§50 General properties of motion in S dimensions 161 ordinates. For the quantities Ii are one-valued integrals of the motion in co-ordinates which allow separation of the variables. When degeneracy occurs, the number of one-valued integrals exceeds S, and so the choice of those which are the desired I is no longer unique. As an example, we may again mention Keplerian motion, which allows separation of the variables in both spherical and parabolic co-ordinates. In §49 it has been shown that, for finite motion in one dimension, the action variable is an adiabatic invariant. This statement holds also for systems with more than one degree of freedom. Here we shall give a proof valid for the general case. Let X(t) be again a slowly varying parameter of the system. In the canonical transformation from the variables P, q to I, W, the generating function is, as we know, the action So(q, I). This depends on A as a parameter and, if A is a func- tion of time, the function So(q, I; X(t)) depends explicitly on time. In such a case the new Hamiltonian H' is not the same as H, i.e. the energy E(I), and by the general formulae (45.8) for the canonical transformation we have H' E(I)+asoldt = E(I)+A, where A III (aso/ad)r. Hamilton's equations give ig = - (50.15) We average this equation over a time large compared with the fundamental periods of the system but small compared with the time during which the parameter A varies appreciably. Because of the latter condition we need not average 1 on the right-hand side, and in averaging the quantities we may regard the motion of the system as taking place at a constant value of A and therefore as having the properties of conditionally periodic motion described above. The action So is not a one-valued function of the co-ordinates: when q returns to its initial value, So increases by an integral multiple of 2I. The derivative A = (aso/ax), is a one-valued function, since the differentiation is effected for constant Ii, and there is therefore no increase in So. Hence A, expressed as a function of the angle variables Wr, is periodic. The mean value of the derivatives of such a function is zero, and therefore by (50.15) we have also which shows that the quantities Ii are adiabatic invariants. Finally, we may briefly discuss the properties of finite motion of closed systems with S degrees of freedom in the most general case, where the vari- ables in the Hamilton-Jacobi equation are not assumed to be separable. The fundamental property of systems with separable variables is that the integrals of the motion Ii, whose number is equal to the number of degrees + To simplify the formulae we assume that there is only one such parameter, but the proof is valid for any number. 162 The Canonical Equations §50 of freedom, are one-valued. In the general case where the variables are not separable, however, the one-valued integrals of the motion include only those whose constancy is derived from the homogeneity and isotropy of space and time, namely energy, momentum and angular momentum. The phase path of the system traverses those regions of phase space which are defined by the given constant values of the one-valued integrals of the motion. For a system with separable variables and S one-valued integrals, these conditions define an s-dimensional manifold (hypersurface) in phase space. During a sufficient time, the path of the system passes arbitrarily close to every point on this hypersurface. In a system where the variables are not separable, however, the number of one-valued integrals is less than S, and the phase path occupies, completely or partly, a manifold of more than S dimensions in phase space. In degenerate systems, on the other hand, which have more than S integrals of the motion, the phase path occupies a manifold of fewer than S dimensions. If the Hamiltonian of the system differs only by small terms from one which allows separation of the variables, then the properties of the motion are close to those of a conditionally periodic motion, and the difference between the two is of a much higher order of smallness than that of the additional terms in the Hamiltonian. PROBLEM Calculate the action variables for elliptic motion in a field U = -a/r. SOLUTION. In polar co-ordinates r, in the plane of the motion we have 'max = 1+av(m2)E) Hence the energy, expressed in terms of the action variables, is E = It depends only on the sum Ir+I, and the motion is therefore degenerate; the two funda- mental frequencies (in r and in b) coincide. The parameters P and e of the orbit (see (15.4)) are related to Ir and I by p= Since Ir and I are adiabatic invariants, when the coefficient a or the mass m varies slowly the eccentricity of the orbit remains unchanged, while its dimensions vary in inverse propor- tion to a and to m. INDEX Acceleration, 1 Coriolis force, 128 Action, 2, 138ff. Couple, 109 abbreviated, 141 Cross-section, effective, for scattering, variable, 157 49ff. Additivity of C system, 41 angular momentum, 19 Cyclic co-ordinates, 30 energy, 14 integrals of the motion, 13 d'Alembert's principle, 124 Lagrangians, 4 Damped oscillations, 74ff. mass, 17 Damping momentum, 15 aperiodic, 76 Adiabatic invariants, 155, 161 coefficient, 75 Amplitude, 59 decrement, 75 complex, 59 Degeneracy, 39, 69, 160f. Angle variable, 157 complete, 160 Angular momentum, 19ff. Degrees of freedom, 1 of rigid body, 105ff. Disintegration of particles, 41ff. Angular velocity, 97f. Dispersion-type absorption, 79 Area integral, 31n. Dissipative function, 76f. Dummy suffix, 99n. Beats, 63 Brackets, Poisson, 135ff. Eccentricity, 36 Eigenfrequencies, 67 Canonical equations (VII), 131ff. Elastic collision, 44 Canonical transformation, 143ff. Elliptic functions, 118f. Canonical variables, 157 Elliptic integrals, 26, 118 Canonically conjugate quantities, 145 Energy, 14, 25f. Central field, 21, 30 centrifugal, 32, 128 motion in, 30ff. internal, 17 Centrally symmetric field, 21 kinetic, see Kinetic energy Centre of field, 21 potential, see Potential energy Centre of mass, 17 Equations of motion (I), 1ff. system, 41 canonical (VII), 131ff. Centrifugal force, 128 integration of (III), 25ff. Centrifugal potential, 32, 128 of rigid body, 107ff. Characteristic equation, 67 Eulerian angles, 110ff. Characteristic frequencies, 67 Euler's equations, 115, 119 Closed system, 8 Collisions between particles (IV), 41ff. Finite motion, 25 elastic, 44ff. Force, 9 Combination frequencies, 85 generalised, 16 Complete integral, 148 Foucault's pendulum, 129f. Conditionally periodic motion, 160 Frame of reference, 4 Conservation laws (II), 13ff. inertial, 5f. Conservative systems, 14 non-inertial, 126ff. Conserved quantities, 13 Freedom, degrees of, 1 Constraints, 10 Frequency, 59 equations of, 123 circular, 59 holonomic, 123 combination, 85 Co-ordinates, 1 Friction, 75, 122 cyclic, 30 generalised, 1ff. Galilean transformation, 6 normal, 68f. Galileo's relativity principle, 6 163 164 Index General integral, 148 Mechanical similarity, 22ff. Generalised Molecules, vibrations of, 70ff. co-ordinates, 1ff. Moment forces, 16 of force, 108 momenta, 16 of inertia, 99ff. velocities, 1ff. principal, 100ff. Generating function, 144 Momentum, 15f. angular, see Angular momentum Half-width, 79 generalised, 16 Hamiltonian, 131f. moment of, see Angular momentum Hamilton-Jacobi equation, 147ff. Multi-dimensional motion, 158ff. Hamilton's equations, 132 Hamilton's function, 131 Hamilton's principle, 2ff. Newton's equations, 9 Holonomic constraint, 123 Newton's third law, 16 Nodes, line of, 110 Impact parameter, 48 Non-holonomic constraint, 123 Inertia Normal co-ordinates, 68f. law of, 5 Normal oscillations, 68 moments of, 99ff. Nutation, 113 principal, 100ff. principal axes of, 100 One-dimensional motion, 25ff., 58ff. tensor, 99 Oscillations, see Small oscillations Inertial frames, 5f. Oscillator Infinite motion, 25 one-dimensional, 58n. Instantaneous axis, 98 space, 32, 70 Integrals of the motion, 13, 135 Jacobi's identity, 136 Particle, 1 Pendulums, 11f., 26, 33ff., 61, 70, 95, Kepler's problem, 35ff. 102f., 129f. Kepler's second law, 31 compound, 102f. Kepler's third law, 23 conical, 34 Kinetic energy, 8, 15 Foucault's, 129f. of rigid body, 98f. spherical, 33f. Perihelion, 36 Laboratory system, 41 movement of, 40 Lagrange's equations, 3f. Phase, 59 Lagrangian, 2ff. path, 146 for free motion, 5 space, 146 of free particle, 6ff. Point transformation, 143 in non-inertial frame, 127 Poisson brackets, 135ff. for one-dimensional motion, 25, 58 Poisson's theorem, 137 of rigid body, 99 Polhodes, 117n. for small oscillations, 58, 61, 66, 69, 84 Potential energy, 8, 15 of system of particles, 8ff. centrifugal, 32, 128 of two bodies, 29 effective, 32, 94 Latus rectum, 36 from period of oscillation, 27ff. Least action, principle of, 2ff. Potential well, 26, 54f. Legendre's transformation, 131 Precession, regular, 107 Liouville's theorem, 147 L system, 41 Rapidly oscillating field, motion in, 93ff. Reactions, 122 Mass, 7 Reduced mass, 29 additivity of, 17 Resonance, 62, 79 centre of, 17 in non-linear oscillations, 87ff. reduced, 29 parametric, 80ff. Mathieu's equation, 82n. Rest, system at, 17 Maupertuis' principle, 141 Reversibility of motion, 9 Index 165 Rigid bodies, 96 Space angular momentum of, 105ff. homogeneity of, 5, 15 in contact, 122ff. isotropy of, 5, 18 equations of motion of, 107ff. Space oscillator, 32, 70 motion of (VI), 96ff. Rolling, 122 Time Rotator, 101, 106 homogeneity of, 5, 13ff. Rough surface, 122 isotropy of, 8f. Routhian, 134f. Top Rutherford's formula, 53f. asymmetrical, 100, 116ff. "fast", 113f. spherical, 100, 106 Scattering, 48ff. symmetrical, 100, 106f., 111f. cross-section, effective, 49ff. Torque, 108 Rutherford's formula for, 53f. Turning points, 25, 32 small-angle, 55ff. Two-body problem, 29 Sectorial velocity, 31 Separation of variables, 149ff. Uniform field, 10 Similarity, mechanical, 22ff. Sliding, 122 Variation, 2, 3 Small oscillations, 22, (V) 58ff. first, 3 anharmonic, 84ff. Velocity, 1 damped, 74ff. angular, 97f. forced, 61ff., 77ff. sectorial, 31 free, 58ff., 65ff. translational, 97 linear, 84 Virial, 23n. non-linear, 84ff. theorem, 23f. normal, 68 Smooth surface, 122 Well, potential, 26, 54f. PHYSICS The enormous increase in the number and size of scientific journals has led to a qualitative change in the problem of scientific communication. The policies of most journals are based on the old need to ensure that no valid science was lost to the scientific public by being rejected ; the problem now seems to be whether almost all good science will be buried among mountains of valid but mediocre work, or secreted in specialized publications. The scientist reads only a tiny fraction of physics, either sharply specialized or selected at random, by rumour or by the author's reputation. 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