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1   \chapter{\label{chapt:introduction}INTRODUCTION AND THEORETICAL BACKGROUND}
2  
3 \section{\label{introSection:molecularDynamics}Molecular Dynamics}
4
5 As a special discipline of molecular modeling, Molecular dynamics
6 has proven to be a powerful tool for studying the functions of
7 biological systems, providing structural, thermodynamic and
8 dynamical information.
9
3   \section{\label{introSection:classicalMechanics}Classical
4   Mechanics}
5  
# Line 22 | Line 15 | sufficient to predict the future behavior of the syste
15   sufficient to predict the future behavior of the system.
16  
17   \subsection{\label{introSection:newtonian}Newtonian Mechanics}
18 + The discovery of Newton's three laws of mechanics which govern the
19 + motion of particles is the foundation of the classical mechanics.
20 + Newton¡¯s first law defines a class of inertial frames. Inertial
21 + frames are reference frames where a particle not interacting with
22 + other bodies will move with constant speed in the same direction.
23 + With respect to inertial frames Newton¡¯s second law has the form
24 + \begin{equation}
25 + F = \frac {dp}{dt} = \frac {mv}{dt}
26 + \label{introEquation:newtonSecondLaw}
27 + \end{equation}
28 + A point mass interacting with other bodies moves with the
29 + acceleration along the direction of the force acting on it. Let
30 + $F_ij$ be the force that particle $i$ exerts on particle $j$, and
31 + $F_ji$ be the force that particle $j$ exerts on particle $i$.
32 + Newton¡¯s third law states that
33 + \begin{equation}
34 + F_ij = -F_ji
35 + \label{introEquation:newtonThirdLaw}
36 + \end{equation}
37  
38 + Conservation laws of Newtonian Mechanics play very important roles
39 + in solving mechanics problems. The linear momentum of a particle is
40 + conserved if it is free or it experiences no force. The second
41 + conservation theorem concerns the angular momentum of a particle.
42 + The angular momentum $L$ of a particle with respect to an origin
43 + from which $r$ is measured is defined to be
44 + \begin{equation}
45 + L \equiv r \times p \label{introEquation:angularMomentumDefinition}
46 + \end{equation}
47 + The torque $\tau$ with respect to the same origin is defined to be
48 + \begin{equation}
49 + N \equiv r \times F \label{introEquation:torqueDefinition}
50 + \end{equation}
51 + Differentiating Eq.~\ref{introEquation:angularMomentumDefinition},
52 + \[
53 + \dot L = \frac{d}{{dt}}(r \times p) = (\dot r \times p) + (r \times
54 + \dot p)
55 + \]
56 + since
57 + \[
58 + \dot r \times p = \dot r \times mv = m\dot r \times \dot r \equiv 0
59 + \]
60 + thus,
61 + \begin{equation}
62 + \dot L = r \times \dot p = N
63 + \end{equation}
64 + If there are no external torques acting on a body, the angular
65 + momentum of it is conserved. The last conservation theorem state
66 + that if all forces are conservative, Energy $E = T + V$ is
67 + conserved. All of these conserved quantities are important factors
68 + to determine the quality of numerical integration scheme for rigid
69 + body \cite{Dullweber1997}.
70 +
71   \subsection{\label{introSection:lagrangian}Lagrangian Mechanics}
72  
73   Newtonian Mechanics suffers from two important limitations: it
# Line 36 | Line 81 | system, alternative procedures may be developed.
81   which arise in attempts to apply Newton's equation to complex
82   system, alternative procedures may be developed.
83  
84 < \subsection{\label{introSection:halmiltonPrinciple}Hamilton's
84 > \subsubsection{\label{introSection:halmiltonPrinciple}Hamilton's
85   Principle}
86  
87   Hamilton introduced the dynamical principle upon which it is
# Line 46 | Line 91 | the kinetic, $K$, and potential energies, $U$.
91   The actual trajectory, along which a dynamical system may move from
92   one point to another within a specified time, is derived by finding
93   the path which minimizes the time integral of the difference between
94 < the kinetic, $K$, and potential energies, $U$.
94 > the kinetic, $K$, and potential energies, $U$ \cite{tolman79}.
95   \begin{equation}
96   \delta \int_{t_1 }^{t_2 } {(K - U)dt = 0} ,
97   \label{introEquation:halmitonianPrinciple1}
# Line 67 | Line 112 | then Eq.~\ref{introEquation:halmitonianPrinciple1} bec
112   \label{introEquation:halmitonianPrinciple2}
113   \end{equation}
114  
115 < \subsection{\label{introSection:equationOfMotionLagrangian}The
115 > \subsubsection{\label{introSection:equationOfMotionLagrangian}The
116   Equations of Motion in Lagrangian Mechanics}
117  
118   for a holonomic system of $f$ degrees of freedom, the equations of
# Line 142 | Line 187 | known as the canonical equations of motions.
187   Eq.~\ref{introEquation:motionHamiltonianCoordinate} and
188   Eq.~\ref{introEquation:motionHamiltonianMomentum} are Hamilton's
189   equation of motion. Due to their symmetrical formula, they are also
190 < known as the canonical equations of motions.
190 > known as the canonical equations of motions \cite{Goldstein01}.
191  
192   An important difference between Lagrangian approach and the
193   Hamiltonian approach is that the Lagrangian is considered to be a
# Line 153 | Line 198 | equations.
198   appropriate for application to statistical mechanics and quantum
199   mechanics, since it treats the coordinate and its time derivative as
200   independent variables and it only works with 1st-order differential
201 < equations.
201 > equations\cite{Marion90}.
202  
203 < \subsection{\label{introSection:poissonBrackets}Poisson Brackets}
203 > When studying Hamiltonian system, it is more convenient to use
204 > notation
205 > \begin{equation}
206 > r = r(q,p)^T
207 > \end{equation}
208 > and to introduce a $2n \times 2n$ canonical structure matrix $J$,
209 > \begin{equation}
210 > J = \left( {\begin{array}{*{20}c}
211 >   0 & I  \\
212 >   { - I} & 0  \\
213 > \end{array}} \right)
214 > \label{introEquation:canonicalMatrix}
215 > \end{equation}
216 > Thus, Hamiltonian system can be rewritten as,
217 > \begin{equation}
218 > \frac{d}{{dt}}r = J\nabla _r H(r)
219 > \label{introEquation:compactHamiltonian}
220 > \end{equation}
221 > where $I$ is an identity matrix and $J$ is a skew-symmetrix matrix
222 > ($ J^T  =  - J $).
223  
224 < \subsection{\label{introSection:canonicalTransformation}Canonical
224 > %\subsection{\label{introSection:canonicalTransformation}Canonical
225   Transformation}
226  
227 + \section{\label{introSection:geometricIntegratos}Geometric Integrators}
228 +
229 + \subsection{\label{introSection:symplecticMaps}Symplectic Maps and Methods}
230 +
231 + \subsection{\label{Construction of Symplectic Methods}}
232 +
233   \section{\label{introSection:statisticalMechanics}Statistical
234   Mechanics}
235  
236 < The thermodynamic behaviors and properties  of Molecular Dynamics
236 > The thermodynamic behaviors and properties of Molecular Dynamics
237   simulation are governed by the principle of Statistical Mechanics.
238   The following section will give a brief introduction to some of the
239   Statistical Mechanics concepts presented in this dissertation.
# Line 172 | Line 242 | Statistical Mechanics concepts presented in this disse
242  
243   \subsection{\label{introSection:ergodic}The Ergodic Hypothesis}
244  
245 +
246 + \section{\label{introSection:molecularDynamics}Molecular Dynamics}
247 +
248 + As a special discipline of molecular modeling, Molecular dynamics
249 + has proven to be a powerful tool for studying the functions of
250 + biological systems, providing structural, thermodynamic and
251 + dynamical information.
252 +
253 + \subsection{\label{introSec:mdInit}Initialization}
254 +
255 + \subsection{\label{introSection:mdIntegration} Integration of the Equations of Motion}
256 +
257   \section{\label{introSection:rigidBody}Dynamics of Rigid Bodies}
258  
259 + A rigid body is a body in which the distance between any two given
260 + points of a rigid body remains constant regardless of external
261 + forces exerted on it. A rigid body therefore conserves its shape
262 + during its motion.
263 +
264 + Applications of dynamics of rigid bodies.
265 +
266 +
267 + %\subsection{\label{introSection:poissonBrackets}Poisson Brackets}
268 +
269   \section{\label{introSection:correlationFunctions}Correlation Functions}
270  
271   \section{\label{introSection:langevinDynamics}Langevin Dynamics}

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