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1   \chapter{\label{chapt:introduction}INTRODUCTION AND THEORETICAL BACKGROUND}
2  
3 < \section{\label{introSection:classicalMechanics}Classical Mechanics}
3 > \section{\label{introSection:molecularDynamics}Molecular Dynamics}
4  
5 < \section{\label{introSection:rigidBody}Dynamics of Rigid Bodies}
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  
10 < \section{\label{introSection:statisticalMechanics}Statistical Mechanics}
10 > \section{\label{introSection:classicalMechanics}Classical
11 > Mechanics}
12  
13 < \section{\label{introSection:molecularDynamics}Molecular Dynamics}
13 > Closely related to Classical Mechanics, Molecular Dynamics
14 > simulations are carried out by integrating the equations of motion
15 > for a given system of particles. There are three fundamental ideas
16 > behind classical mechanics. Firstly, One can determine the state of
17 > a mechanical system at any time of interest; Secondly, all the
18 > mechanical properties of the system at that time can be determined
19 > by combining the knowledge of the properties of the system with the
20 > specification of this state; Finally, the specification of the state
21 > when further combine with the laws of mechanics will also be
22 > sufficient to predict the future behavior of the system.
23  
24 < \section{\label{introSection:langevinDynamics}Langevin Dynamics}
24 > \subsection{\label{introSection:newtonian}Newtonian Mechanics}
25  
26 < \section{\label{introSection:hydroynamics}Hydrodynamics}
26 > \subsection{\label{introSection:lagrangian}Lagrangian Mechanics}
27  
28 + Newtonian Mechanics suffers from two important limitations: it
29 + describes their motion in special cartesian coordinate systems.
30 + Another limitation of Newtonian mechanics becomes obvious when we
31 + try to describe systems with large numbers of particles. It becomes
32 + very difficult to predict the properties of the system by carrying
33 + out calculations involving the each individual interaction between
34 + all the particles, even if we know all of the details of the
35 + interaction. In order to overcome some of the practical difficulties
36 + which arise in attempts to apply Newton's equation to complex
37 + system, alternative procedures may be developed.
38 +
39 + \subsection{\label{introSection:halmiltonPrinciple}Hamilton's
40 + Principle}
41 +
42 + Hamilton introduced the dynamical principle upon which it is
43 + possible to base all of mechanics and, indeed, most of classical
44 + physics. Hamilton's Principle may be stated as follow,
45 +
46 + The actual trajectory, along which a dynamical system may move from
47 + one point to another within a specified time, is derived by finding
48 + the path which minimizes the time integral of the difference between
49 + the kinetic, $K$, and potential energies, $U$.
50 + \begin{equation}
51 + \delta \int_{t_1 }^{t_2 } {(K - U)dt = 0} ,
52 + \label{introEquation:halmitonianPrinciple1}
53 + \end{equation}
54 +
55 + For simple mechanical systems, where the forces acting on the
56 + different part are derivable from a potential and the velocities are
57 + small compared with that of light, the Lagrangian function $L$ can
58 + be define as the difference between the kinetic energy of the system
59 + and its potential energy,
60 + \begin{equation}
61 + L \equiv K - U = L(q_i ,\dot q_i ) ,
62 + \label{introEquation:lagrangianDef}
63 + \end{equation}
64 + then Eq.~\ref{introEquation:halmitonianPrinciple1} becomes
65 + \begin{equation}
66 + \delta \int_{t_1 }^{t_2 } {L dt = 0} ,
67 + \label{introEquation:halmitonianPrinciple2}
68 + \end{equation}
69 +
70 + \subsection{\label{introSection:equationOfMotionLagrangian}The
71 + Equations of Motion in Lagrangian Mechanics}
72 +
73 + for a holonomic system of $f$ degrees of freedom, the equations of
74 + motion in the Lagrangian form is
75 + \begin{equation}
76 + \frac{d}{{dt}}\frac{{\partial L}}{{\partial \dot q_i }} -
77 + \frac{{\partial L}}{{\partial q_i }} = 0,{\rm{ }}i = 1, \ldots,f
78 + \label{introEquation:eqMotionLagrangian}
79 + \end{equation}
80 + where $q_{i}$ is generalized coordinate and $\dot{q_{i}}$ is
81 + generalized velocity.
82 +
83 + \subsection{\label{introSection:hamiltonian}Hamiltonian Mechanics}
84 +
85 + Arising from Lagrangian Mechanics, Hamiltonian Mechanics was
86 + introduced by William Rowan Hamilton in 1833 as a re-formulation of
87 + classical mechanics. If the potential energy of a system is
88 + independent of generalized velocities, the generalized momenta can
89 + be defined as
90 + \begin{equation}
91 + p_i = \frac{\partial L}{\partial \dot q_i}
92 + \label{introEquation:generalizedMomenta}
93 + \end{equation}
94 + The Lagrange equations of motion are then expressed by
95 + \begin{equation}
96 + p_i  = \frac{{\partial L}}{{\partial q_i }}
97 + \label{introEquation:generalizedMomentaDot}
98 + \end{equation}
99 +
100 + With the help of the generalized momenta, we may now define a new
101 + quantity $H$ by the equation
102 + \begin{equation}
103 + H = \sum\limits_k {p_k \dot q_k }  - L ,
104 + \label{introEquation:hamiltonianDefByLagrangian}
105 + \end{equation}
106 + where $ \dot q_1  \ldots \dot q_f $ are generalized velocities and
107 + $L$ is the Lagrangian function for the system.
108 +
109 + Differentiating Eq.~\ref{introEquation:hamiltonianDefByLagrangian},
110 + one can obtain
111 + \begin{equation}
112 + dH = \sum\limits_k {\left( {p_k d\dot q_k  + \dot q_k dp_k  -
113 + \frac{{\partial L}}{{\partial q_k }}dq_k  - \frac{{\partial
114 + L}}{{\partial \dot q_k }}d\dot q_k } \right)}  - \frac{{\partial
115 + L}}{{\partial t}}dt \label{introEquation:diffHamiltonian1}
116 + \end{equation}
117 + Making use of  Eq.~\ref{introEquation:generalizedMomenta}, the
118 + second and fourth terms in the parentheses cancel. Therefore,
119 + Eq.~\ref{introEquation:diffHamiltonian1} can be rewritten as
120 + \begin{equation}
121 + dH = \sum\limits_k {\left( {\dot q_k dp_k  - \dot p_k dq_k }
122 + \right)}  - \frac{{\partial L}}{{\partial t}}dt
123 + \label{introEquation:diffHamiltonian2}
124 + \end{equation}
125 + By identifying the coefficients of $dq_k$, $dp_k$ and dt, we can
126 + find
127 + \begin{equation}
128 + \frac{{\partial H}}{{\partial p_k }} = q_k
129 + \label{introEquation:motionHamiltonianCoordinate}
130 + \end{equation}
131 + \begin{equation}
132 + \frac{{\partial H}}{{\partial q_k }} =  - p_k
133 + \label{introEquation:motionHamiltonianMomentum}
134 + \end{equation}
135 + and
136 + \begin{equation}
137 + \frac{{\partial H}}{{\partial t}} =  - \frac{{\partial L}}{{\partial
138 + t}}
139 + \label{introEquation:motionHamiltonianTime}
140 + \end{equation}
141 +
142 + Eq.~\ref{introEquation:motionHamiltonianCoordinate} and
143 + Eq.~\ref{introEquation:motionHamiltonianMomentum} are Hamilton's
144 + equation of motion. Due to their symmetrical formula, they are also
145 + known as the canonical equations of motions.
146 +
147 + An important difference between Lagrangian approach and the
148 + Hamiltonian approach is that the Lagrangian is considered to be a
149 + function of the generalized velocities $\dot q_i$ and the
150 + generalized coordinates $q_i$, while the Hamiltonian is considered
151 + to be a function of the generalized momenta $p_i$ and the conjugate
152 + generalized coordinate $q_i$. Hamiltonian Mechanics is more
153 + appropriate for application to statistical mechanics and quantum
154 + mechanics, since it treats the coordinate and its time derivative as
155 + independent variables and it only works with 1st-order differential
156 + equations.
157 +
158 + \subsection{\label{introSection:poissonBrackets}Poisson Brackets}
159 +
160 + \subsection{\label{introSection:canonicalTransformation}Canonical
161 + Transformation}
162 +
163 + \section{\label{introSection:statisticalMechanics}Statistical
164 + Mechanics}
165 +
166 + The thermodynamic behaviors and properties  of Molecular Dynamics
167 + simulation are governed by the principle of Statistical Mechanics.
168 + The following section will give a brief introduction to some of the
169 + Statistical Mechanics concepts presented in this dissertation.
170 +
171 + \subsection{\label{introSection::ensemble}Ensemble}
172 +
173 + \subsection{\label{introSection:ergodic}The Ergodic Hypothesis}
174 +
175 + \section{\label{introSection:rigidBody}Dynamics of Rigid Bodies}
176 +
177   \section{\label{introSection:correlationFunctions}Correlation Functions}
178 +
179 + \section{\label{introSection:langevinDynamics}Langevin Dynamics}
180 +
181 + \subsection{\label{introSection:generalizedLangevinDynamics}Generalized Langevin Dynamics}
182 +
183 + \subsection{\label{introSection:hydroynamics}Hydrodynamics}

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