multiple scattering angles. Figure rendered using Mathematica (Wolfram Research, Inc.).

Figure 8

Table 3. Neutron spectrometers with characteristics suitable for protein dynamics

Figure 9

Fig. 7. Schematic representation of the backscattering spectrometer IN16B at the ILL. A polychromatic (‘pink’) neutron beam (dashed line) illuminates the so-called PST (disk in the figure marked by ‘1’), which reflects the beam toward the backscattering monochromator (far bottom left, 2). This single crystal sends the monochromatic neutrons back toward the PST (1), which lets pass this neutron bunch via an open segment in the disk toward the sample (illustrated by the small cylinder, 3). The scattered neutrons are analyzed by the large crystals mounted on the surface of a sphere with a radius of 2 m, and the sample at its center (right part of the image, 4). The analyzed neutrons are detected by the detector tubes mounted right behind the sample (5). Figure rendered using Mathematica (Wolfram Research, Inc.), adapted from Hennig (2011).

Figure 10

Fig. 8. Schematic of the principle of a backscattering spectrometer. In the example, a neutron with energy E0 + δE is delivered to the sample, where E0 is the energy in backscattering from the analyzer crystals. After scattering by the sample, if the energy transfer equals − δE the neutron is reflected by the analyzers and detected; if the energy transfer differs from − δE the neutron is not reflected and is usually absorbed by absorbing material placed behind the analyzers. The thickness of the sample is chosen such that the probability for a neutron to be scattered once is $\sim 10{\rm \%} $ and that of being scattered twice is hence $\sim \!1{\rm \%} $. The distance from the sample to the analyzers is typically 2 m, while the distance from the sample to the detectors amounts to <0.2m. Figure rendered using Mathematica (Wolfram Research, Inc.).

Figure 11

Fig. 9. Simplified schematic representation of a spin echo spectrometer. A neutron beam with a typical wavelength spread of $\Delta \lambda /\lambda \approx 8{\rm \%} $ impinges from the left and first passes a polarizer and π/2- (i.e. 90°-)spin-flipper (marked by ‘1’). In a classical picture, this device ‘flips’ the neutron spin axis to be perpendicular to their flight axis. The beam subsequently enters a first, homogeneous magnetic field, illustrated by the schematic cylindrical coil (2). The neutron spins precess in this first magnetic field, as indicated by the arrows perpendicular to the optical axis and illuminate the sample (3) illustrated by the square box. The scattered neutrons pass _a_ π-spin flipper behind the sample (4) to invert their spin and enter a second, equivalent magnetic field indicated by the cylindrical coil on the right side of the figure (5), where they precess again and finally pass a π/2-flipper and polarization analyzer (6) and hit the detector (7). If the neutrons are elastically scattered by the sample, they will have the same polarization in (6) as they have had in (1) due to this symmetric setup. In contrast, any change in their velocity by the scattering in the sample will change their initial polarization. The scattering angle 2Θ is adjusted by rotating the arm (4–7) around the sample (3). Figure rendered using Mathematica (Wolfram Research, Inc.), adapted from Hennig (2011).

Figure 12

Fig. 10. Graphical representation of a normal mode of IgG (Harris et al., 1997) obtained through the anisotropic network model for CG normal mode analysis (Eyal et al., 2015).

Figure 13

Fig. 11. Comparison of the HWHM Γ as a function of q2 for Fickian diffusion and jump-diffusion. For Fickian diffusion Γ = Dq2: a straight line is obtained and the slope gives the diffusion coefficient D. For unrestricted jump-diffusion, the slope at low q gives the jump-diffusion coefficient D1, and the asymptote at high q gives the inverse of the residence time τ0. Figure rendered using Mathematica (Wolfram Research, Inc.).

Figure 14

Table 4. Effective force constants (Eq. (61)) of proteins in solution from different studies

Figure 15

Table 5. Parameters on protein internal dynamics obtained from TOF and NBS studies

Figure 16

Table 5b. Parameters on protein internal dynamics obtained from TOF and NBS studies (continued from page 23)

Figure 17

Table 6. Relaxation times and amplitudes of protein internal modes obtained from NSE studies

Figure 18

Fig. 12. Average mean-square displacements $ \langle u^2 \rangle $ of hydrogen atoms in Mb hydrated powder. Figure adapted and reproduced with permission from Doster et al. (1989). Copyright Nature Publishing Group.

Figure 19

Fig. 13. HWHM, Γ, of the internal motion Lorentzian L(Γ, ω), for Mb samples. The lines are guide to the eye. Except for the dry Mb sample, Γ increases with q2, which characterizes the presence of local diffusive motions as soon as the protein is hydrated. In the case of dry Mb, Γ is almost constant, as expected from a reorientational type of motion. The inverse of Γ gives the correlation time of the motions. In solutions, the correlation time extrapolated at q = 0 is ~4.4  ps, less than half of that in powders. Figure adapted and reproduced with permission from Pérez et al. (1999). Copyright Elsevier.

Figure 20

Fig. 14. Sketch of the gradual dynamics activation from protein powders to proteins in solution. Numerous studies indicate that, generally, additional dynamics is present in proteins in solution compared with hydrated protein powders, which in turn are characterized by additional types of motions compared with dry protein powders. IgG (Harris et al., 1997) was rendered using PyMol (DeLano, 2002) and the figure was produced with Gimp (Spencer Kimball and the GIMP Development Team).

Figure 21

Fig. 15. (a) EISF of: BLA (black squares) and MBLA (empty circles). Although a better fit to the EISF was achieved with a two-sphere model, the one sphere model (Eq. (40)) was used in Bu et al. (2000) to describe the change in the effective radius of restricted motions. (b) q dependence of HWHM Γ of the quasi-elastic Lorentzian peak of: BLA (black squares) and MBLA (empty circles). Clear differences are visible between the two states of the protein. Figure adapted and reproduced with permission from Bu et al. (2000). Copyright Elsevier.

Figure 22

Fig. 16. HWHM Γ of the Lorentzian accounting for the internal motion of Hb from (a) platypus Hb, (b) chicken Hb, (c) crocodile Hb, as a function of the squared scattering vector q2. The solid lines are fits according to a jump-diffusion model in the range of 0.64 ⩽ q2 ⩽ 3.24 Å−2. The horizontal solid lines indicate the region of constant half-widths. Figure reproduced with permission from Stadler et al. (2014a). Copyright Elsevier.

Figure 23

Fig. 17. (a) Difference of the corrected diffusion coefficients $D_{eff}^{0}(q)$ and the calculated translational or rotational diffusion coefficient. (b) Diffusion form factor of the normal modes 7 and 11 for the protein configuration with and without the cofactor. (c) Top – Motional pattern of mode 7: without cofactor the exterior domain (catalytic domain) tilts outward and opens the cleft. The inner domain with connection points between the monomers remains stiff. Bottom: Motional pattern of mode 11: with and without the bound cofactor the monomers within a dimer exhibit torsional motion around the long dimer axis (in the image plane), which is more pronounced with the cofactor. Figure reproduced with permission from (Biehl et al., 2008). Copyright American Physical Society.

Figure 24

Fig. 18. Translational self-diffusion coefficients Dt normalized by the dilute limit diffusion coefficient Dt(0) (circles) for two different temperatures (red and purple circles denote 280 and 300 K, respectively) after separation of the rotational contributions. The purple line superimposed on the data is a guide to the eye obtained from a polynomial fit indicating the temperature-independent master-curve. The top and bottom dashed purple lines indicate the upper and lower 96% prediction bounds, respectively. The blue lines denote the colloidal short-time self-diffusion for hard spheres (light blue, solid) and charged spheres (dark blue, dashed). The inset in the top right corner illustrates the flow field (light blue stream line plot) generated by the movement of three spheres (velocities are denoted by blue arrows) and therefore experiencing hydrodynamic forces (pink arrows). Figure reproduced with permission from Roosen-Runge et al. (2011). Copyright National Academy of Sciences of the United States of America.

Figure 25

Fig. 19. Comparison of normalized long-time self-diffusion coefficient, $D_{{\rm s}\_{\rm L}}/D_0$ and normalized short-time self-diffusion coefficient, Ds/D0, as a function of volume fraction. Figure reproduced with permission from Liu et al. (2010). Copyright American Chemical Society.