A timelike geodesic has timelike tangent and vanishing covariant acceleration in an affine parameter. Choosing proper time gives .
Physically, an ideal massive test particle in free fall follows a timelike geodesic when nongravitational forces and appreciable self-gravity can be neglected. The normalization above uses ; in SI units it is . Zero covariant acceleration does not mean constant coordinate velocity: a dropped object accelerates relative to the ground. Conversely, a person standing on the ground is pushed away from free fall by the supporting surface. A photon follows a null geodesic, whose parameter cannot be proper time. See Tong's geodesics in spacetime.
For and , the conformal factor makes spatial translation a Killing vector field. Using proper time, its conserved momentum is . With and this becomesThus alone is not constant. Set . Every unparametrized timelike geodesic in a connected nonzero- patch has the formThe nonvertical paths have and proper-time parametrizationThe chart excludes , where its metric is degenerate; a vertical family must not be lost by dividing by the conserved momentum.
For , with smooth odd and , the conserved energy gives and . Both half-cycle integrals over contain an even weight times . The odd contribution vanishes, leaving the unperturbed half-period in each clock. The waveforms need not be sinusoidal, but both periods are unchanged for .
In a positive-time patch, proper-time first integrals give and . If , the unparametrized timelike geodesics are on an appropriate branch; in the expanded quadratic form their discriminant is positive. If , there is the separate family , . A description using only the nonvertical quadratic family omits genuine timelike geodesics.
Articles by others on the same topic
There are currently no matching articles.