Matter symmetries in general relativistic kinetic theory
- 1 September 1973
- journal article
- Published by AIP Publishing in Journal of Mathematical Physics
- Vol. 14 (9) , 1254-1257
- https://doi.org/10.1063/1.1666475
Abstract
It is shown that a surface forming matter symmetry for collision-free general relativistic kinetic theory gives rise to an isometry on the space-time. Specific solutions are given, and it is shown that limiting the surface forming conditions to the mass subbundle does not alter the results. A possible method for solving more general cases is given.Keywords
This publication has 2 references indexed in Scilit:
- Relativistic, Spherically Symmetric Star Clusters. I. Stability Theory for Radial PerturbationsThe Astrophysical Journal, 1968
- Isotropic Solutions of the Einstein-Liouville EquationsJournal of Mathematical Physics, 1968