Mechanics - Osgood

Mechanics - Title page of a book

MECHANICS

BY WILLIAM FOGG OSGOOD,

NEW YORK, THE MACMILLAN COMPANY, 1949
    

DOWNLOAD FREE BOOK:   Mechanics
    

PREFACE

Mechanics is a natural science, and like any natural science requires for its comprehension the observation and knowledge of a vast fund of individual cases. Arid so the solution of problems is of prime importance throughout all the study of this subject.

But Mechanics is not an empirical subject in the sense in which physics and chemistry, when dealing with the border region of the human knowledge of the day are empirical. The latter take cognizance of a great number of isolated facts, which it is not as yet possible to arrange under a few laws, or postulates. The laws of Mechanics, like the laws of Geometry, so far as first approximations go the laws that explain the motion of the golf ball or the gyroscope or the skidding automobile, and which make possible the calculation of lunar tables and the prediction of eclipses these laws are known, and will be as new arid important two thousand years hence, as in the recent past of science when first they emerged into the light of day.

Here, then, is the problem of training the student in Mechanics to provide him with a vast fund of case material and to develop in him the habits of thought which refer a new problem back to the few fundamental laws of the subject. The physicist is keenly alive to the first requirement and tries to meet it both by simple laboratory experiments and by problems in the part of a general course on physics which is especially devoted to "Mechanics." The interest of the mathematician too often begins with virtual velocities and d'Alembert's Principle, and the variational principles, of which Hamilton's Principle is the most important. Both arc right, in the sense that they are doing nothing that is wrong; but each takes such a fragmentary view of the whole subject, that his work is ineffectual.

The world in which the boy and girl have lived is the true laboratory of elementary mechanics. The tennis ball, the golf ball, the shell on the river; the automobile good old Model T, in its day, and the home-made autos and motor boats which youngsters construct and will continue to construct the amateur printing press; the games in which the mechanics of the body is a part; all these things go to provide the student with rich laboratory experience before he begins a systematic study of mechanics. It is this experience on which the teacher of Mechanics can draw, and draw, and draw again.

The Cambridge Tripos of fifty years and more ago has been discredited in recent years, and the criticism was not without foundation. It was a method which turned out problem solvers so said its opponents. But it turned out a Clerk Maxwell and it vitally influenced the training of the whole group of English physicists, whose work became so illustrious. In his interesting autobiography, From Emigrant to Inventor, Pupin acknowledges in no uncertain terms the debt he owes to just this training, and to Arthur Gordon Webster, through whom he first came to know this method a method which Benjamin Osgood Peirce also prized highly in his work as a physicist. And so we make no apologies for availing ourselves to the fullest extent of that which the old Tripos Papers contributed to training in Mechanics. But we do not stop there. After all, it is the laws of Mechanics, their comprehension, their passing over into the flesh and blood of our scientific thought, and the mathematical technique and theory, that is our ultimate goal. To attain to this goal the mathematical theory, absurdly simple as it is at the start, must be systematically inculcated into the student from the beginning. In this respect the physicists fail us. Because the mathematics is simple, they do not think it important to insist on it. Any way to get an answer is good enough for them. But a day of reckoning comes. The physicist of to-day is in desperate need of mathematics, and at best all he can do is to grope, trying one mathematical expedient after another and holding to no one of these long enough to test it mathematically. Nor is he to be blamed. It is the old (and most useful) method of trial and error he is employing, and must continue to employ for the present.

Is the writer on Mechanics, per contra, to accept the challenge of preparing the physicist to solve these problems? That is too large a task. Rather, it is the wisdom of Pasteur who said: "Fortune favors the prepared mind" that may well be a guide for us now and in the future. What can be done, and what we have attempted in the present work, is to unite a broad and deep known edge of the most elementary physical phenomena in the field of Mechanics with the best mathematical methods of the present day, treating with completeness, clarity, and rigor the beginnings of the subject; in scope not restricted, in detail not involved, in spirit scientific.

The book is adapted to the needs of a first course in Mechanics, given for sophomores, and culminating in a thorough study of the dynamics of a rigid body in two dimensions. This course may be followed by a half-course or a full course which begins with the kinematics and kinetics of a rigid body in three dimensions and proceeds to Lagrange's Equations and the variational principles. So important are Hamilton's Equations and their solution by means of Jacobi's Equation, that this subject has also been included. It appears that there is a special need for treating this theory, for although it is exceedingly simple, the current text- books are unsatisfactory. They assume an undefined knowledge of the theory of partial differential equations of the first order, but they do not show how the theory is applied. As a matter of fact, no theory of these equations at all is required for understanding the solution just mentioned. What is needed is the fact that Hamilton's Equations are invariant of a contact transformation. A simple proof is given in Chapter XIV, in which the method most important for the physicist, namely, the method of separating the variables, is set forth with no involved preliminaries. But even this proof may be omitted or postponed, and the student may strike in at once with Chapter XV.

The concept of the vector is essential throughout Mechanics, but intricate vector analysis is wholly unnecessary. A certain minute amount of the latter is however helpful, and has been set forth in Appendix A.

Appendix D contains a definitive formulation of a class of problems which is most important in physics, and shows how d'Alembert's Principle and Lagrange's Equations apply. It ties together the various detailed studies of the text and gives the reader a comprehensive view of the subject as a whole.

The book is designed as a careful and thorough introduction to Mechanics, but not of course, in this brief compass, as a treatise. With the principles of Mechanics once firmly established and clearly illustrated by numerous examples the student is well equipped for further study in the current text-books, of which may be mentioned: Routh: An Elementary Treatise on Rigid Dynamics and also Advanced Dynamics, by the same author; particularly valuable for its many problems. Webster, Dynamics good material, and excellent for the student who is well trained in the rudiments, but hard reading for the beginner through poor presentation and lacunae in the theory; Appell, Mecanique rationelle, vols. i and ii a charming book, which the student may open at any chapter for supplementary reading and examples. Jeans, Mechanics, may also be mentioned for supplementary exercises; as a text it is unnecessarily hard mathematically for the Sophomore, and it does not go far enough physically for the upper classman. It is unnecessary to emphasize the importance of further study by the problem method of more advanced and difficult exercises, such as are found in these books. But to go further in incorporating these problems into the present work would increase its size unduly.

It is not merely a formal tribute, but one of deep appreciation, which I wish to pay to The Macmillan Company and to The Norwood Press for their hearty cooperation in all the many difficult details of the typography. Good composition is a distinct aid in setting forth the thought which the formulas are designed to express. Its beauty is its own reward.

To his teacher, Benjamin Osgood Peirce, who first blazed the trail in his course, Mathematics 4, given at Harvard in the middle of the eighties the Author wishes to acknowledge his profound gratitude. Out of these beginnings the book has grown, developed through the Author's courses at Harvard, extending over more than forty years, and out of courses given later at The National University of Peking. May it prove a help to the beginner in his first approach to the subject of Mechanics.

 
CONTENTS

CHAPTER I - STATICS OF A PARTICLE
1. Parallelogram of Forces
2. Analytic Treatment by Trigonometry
3. Equilibrium. The Triangle of Forces. Addition of Vectors
4. The Polygon of Forces
5. Friction
6. Solution of a Trigonometric Equation. Problem
Exercises on Chapter I

CHAPTER II - STATICS OF A RIGID BODY
1. Parallel Forces in a Plane
2. Analytic Formulation; n Forces
3. Centre of Gravity
4. Moment of a Force
5. Couples in a Plane
6. Resultant of Forces in a Plane. Equilibrium
7. Couples in Space
8. Resultant of Forces in Space. Equilibrium
9. Moment of a Vector. Couples
10. Vector Representation of Resultant Force and Couple. Resultant Axis. Wrench
11. Moment of a Vector about a Line
12. Equilibrium
13. Centre of Gravity of n Particles
14. Three Forces
Exercises on Chapter II

CHAPTER III - MOTION OF A PARTICLE
1. Rectilinear Motion
2. Newton's Laws of Motion
3. Absolute Units of Force
4. Elastic Strings
5. A Problem of Motion
6. Continuation; the Time
7. Simple Harmonic Motion
8. Motion under the Attraction of Gravitation
9. Work Done by a Variable Force
10. Kinetic Energy and Work
11. Change of Units in Physics
12. The Check of Dimensions
13. Motion in a Resisting Medium
14. Graph of the Resistance
15. Motion in a Plane and in Space
16. Vector Acceleration
17. Newton's Second Law
18. Motion of a Projectile
19. Constrained Motion
20. Simple Pendulum Motion
21. Motion on a Smooth Curve
22. Centrifugal Force
23. The Centrifugal Oil Cup
24. The Centrifugal Field of Force
25. Central Force
26. The Two Body Problem
27. The Inverse Problem to Determine the Force
28. Kepler's Laws
29. On the Notion of Mass

CHAPTER IV - DYNAMICS OF A RIGID BODY
1. Motion of the Centre of Gravity
2. Applications
3. The Equation of Moments
4. Rotation about a Fixed Axis under Gravity
5. The Compound Pendulum
6. Continuation. Discussion of the Point of Support
7. Kater's Pendulum
8. Atwood's Machine
9. The General Case of Rotation about a Point
10. Moments of Inertia
11. The Torsion Pendulum
12. Rotation of a Plane Lamina, No Point Fixed
13. Examples
14. Billiard Ball, Struck Full
15. Continuation. The Subsequent Motion
16. Further Examples
Exercises on Chapter IV

CHAPTER V - KINEMATICS IN TWO DIMENSIONS
1. The Rolling Wheel
2. The Instantaneous Centre
3. Rotation about the Instantaneous Centre
4. The Centrodes
5. Continuation. Proof of the Fundamental Theorem
6. The Dancing Tea Cup
7. The Kinetic Energy of a Rigid System
8. Motion of Space with One Point Fixed
9. Vector Angular Velocity
10. Moving Axes. Proof of the Theorem of 8
11. Space Centrode and Body Centrode
12. Motion of Space. General Case
13. The Ruled Surfaces
14. Relative Velocities
15. Proof of the Theorem of 12
16. Lissajou's Curves
17. Continuation. The General Case. The Commensurable Case. Periodicity
Professor Sabine's Tracings of Lissajou's Curves between pages

CHAPTER VI - ROTATION
1. Moments of Inertia
2. Principal Axes of a Central Quadric
3. Continuation. Determination of the Axes
4. Moment of Momentum. Moment of a Localized Vector
5. The Fundamental Theorem of Moments
6. Vector Form for the Motion of the Centre of Mass
7. The Invariable Line and Plane
8. Transformation of
9. Moments about the Centre of Mass
10. Moments about an Arbitrary Point
11. Moments about the Instantaneous Centre
12. Evaluation of a for a Rigid System; One Point Fixed
13. Euler's Dynamical Equations
14. Motion about a Fixed Point
15. Euler's Geometrical Equations
16. Continuation. The Direction Cosines of the Moving Axes
17. The Gyroscope
18. The Top
19. Continuation. Discussion of the Motion
20. Intrinsic Treatment of the Gyroscope
21. The Relations Connecting v, F, and K
22. Discussion of the Intrinsic Equations
23. Billiard Ball
24. Cartwheels
25. Resume

CHAPTER VII - WORK AND ENERGY
1. Work
2. Continuation: Curved Paths
3. Field of Force. Force Function. Potential
4. Conservation of Energy
5. Vanishing of the Internal Work for a Rigid System
6. Kinetic Energy of a Rigid Body
7. Final Definition of Work
8. Work Done by a Moving Stairway
9. Other Cases in Which the Internal Work Vanishes
10. Work and Energy for a Rigid Body

CHAPTER VIII - IMPACT
1. Impact of Particles
2. Continuation. Oblique Impact
3. Rigid Bodies
4. Proof of the Theorem
5. Tennis Ball, Returned with a Lawford

CHAPTER IX - RELATIVE MOTION AND MOVING AXES
1. Relative Velocity
2. Linear Velocity in Terms of Angular Velocity
3. Acceleration
4. The Dynamical Equations
5. The Centrifugal Field
6. Foucault Pendulum

CHAPTER X - LAGRANGE'S EQUATIONS AND VIRTUAL VELOCITIES
1. The Problem
2. Lagrange's Equations in the Simplest Case
3. Continuation. Particle on a Fixed or Moving Surface
4. The Spherical Pendulum
5. Geodesies
6. Lemma
7. Lagrange's Equations in the General Case
8. Discussion of the Equations. Holonomic and Non-Holonomic Systems
9. Continuation. The Forces
10. Conclusion. Lagrange's Multipliers
11. Virtual Velocities and Virtual Work
12. Computation of Qr
13. Virtual Velocities, an Aid in the Choice of the pi
14. On the Number m of the Qr
15. Forces of Constraint
16. Euler's Equations, Deduced from Lagrange's Equations
17. Solution of Lagrange's Equations
18. Equilibrium
19. Small Oscillations
Exercises on Chapter X

CHAPTER XI - HAMILTON'S CANONICAL EQUATIONS
1. The Problem
2. A General Theorem
3. Proof of Hamilton's Equations

CHAPTER XII - D'ALEMBERT'S PRINCIPLE
1. The Problem
2. Lagrange's Equations for a System of Particles, Deduced from d'Alembert's Principle
3. The Six Equations for a System of Particles, Deduced from d'Alembert's Principle
4. Lagrange's Equations in the General Case, and d'Alembert's Principle
5. Application : Euler's Dynamical Equations
6. Examples

CHAPTER XIII - HAMILTON'S PRINCIPLE AND THE PRINCIPLE OF LEAST ACTION
1. Definition
2. The Integral of Rational Mechanics
3. Application to the Integral of Kinetic Energy
4. Virtual Work
5. The Fundamental Equation
6. The Variational Principle
7. Hamilton's Principle
8. Lagrange's Principle of Least Action
9. Jacobi's Principle of Least Action
10. Critique of the Methods. Retrospect and Prospect
11. Applications
12. Hamilton's Integral a Minimum in a Restricted Region
13. Jacobi's Integral a Minimum in a Restricted Region

CHAPTER XIV - CONTACT TRANSFORMATIONS
1. Purpose of the Chapter
2. Integral Invariants
3. Consequences of the Theorem
4. Transformation of Hamilton's Equations by Contact Transformations
5. Particular Contact Transformations
6. Theft-Relations

CHAPTER XV - SOLUTION OF HAMILTON'S EQUATIONS
1. The Problem and Its Treatment
2. Reduction to the Equilibrium Problem
3. Example. Simple Harmonic Motion
4. H, Independent of t.
5. Examples. Projectile in vacuo
6. Comparison of the Two Methods
7. Cyclic Coordinates
8. Continuation. The General Case
9. Examples. The Two-Body Problem
10. Continuation. The Top
11. Perturbations. Variation of Constants
12. Continuation. A Second Method


DOWNLOAD FREE BOOK:   Mechanics


Free books category: