- •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
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It has been shown that similar conformations that belong to adjacent energy basins separated by high energy barriers are incorrectly grouped together by the straightforward cluster analysis [29].
C. Principal Component Analysis
An inherent problem associated with conformational analysis is the high dimensionality of the molecular conformational spaces. An N-atom molecule has 3N degrees of freedom, and its corresponding conformational space is (3N 6)-dimensional. As a result, even relatively small molecules have very large conformational spaces, making them difficult to analyze. For example, a small heptapeptide may have a 100-dimensional or even 150dimensional conformational space, depending on its precise amino acid composition. Principal component analysis (PCA) is a computational tool that reduces the effective dimensionality of molecular conformational spaces while retaining an accurate representation of the interconformational distances. This task is accomplished by projecting the original multidimensional data onto an optimal low-dimensional subspace, allowing visual inspection of conformational spaces and of dynamic trajectories that traverse these spaces. Principal component analysis (PCA) was introduced to protein simulations under the name quasi-harmonic analysis by Ichiye and Karplus [31] and is becoming widely used for a variety of applications involving sampling and visualization of conformational spaces [32– 35]. A review of principal component analysis can be found in Ref. 36.
How does principal component analysis work? Consider, for example, the two-di- mensional distribution of points shown in Figure 7a. This distribution clearly has a strong linear component and is closer to a one-dimensional distribution than to a full two-dimen- sional distribution. However, from the one-dimensional projections of this distribution on the two orthogonal axes X and Y you would not know that. In fact, you would probably conclude, based only on these projections, that the data points are homogeneously distributed in two dimensions. A simple axes rotation is all it takes to reveal that the data points
Figure 7 (a) A two-dimensional distribution of points and their one-dimensional projections on the original axes. Judging just from the 1D projections one would probably conclude that the original distribution is homogeneously distributed in two dimensions. (b) The same distribution of points and their 1D projections on the new axes set obtained by PCA by using a similarity transformation. The new 1D projections highlight the strong 1D character of the distribution.
Conformational Analysis |
87 |
are preferentially spread along one dimension, as reflected by the broad distribution along one of the new axes and a narrow distribution along the other in Figure 7b. The above procedure is what is done by PCA. Starting from a multidimensional distribution of data points (in our case, of molecular conformations), PCA performs a similarity transformation on the original axes to find a new set of axes that best fits the data. The first new axis is selected such that the variance of the distribution along it is the largest possible. The second axis is placed orthogonal to the first in the direction of the second largest variance of the distribution, and so forth. In this new axes set it is usually possible to identify a low-dimensional subspace that captures most of the relative distances between individual conformations.
In general, two related techniques may be used: principal component analysis (PCA) and principal coordinate analysis (PCoorA). Both methods start from the n m data matrix M, which holds the m coordinates defining n conformations in an m-dimensional space. That is, each matrix element Mij is equal to qij, the jth coordinate of the ith conformation. From this starting point PCA and PCoorA follow different routes.
Principal component analysis (PCA) takes the m-coordinate vectors q associated with the conformation sample and calculates the square m m MTM matrix, reflecting the relationships between the coordinates. This matrix, also known as the covariance matrix C,
is defined as |
|
C (q q)(q q)T |
(14) |
where the averaging is over the conformation sample (in Cartesian space m 3N for an N-atom molecule). The covariance matrix C is diagonalized to obtain the eigenvectors that capture most of the variation in atomic position fluctuations.
Principal coordinate analysis (PCoorA) [37], on the other hand, operates on the square n n MMT matrix, reflecting the relationships between the conformations. The elements of this matrix, also known as the distance matrix , are distances dij between two conformations i and j [such as those defined in Eqs. (12) and (13)]. Since the distances dij can also be obtained from the n n matrix A of latent roots (eigenvectors), one can use this matrix for the projection, defining Aij 1/2d2ij and Aii 0 (for i, j 1, 2, . . . , n). To guarantee that the matrix A has a zero root (and thus guarantee that it corresponds to a real configuration) it is ‘‘centered,’’ so that the sum of every row and the sum of every column of A is zero. This centering, which does not alter the distances dij, is defined as
Aij* Aij Aij i Aij j 2Aij ij |
(15) |
where k is the mean over all specific indices k i, j, ij. The centered matrix A* is diagonalized using standard matrix algebra to obtain the latent eigenvectors and the diagonal matrix of eigenvalues. The resulting eigenvalues (normalized) give the percentage of the projection of the original distribution on the new coordinate set, and the eigenvectors (scaled by their corresponding eigenvalues) give the new coordinates of the original points in the new axes set. For a more detailed description of this method, see Refs. 29 and 37.
It should be stressed that PCA and PCoorA are dual methods that give the same analytical results. Using one or the other is simply a matter of convenience, whether one prefers to work with the covariance matrix C or with the distance matrix ∆.
As stated earlier, the main motivation for using either PCA or PCA is to construct a low-dimensional representation of the original high-dimensional data. The notion behind this approach is that the effective (or essential, as some call it [33]) dimensionality of a molecular conformational space is significantly smaller than its full dimensionality (3N- 6 degrees of freedom for an N-atom molecule). Following the PCA procedure, each new
88 |
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Figure 8 A joint principal coordinate projection of the occupied regions in the conformational spaces of linear (Ala)6 (triangles) and its conformational constraint counterpart, cyclic-(Ala)6 (squares), onto the optimal 3D principal axes. The symbols indicate the projected conformations, and the ellipsoids engulf the volume occupied by the projected points. This projection shows that the conformational volume accessible to the cyclic analog is only a small subset of the conformational volume accessible to the linear peptide, (Adapted from Ref. 41.)
axis k is associated with a normalized eigenvalue λk that reflects the relative weight of that axis in reproducing the original data. An axis with a high λk value is significant for the projection, whereas axes with small λk values are insignificant. By sorting the new axes according to their λk weight it is possible to select a small subset of effective coordinates that capture most of the conformational relationships of the original high-dimen- sional space. The quality of such a projection can be estimated by the average difference between conformation distances reconstructed in the low s-dimensional subspace d(ijs) and the original distance dij. The reconstructed distances are defined as
s |
|
dij(s)2 (Qik Qjk)2 |
(16) |
k 1
where Qik is the coordinate of the ith conformation along the kth new (principal) axis. It can be shown that the average deviation of the distances in s dimensions from the exact distances is given by the sum of the first s eigenvalues,
s |
|
dij2 dij(s)2 ij 1 λk |
(17) |
k 1
Thus by summing the normalized eigenvalues of the first s dimensions one can judge the quality of a projection onto that subspace.
Fortunately, it was found that in polypeptide systems the effective dimensionality of conformational spaces is significantly smaller than the dimensionality of the full space, with only a few principal axes contributing to the projection [38–41]. In fact, in many cases a projection quality of 70–90% can be achieved in as few as three dimensions [42], opening the way for real 3D visualization of molecular conformational space. Figure 8
Conformational Analysis |
89 |
shows a 3D visualization of the conformational spaces of two hexapeptides, (Ala)6 and cyclic-(Ala)6, jointly projected on the same principal coordinate set. The comparison shows that the conformation volume occupied by the linear peptide is about 10 times larger than the conformation volume occupied by its conformationally constrained counterpart. Quantifying relative flexibility of analogous peptides through joint principal projections was shown to be useful, for example, in predicting their relative bioactivity [41].
V.CONCLUSION
In this chapter we surveyed a variety of computational methods that contribute to the ‘‘conformational analysis’’ of complex molecules. These include methods for searching and sampling the molecular conformation space, methods for local optimization of the sampled conformations, and basic analytical techniques. In practice, many variations of the basic methodologies are reported as researchers continuously try to improve and enhance these procedures. The different methods are often used in conjunction to form a complete conformational analysis study of a bimolecular system of interest. However, each of the different procedures can also be used separately as part of computational studies with other goals. The need for these analytical techniques is to a large extent brought about by the continuous increase is simulation times, which generates more data than ever before, requiring systematic ways to interpret and represent them.
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