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