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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
10 \section{\label{introSection:classicalMechanics}Classical
11 Mechanics}
12
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 \subsection{\label{introSection:newtonian}Newtonian Mechanics}
25
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}