The energy of a curve #
The energy of a curve γ in a Riemannian manifold between the parameters a and b is
E(γ) = ½ ∫_a^b ‖γ'(t)‖² dt, where γ' is the velocity TauCeti.Manifold.curveVelocity. This
file defines it and records its elementary properties: it vanishes on constant curves and on
degenerate parameter intervals, changes sign under reversal of the parameter interval, and is
nonnegative on positively oriented ones, and adds over adjacent parameter intervals. On a
parameter set s containing the interval, it may equally be computed from the within-set velocity
TauCeti.Manifold.curveVelocityWithin, which is the form used for geodesics on closed intervals,
where the unrestricted velocity can take junk values at the endpoints. Its first
variation is in TauCeti.Geometry.Manifold.Riemannian.FirstVariation.Basic, and its value on
geodesic segments is in TauCeti.Geometry.Manifold.Riemannian.Geodesic.ConstantSpeed.
Main definitions and results #
TauCeti.Manifold.energy: the energy of a curve between two parameters.TauCeti.Manifold.energy_const,TauCeti.Manifold.energy_self: the energy vanishes on a constant curve and on a degenerate parameter interval.TauCeti.Manifold.energy_symm,TauCeti.Manifold.energy_nonneg: the energy is odd in the orientation of the parameter interval and nonnegative on positively oriented ones.TauCeti.Manifold.energy_add_adjacent: the energy is additive over adjacent parameter intervals.TauCeti.Manifold.energy_congr: energy depends only on the open-interval restriction.TauCeti.Manifold.sum_energy_adjacent_intervals: energy is additive over finite partitions.TauCeti.Manifold.energy_eq_integral_curveVelocityWithin: the energy computed from the velocity within any parameter set containing the interval.
References #
- J. Milnor, Morse Theory, Annals of Mathematics Studies 51, Princeton, 1963, §12, the energy of a path.
- M. P. do Carmo, Riemannian Geometry, Birkhäuser, 1992, Ch. 9, §2.
The energy of a curve γ between the parameters a and b: half the integral of its
squared Riemannian speed, E(γ) = ½ ∫_a^b ‖γ'(t)‖² dt. It is meant for curves which are C¹
near [a, b]; for other curves the integrand may take junk values.
Instances For
The defining formula for the energy.
A constant curve has zero energy.
The energy over a degenerate parameter interval vanishes.
Reversing the parameter interval changes the sign of the energy.
The energy over a positively oriented parameter interval is nonnegative.
The energy is additive over adjacent parameter intervals, provided the squared speed is integrable on both.
Curves agreeing near a parameter have the same Riemannian speed there.
Energy depends only on the curve on the open parameter interval; values at its endpoints and outside the interval do not affect the integral.
Energy is additive over any finite partition on which the squared speed is integrable. The partition need not be strict or increasing.
On any parameter set s containing the interval between a and b, the energy may be
computed from the velocity within s. The two velocities agree on the open interval, so no
regularity of γ is needed.