- •Foreword
- •Preface
- •Contents
- •Introduction
- •Oren M. Becker
- •Alexander D. MacKerell, Jr.
- •Masakatsu Watanabe*
- •III. SCOPE OF THE BOOK
- •IV. TOWARD A NEW ERA
- •REFERENCES
- •Atomistic Models and Force Fields
- •Alexander D. MacKerell, Jr.
- •II. POTENTIAL ENERGY FUNCTIONS
- •D. Alternatives to the Potential Energy Function
- •III. EMPIRICAL FORCE FIELDS
- •A. From Potential Energy Functions to Force Fields
- •B. Overview of Available Force Fields
- •C. Free Energy Force Fields
- •D. Applicability of Force Fields
- •IV. DEVELOPMENT OF EMPIRICAL FORCE FIELDS
- •B. Optimization Procedures Used in Empirical Force Fields
- •D. Use of Quantum Mechanical Results as Target Data
- •VI. CONCLUSION
- •REFERENCES
- •Dynamics Methods
- •Oren M. Becker
- •Masakatsu Watanabe*
- •II. TYPES OF MOTIONS
- •IV. NEWTONIAN MOLECULAR DYNAMICS
- •A. Newton’s Equation of Motion
- •C. Molecular Dynamics: Computational Algorithms
- •A. Assigning Initial Values
- •B. Selecting the Integration Time Step
- •C. Stability of Integration
- •VI. ANALYSIS OF DYNAMIC TRAJECTORIES
- •B. Averages and Fluctuations
- •C. Correlation Functions
- •D. Potential of Mean Force
- •VII. OTHER MD SIMULATION APPROACHES
- •A. Stochastic Dynamics
- •B. Brownian Dynamics
- •VIII. ADVANCED SIMULATION TECHNIQUES
- •A. Constrained Dynamics
- •C. Other Approaches and Future Direction
- •REFERENCES
- •Conformational Analysis
- •Oren M. Becker
- •II. CONFORMATION SAMPLING
- •A. High Temperature Molecular Dynamics
- •B. Monte Carlo Simulations
- •C. Genetic Algorithms
- •D. Other Search Methods
- •III. CONFORMATION OPTIMIZATION
- •A. Minimization
- •B. Simulated Annealing
- •IV. CONFORMATIONAL ANALYSIS
- •A. Similarity Measures
- •B. Cluster Analysis
- •C. Principal Component Analysis
- •REFERENCES
- •Thomas A. Darden
- •II. CONTINUUM BOUNDARY CONDITIONS
- •III. FINITE BOUNDARY CONDITIONS
- •IV. PERIODIC BOUNDARY CONDITIONS
- •REFERENCES
- •Internal Coordinate Simulation Method
- •Alexey K. Mazur
- •II. INTERNAL AND CARTESIAN COORDINATES
- •III. PRINCIPLES OF MODELING WITH INTERNAL COORDINATES
- •B. Energy Gradients
- •IV. INTERNAL COORDINATE MOLECULAR DYNAMICS
- •A. Main Problems and Historical Perspective
- •B. Dynamics of Molecular Trees
- •C. Simulation of Flexible Rings
- •A. Time Step Limitations
- •B. Standard Geometry Versus Unconstrained Simulations
- •VI. CONCLUDING REMARKS
- •REFERENCES
- •Implicit Solvent Models
- •II. BASIC FORMULATION OF IMPLICIT SOLVENT
- •A. The Potential of Mean Force
- •III. DECOMPOSITION OF THE FREE ENERGY
- •A. Nonpolar Free Energy Contribution
- •B. Electrostatic Free Energy Contribution
- •IV. CLASSICAL CONTINUUM ELECTROSTATICS
- •A. The Poisson Equation for Macroscopic Media
- •B. Electrostatic Forces and Analytic Gradients
- •C. Treatment of Ionic Strength
- •A. Statistical Mechanical Integral Equations
- •VI. SUMMARY
- •REFERENCES
- •Steven Hayward
- •II. NORMAL MODE ANALYSIS IN CARTESIAN COORDINATE SPACE
- •B. Normal Mode Analysis in Dihedral Angle Space
- •C. Approximate Methods
- •IV. NORMAL MODE REFINEMENT
- •C. Validity of the Concept of a Normal Mode Important Subspace
- •A. The Solvent Effect
- •B. Anharmonicity and Normal Mode Analysis
- •VI. CONCLUSIONS
- •ACKNOWLEDGMENT
- •REFERENCES
- •Free Energy Calculations
- •Thomas Simonson
- •II. GENERAL BACKGROUND
- •A. Thermodynamic Cycles for Solvation and Binding
- •B. Thermodynamic Perturbation Theory
- •D. Other Thermodynamic Functions
- •E. Free Energy Component Analysis
- •III. STANDARD BINDING FREE ENERGIES
- •IV. CONFORMATIONAL FREE ENERGIES
- •A. Conformational Restraints or Umbrella Sampling
- •B. Weighted Histogram Analysis Method
- •C. Conformational Constraints
- •A. Dielectric Reaction Field Approaches
- •B. Lattice Summation Methods
- •VI. IMPROVING SAMPLING
- •A. Multisubstate Approaches
- •B. Umbrella Sampling
- •C. Moving Along
- •VII. PERSPECTIVES
- •REFERENCES
- •John E. Straub
- •B. Phenomenological Rate Equations
- •II. TRANSITION STATE THEORY
- •A. Building the TST Rate Constant
- •B. Some Details
- •C. Computing the TST Rate Constant
- •III. CORRECTIONS TO TRANSITION STATE THEORY
- •A. Computing Using the Reactive Flux Method
- •B. How Dynamic Recrossings Lower the Rate Constant
- •IV. FINDING GOOD REACTION COORDINATES
- •A. Variational Methods for Computing Reaction Paths
- •B. Choice of a Differential Cost Function
- •C. Diffusional Paths
- •VI. HOW TO CONSTRUCT A REACTION PATH
- •A. The Use of Constraints and Restraints
- •B. Variationally Optimizing the Cost Function
- •VII. FOCAL METHODS FOR REFINING TRANSITION STATES
- •VIII. HEURISTIC METHODS
- •IX. SUMMARY
- •ACKNOWLEDGMENT
- •REFERENCES
- •Paul D. Lyne
- •Owen A. Walsh
- •II. BACKGROUND
- •III. APPLICATIONS
- •A. Triosephosphate Isomerase
- •B. Bovine Protein Tyrosine Phosphate
- •C. Citrate Synthase
- •IV. CONCLUSIONS
- •ACKNOWLEDGMENT
- •REFERENCES
- •Jeremy C. Smith
- •III. SCATTERING BY CRYSTALS
- •IV. NEUTRON SCATTERING
- •A. Coherent Inelastic Neutron Scattering
- •B. Incoherent Neutron Scattering
- •REFERENCES
- •Michael Nilges
- •II. EXPERIMENTAL DATA
- •A. Deriving Conformational Restraints from NMR Data
- •B. Distance Restraints
- •C. The Hybrid Energy Approach
- •III. MINIMIZATION PROCEDURES
- •A. Metric Matrix Distance Geometry
- •B. Molecular Dynamics Simulated Annealing
- •C. Folding Random Structures by Simulated Annealing
- •IV. AUTOMATED INTERPRETATION OF NOE SPECTRA
- •B. Automated Assignment of Ambiguities in the NOE Data
- •C. Iterative Explicit NOE Assignment
- •D. Symmetrical Oligomers
- •VI. INFLUENCE OF INTERNAL DYNAMICS ON THE
- •EXPERIMENTAL DATA
- •VII. STRUCTURE QUALITY AND ENERGY PARAMETERS
- •VIII. RECENT APPLICATIONS
- •REFERENCES
- •II. STEPS IN COMPARATIVE MODELING
- •C. Model Building
- •D. Loop Modeling
- •E. Side Chain Modeling
- •III. AB INITIO PROTEIN STRUCTURE MODELING METHODS
- •IV. ERRORS IN COMPARATIVE MODELS
- •VI. APPLICATIONS OF COMPARATIVE MODELING
- •VII. COMPARATIVE MODELING IN STRUCTURAL GENOMICS
- •VIII. CONCLUSION
- •ACKNOWLEDGMENTS
- •REFERENCES
- •Roland L. Dunbrack, Jr.
- •II. BAYESIAN STATISTICS
- •A. Bayesian Probability Theory
- •B. Bayesian Parameter Estimation
- •C. Frequentist Probability Theory
- •D. Bayesian Methods Are Superior to Frequentist Methods
- •F. Simulation via Markov Chain Monte Carlo Methods
- •III. APPLICATIONS IN MOLECULAR BIOLOGY
- •B. Bayesian Sequence Alignment
- •IV. APPLICATIONS IN STRUCTURAL BIOLOGY
- •A. Secondary Structure and Surface Accessibility
- •ACKNOWLEDGMENTS
- •REFERENCES
- •Computer Aided Drug Design
- •Alexander Tropsha and Weifan Zheng
- •IV. SUMMARY AND CONCLUSIONS
- •REFERENCES
- •Oren M. Becker
- •II. SIMPLE MODELS
- •III. LATTICE MODELS
- •B. Mapping Atomistic Energy Landscapes
- •C. Mapping Atomistic Free Energy Landscapes
- •VI. SUMMARY
- •REFERENCES
- •Toshiko Ichiye
- •II. ELECTRON TRANSFER PROPERTIES
- •B. Potential Energy Parameters
- •IV. REDOX POTENTIALS
- •A. Calculation of the Energy Change of the Redox Site
- •B. Calculation of the Energy Changes of the Protein
- •B. Calculation of Differences in the Energy Change of the Protein
- •VI. ELECTRON TRANSFER RATES
- •A. Theory
- •B. Application
- •REFERENCES
- •Fumio Hirata and Hirofumi Sato
- •Shigeki Kato
- •A. Continuum Model
- •B. Simulations
- •C. Reference Interaction Site Model
- •A. Molecular Polarization in Neat Water*
- •B. Autoionization of Water*
- •C. Solvatochromism*
- •F. Tautomerization in Formamide*
- •IV. SUMMARY AND PROSPECTS
- •ACKNOWLEDGMENTS
- •REFERENCES
- •Nucleic Acid Simulations
- •Alexander D. MacKerell, Jr.
- •Lennart Nilsson
- •D. DNA Phase Transitions
- •III. METHODOLOGICAL CONSIDERATIONS
- •A. Atomistic Models
- •B. Alternative Models
- •IV. PRACTICAL CONSIDERATIONS
- •A. Starting Structures
- •C. Production MD Simulation
- •D. Convergence of MD Simulations
- •WEB SITES OF INTEREST
- •REFERENCES
- •Membrane Simulations
- •Douglas J. Tobias
- •II. MOLECULAR DYNAMICS SIMULATIONS OF MEMBRANES
- •B. Force Fields
- •C. Ensembles
- •D. Time Scales
- •III. LIPID BILAYER STRUCTURE
- •A. Overall Bilayer Structure
- •C. Solvation of the Lipid Polar Groups
- •IV. MOLECULAR DYNAMICS IN MEMBRANES
- •A. Overview of Dynamic Processes in Membranes
- •B. Qualitative Picture on the 100 ps Time Scale
- •C. Incoherent Neutron Scattering Measurements of Lipid Dynamics
- •F. Hydrocarbon Chain Dynamics
- •ACKNOWLEDGMENTS
- •REFERENCES
- •Appendix: Useful Internet Resources
- •B. Molecular Modeling and Simulation Packages
- •Index
Modeling in NMR Structure Determination |
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where more information on the data can be used to evaluate the restraint (e.g., by inspecting the peak shape).
B. Automated Assignment of Ambiguities in the NOE Data
Assigning ambiguous NOEs is one of the major bottlenecks in NMR solution structure determination, comparable to map fitting in X-ray crystallography. In principle, ambiguous NOEs need not be explicitly assigned if they are used as ADRs, because the assignment is done implicitly in the structure calculation. This is because the summed distance D is strongly weighted toward the shortest of the contributing distances. If ADRs are used in the refinement of an already reasonably well determined structure, this weighting is expected to, in most cases, favor the really dominating contribution to the ambiguous NOE. The implicit assignments, achieved through weighting with the distances in the structure, will be mostly correct, and the path to the final structure satisfying all data will be relatively smooth.
The case is very different when ADRs are used for calculating structures ab initio, starting from random structures. Obviously, most of the initial implicit assignments from the random structures are incorrect, and the path toward the final structure is much more difficult owing to additional local minima in the energy. During the calculation, the interproton distances, and with them the weighting on different assignment possibilities, need to change. However, convergence can be achieved by treating the amiguous NOEs appropriately in generalized simulated annealing protocols (see Fig. 5).
C. Iterative Explicit NOE Assignment
The main difficulties with a fully automated method lie in defining rules for explicit assignment based on an ensemble of structures with possibly incorrect features and providing mechanisms for correcting incorrect assignments. Two fully automated iterative assignment methods have been proposed, one based on ADRs (ARIA: ambiguous restraints for iterative assignment) [20,23] and the other on self-correcting distance geometry (NOAH [22]).
Methods to assign ambiguous NOEs follow a sequence of steps (see Fig. 6). Structures are calculated and NOEs are assigned in an iterative way. In the first iteration, the assignments have to be based on the frequencies alone. In the following iterations, the assignments of ambiguous NOEs are derived from the structures by comparing interproton distances corresponding to each assignment possibility. In the ‘‘traditional’’ approach, one possibility would be chosen by hand, and a peak would not be used if an unambiguous assignment were impossible. In contrast, the automated methods use ambiguous peaks during the structure calculation. The key difference between these methods is in how ambiguous peaks are converted into distance restraints. The program ARIA generates one ADR for each ambiguous peak, whereas the program NOAH creates an unambiguous restraint for each assignment possibility.
In general, the advantages of using an automated method may be comparable to those of SA refinement in X-ray crystallography [68], where many of the operations necessary to refine a structure can be done automatically and the remaining manual interventions are easier because the SA refinement usually results in a more easily interpreted electron density map. Automated methods are usually used in combination with manual assignment. However, fully automated assignment of the NOEs is possible (see Fig. 7) [69].
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Nilges |
Figure 6 Steps in automated assignment. (1) Select the Sconv lowest energy structures from iteration i 1 that are used to interpret the spectra. (2) For each peak, list all possible assignments compatible with the resonances within a frequency range. (3) Extract a distance for each assignment possibility from the ensemble of structures. (4) Use the distances to assign ambiguous NOEs. (5) Calibrate the peak volumes to obtain distance restraints. (6) Calculate structures based on the new restraints.
D. Symmetrical Oligomers
Symmetrical oligomers present a special difficulty for NMR spectroscopy, because all symmetry-related hydrogens will have equivalent magnetic environments and therefore will be degenerate in chemical shift. Only one monomer is ‘‘seen’’ in the spectra. In principle, every single NOE peak in the spectrum is therefore ambiguous. This ambiguity that arises from the symmetry can be treated with the same concept as ambiguities due to limited spectral resolution with ambiguous distance restraints. Structure determinations of symmetrical oligomers were reviewed in detail recently [70].
The same principal ideas are incorporated in the calculation protocols for symmetrical oligomers as with asymmetrical systems, i.e., the weight is reduced specifically for ADRs or all distance restraints. In addition, the symmetry of the system restricts conforma-
Modeling in NMR Structure Determination |
267 |
Figure 7 Example of a fully automated assignment. The structure ensemble of the seven lowest energy structures at each iteration is shown. These structures are used for the violation analysis and for a partial assignment of ambiguous NOEs. In the first iteration the structures are calculated with all restraints, where each restraint has all assignment possibilities. In each subsequent iteration, consistently violated restraints are removed, and assignment possibilities are selected with increasingly tight criteria such that at the end of the eight iterations most NOEs are unambiguously assigned.
tional space and is maintained during the calculation by additional restraints. An attractive potential between the monomers can be used in the beginning of the protocol to prevent them from drifting apart. The special difficulties with symmetrical oligomer calculations arise for two reasons: First, all NOEs are ambiguous a priori; second, the assignments of neighboring residues are strongly correlated. A minimization method such as simulated annealing that moves single atoms (or rigid parts of amino acids) may not be optimal for moving larger parts of the structure coherently if a whole set of NOEs needs to be implicitly reassigned. As a result, the structure calculation has a lower convergence rate than for asymmetrical systems. A combination of annealing calculations with other optimization approaches (e.g., a recent branch-and-bound algorithm [36]) may be a more efficient approach. However, the present approaches based on annealing alone have been successful in several cases for quite complex systems (up to a tetramer and a hexamer [70]).
V.TREATMENT OF SPIN DIFFUSION
Depending on experimental parameters, NOE intensities will be affected by spin diffusion (Fig. 8). Magnetization can be transferred between two protons via third protons such that the NOE between the two protons is increased and may be observed even when the distance between the two protons is above the usual experimental limit. This is a consequence of the d 6 distance dependence of the NOE. Depending on the conformation, it can be more efficient to move magnetization over intermediate protons than directly. The treatment of spin diffusion during structure refinement is reviewed in more detail in Refs. 31, and 71– 73.
From a given structure, the NOE effect can be calculated more realistically by complete relaxation matrix analysis. Instead of considering only the distance between two protons, the complete network of interactions is considered (Fig. 8). Approximately, the
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Figure 8 Effects of spin diffusion. The NOE between two protons (indicated by the solid line) may be altered by the presence of alternative pathways for the magnetization (dashed lines). The size of the NOE can be calculated for a structure from the experimental mixing time, τm, and the complete relaxation matrix, (Rij), which is a function of all interproton distances dij and functions describing the motion of the protons. γ is the gyromagnetic ratio of the proton, is the Planck constant, τ is the rotational correlation time, and ω is the Larmor frequency of the proton in the magnetic field. The expression for (Rij) is an approximation assuming an internally rigid molecule.
relaxation matrix (Rij) depends on all interproton distances and on parameters describing overall and local motion. The long mixing times often necessary in heteronuclear NOE experiments would make spin diffusion estimates especially valuable. To calculate heteronuclear NOEs realistically, the transfer efficiencies between protons and heteronuclei should be incorporated into the equations [74].
One approach to include spin diffusion corrections in a structure calculation is a direct refinement against NOE intensities, analogous to X-ray crystal structure refinement. In this approach, forces are calculated directly from the difference between the experimental NOE intensities and those calculated from the structure via the relaxation matrix. This necessitates, however, an expensive evaluation of derivatives of the simulated NOE spectra with respect to coordinates at every minimization step. Approximations and faster methods to evaluate the gradients [75] make this direct approach more feasible. Various pseudo-energy functions have been proposed. The simplest form (harmonic in the difference between experimental and calculated NOE) places a predominant weight on the largest intensities (shortest distances), which are most often due to intraresidue interactions and will therefore contribute little to determining the conformation of the molecule. By using pseudo-energy functions depending on the sixth root of the difference between calculated and experimental NOEs, the weight is distributed more equally.