Coordinate families for the Schwarzschild geometry based on radial timelike geodesics
Abstract
We explore the connections between various coordinate systems associated with observers moving inwardly along radial geodesics in the Schwarzschild geometry. Painlev\'e-Gullstrand (PG) time is adapted to freely falling observers dropped from rest from infinity; Lake-Martel-Poisson (LMP) time coordinates are adapted to observers who start at infinity with non-zero initial inward velocity; Gautreau-Hoffmann (GH) time coordinates are adapted to observers dropped from rest from a finite distance from the black hole horizon. We construct from these an LMP family and a proper-time family of time coordinates, the intersection of which is PG time. We demonstrate that these coordinate families are distinct, but related, one-parameter generalizations of PG time, and show linkage to Lema\^itre coordinates as well.
Keywords
Cite
@article{arxiv.1211.4337,
title = {Coordinate families for the Schwarzschild geometry based on radial timelike geodesics},
author = {Tehani K. Finch},
journal= {arXiv preprint arXiv:1211.4337},
year = {2015}
}
Comments
13 pages and 10 figures. New title and abstract; expanded discussion on Gautreau-Hoffmann coordinates, and coordinate classifications; figures added; references added. Submitted for publication