The Classical Mechanics Chinmoy Taraphdar Asian Books Private Limited
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The Classical
Mechanics
Chinmoy Taraphdar Lecturer, Dept. of Physics
Bankura Christian College
Bankura, West Bengal
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I st Published 2007
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Preface
This book, organised into ten chapters, is written to cover the syllabus of classical
mechanics for the students of physics at the graduate and postgraduate level. I
hope that the clear, lucid and comprehensive coverage of this book will help
students to gain a thorough grounding of the subject.
The beginning part of this book explains several chapters on the basis of
Newtonian mechanics and then the text explains the generalised co-ordinates
and Lagrangian mechanics along with Hamiltonian mechanics basically for the
holonomic system. The concluding chapter deals with the canonical
transformations by which the solution to the particular problem can be obtained
trivially. Some problems have been worked out to aid in understanding the
underlying theory at the end of each chapter.
Finally, the expressions of acknowledgements. I am indebted to my
colleagues, students who have kindly given me valuable comments and
suggestions. I acknowledge with a deep sense of gratitude my indebtedness to
the authors whose standard works in the field I have freely consulted to my
benefit. I also acknowledge my indebtedness to my wife 'Anamika', my daughter
'Sreetama' and my son 'Jyotirmoy' for their help at every stage of the preparation
of the manuscript. My special thanks are due to all concerned of 'Asian Books
Private Limited', especially to Ms. Purobi Biswas, Production Manager. Mr.
Subhadip Khan, the Branch Manager of Kolkata office for their kind help in
bringing out the volume in its admirable form and bearing with me at every
stage with unfailing patience and good humour.
It is fervently hoped that the book will be of value to the students and
teachers alike. Comments and suggestions for improvements to the text will be
thankfully acknowledged.
Chinmoy Taraphdar
Contents
Preface
Chapter 1. Vector
1.1. Fundamental Concept of Scalar and Vectors, 1
1.2. Unit Vectors and General representation of a vector, 1
1.3. Multiplication and Division of Vectors by Scalar, 2
1.4. Collinear Vectors, 3
1.5. Linear Dependence or Independence of Vectors, 3
1.6. Addition and Subtraction of two Vectors, 4
1.7. Addition of More Than Two Vectors, 5
1.8. Position Vector and Its Representation in Co-ordinate System, 5
1.9. Condition of Co-planarity of Vectors, 7
1.10. Rotational Invarience of Vector in Reference Frame, 8
1.11. Product of Two Vectors, 8
1.12. Scalar Tripple Product, 10
1.13. Vector Tripple Product, 11
1.14. Pseudo Vectors and Pseudo Scalars, 11
1.15. Vector Derivatives (Ordinary), 13
1.16. Vector Derivatives (Partial) and Vector Operators, 13
1.17. Laplacian and D'Alambertian Operator, 18
1.18. Vector Integration, 19
1.19. Gauss's Divergence Theorem, 20
1.20. Green's Theorem, 21
1.21. Stoke's Theorem, 22
1.23. Reciprocal Vectors, 24
1.23. Scalar and Vector Field, 24
1.25. Elementary Idea about Vector Space, 24
1.25. Linear Operator in Vector Space, 25
Summary, 26
Worked Out Examples, 29
Exercises, 34
Chapter 2. Linear Motion
2.1. Introduction, 37
2.2. Kinematics, 37
2.3. Basic Definitions of Required Parameters, 37
2.4. Velocity and Acceleration in Several Co-ordinate System, 40
2.5. Tangential and Normal Component of Velocity and Acceleration, 41
2.6. Radial and Transverse Component of Velocity and Acceleration, 42
2.7. Newton's Laws of Motion, 44
2.8. Accelerated Linear Motion, 45
(iii)
1-36
37-64
(vi)
2.9. Graphical Treatment of Linear Motion, 45
2.10. Conservation of Linear Motion, 46
2.11. Time Integral of Force (Impulse), 46
2.12. Work,47
2.13. Power, 48
2.14. Energy: Kinetic and Potential, 48
2.15. Conservative Force, 49
2.16. Conservation of Energy, 49
2.17. Center of Mass and Its Motion, 50
2.18. The Two Body Problem, 51
2.19. Application of the Principle of Linear Motion, 52
2.20. Mechanics of Variable Mass, 53
Summary, 55
Worked Out Examples, 58
Exercises, 64
Chapter 3. Rotational Motion: Rigid Body Rotation 65-94
3.1. Introduction, 65
3.2. Angular velocity and Angular Momentum, 65
3.3. Angular Acceleration, 66
3.4. Moment of Inertia and Torque, 67
3.5. Centrifugal force, 70
3.6. Rotational Kinetic Energy, 71
3.7. Angular Momentum for Rigid Body Rotation, 72
3.8. Kinetic Energy for Rigid Body Rotation, 74
3.9. Axes theorem for Moment of Inertia, 75
3.10. Calculation of Moment of Inertia in different cases, 76
3.11. Momental Ellipsoid or Ellipsoid of Inertia, 83
3.13. Moment and product of Inertia and Ellipsoid of inertia of some,
symmetrical bodies, 84
3.12. Moment of Inertia Tensor, 87
3.14. Routh's Rule, 87
3.15. Euler's Angles, 88
Summary,89
Worked Out Examples, 91
Exercises, 93
Chapter 4. Reference Frame 95-111
4.1. Introduction, 95
4.2. Non Inertial Frame and Pseudo Force, 95
4.3. Effect of rotation of earth on acceleration due to gravity, 99
4.4. Effect of Coriolis Force on a particle moving on the surface of earth, 101
4.5. Effect of Coriolis force on a particle falling freely under gravity, 103
4.6. Principle of Foucault's Pendulum, 104
4.7. Flow of River on Earth Surface, 106
Summary, 106
Worked out Examples, 107
Exercises, 110
(vii)
Chapter 5. Central Force 112-124
5.1. Introduction, 112
5.2. Definition and Characteristics of Central force, 112
5.3. Conservation of Angular Momentum under Central Force, 113
5.4. Conservation of energy under central force, 113
5.5. Equation of motion under attractive central force, 115
5.6. Application of central force theory to gravitation Deduction of
Keplar's law, 116
5.7. Energy conservation for planetory motion, 118
5.8. Stability of Orbits, 120
Summary, 120
Worked out Examples, 121
Exercises, 124
Chapter 6. Theory of Collision 125-137
6.1. Introduction, 125
6.2. Characteristics of Collision, 125
6.3. Lab Frame and Center of Mass Frame, 126
6.4. Direct or Linear Collision, 127
6.5. Characteristic of Direct Collision, 129
6.6. Maximum Energy transfer due to head on elastic collision, 130
6.7. Oblique Collision, 131
Summary, 132
Worked Out Examples, 133
Exercises, 137
Chapter 7. Conservation Principle and Constrained Motion 138-154
7.1. Characteristics of Conservation Principle, 138
7.2. Mechanics of a single particle and system of particles, 139
7.3. Conservation of linear momentum, 140
7.4. Conservation of Angular Momentum, 141
7.5. Conservation of Energy, 142
7.6. Constrained Motion, 145
7.7. Generalised Co-ordinates and other Generalised Parameters, 146
7.8. Limitation of Newton's Law, 151
Summary, 151
Worked out examples, 153
Exercises, 154
Chapter 8. Variational Principle and Lagrangian Mechanics 155-193
8.1. Introduction, 155
8.2. Forces of Constraint, 155
8.3. Virtual Displacement, 156
8.4. Principle of Virtual Work, 156
8.5. D' Alembert's Principle, 157
8.6. Lagrange's equations for a holonomic System, 158
8.7. Lagrange's equation for a conservative, non-holonomic system, 160
8.8. Introduction to Calculus of variations, 161
8.9. Variational Technique for many independent variables:
Euler-Lagrange's differential equation, 165
( viii)
8.10. Hamilton's Variational Principle, 166
8.11. Derivation of Hamilton's principle from Lagrange's equation, 167
8.12. Derivation of Lagrange's equations from Hamilton's principle, 168
8.13. Derivation of Lagrange's equation from D' Alambert's principle, 169
8.14. Derivation of Hamilton's Principle from D' Alambert's Principle, 171
8.15. Cyclic or Ignorable Co-ordinates, 172
8.16. Conservation Theorems, 172
8.17. Gauge Function for Lagrangian, 175
8.18. Invarience of Lagrange's equations under Generalised
Co-ordinate, transformations, 177
8.19. Concept of Symmetry: Homogeneity and Isotropy, 178
8.20. Invarience of Lagrange's equation under Galilean Transformation, 179
8.21. Application's of Lagrange's equation of motion in several mechanical
systems, 180
Summary, 186
Worked Out Examples, 187
Exercises, 193
Chapter 9. Hamiltonian Formulation in Mechanics 194-209 9.1. Introduction, 194
9.2. Hamiltonian of the System, 194
9.3. Concept of Phase Space, 195
9.5. Hamilton's Canonical Equations in different Co-ordinate System, 197
9.6. Hamilton's Canonical equations from Hamilton's Intergral Principle, 199
9.7. Physical Significance of Hamiltonian of the System, 201
9.8. Advantage of Hamiltonian Approach, 201
9.9. Principle of Least Action, 201
9.10. Difference between Hamilton's Principle and the principle of least,
action, 203
9.11. Application of Hamilton's Canonical Equations, 203
Summary, 206
Worked Out Examples, 206
Exercises, 209
Chapter 10. Canonical Transformations 210-232
10.1. Introduction to Canonical Transformations, 210
10.2. Hamilton-Jocobi Method, 215
10.3. Application of Hamilton-Jacobi method to the particle falling freely, 217
10.4. Han,iIton's Characteristics function, 219
10.5. Action and Angle Variables, 220
10.6. Application of Action Angle Variables to Harmonic Oscillator Problem, 221
10.7. Poisson's Bracket, 222
10.8. Poisson's Theorem, 223
10.9. Jacobi's Identity, 224
10.10. Lagrange's Brackets, 225
10.11. Liouville's Theorem, 226
Summary, 227
Worked Out Examples, 229
Exercises. 231
Chapter-I
Vector
1.1. Fundamental Concept of Scalar and Vectors:
Any physical quantity· having both direction and magnitude is called vector
quantity and these quantity must obey some fundamental laws of addition and
subtraction.
But the quantity having only magnitude, but no direction is called scalar
quantity. Basically, the magnitude or measure of a scalar quantity is quite
independent of any co-ordinate system, but the measure of vector quantity
depends on the frame choosen.
All scalar quantities are, however, subject to the ordinary algebraical laws
of addition and multiplication:
viz. (i) a + b = b + a
a x b = b x a (Commutative law)
(ii) (a + b) + c = a + (b + c)
(a x b) x c = a x (b xc) (Associative law)
(iii) a x (b + c) = a x b + a x c
(a + b) x c = a Xc + b x c (Distributive law)
On the other hand vectors are subject to the triangular or parallelogram law
of addition (or subtraction).
1.2. Unit Vectors and General representation of a
vector:
A vector is analytically represented by a letter
with an arrow over it, i.e, A and its magnitude is
p
o * Basically, Physical quantities are Tensor. Any tensor is that quantity which may
change under co-ordinate transformatIOn. The tensor of rank 'n' is that quantity
which transforms through 'n' no. of cu-efficient matrices. Actually a vector is a
tensor of rank 1 where as a scalar is a tensor of rank O.