Solving Einstein's equations for rotating spacetimes: Evolution of relativistic star clusters
- 15 May 1994
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review D
- Vol. 49 (10) , 5153-5164
- https://doi.org/10.1103/physrevd.49.5153
Abstract
No abstract availableThis publication has 16 references indexed in Scilit:
- Relativistic Stellar Systems with Spindle SingularitiesThe Astrophysical Journal, 1993
- Critical behavior and scaling in vacuum axisymmetric gravitational collapsePhysical Review Letters, 1993
- Trapping a geon: Black hole formation by an imploding gravitational wavePhysical Review D, 1992
- Numerically generated black-hole spacetimes: Interaction with gravitational wavesPhysical Review D, 1992
- Collisions of relativistic clusters and the formation of black holesPhysical Review D, 1992
- Gravitational collapse of rotating spheroids and the formation of naked singularitiesPhysical Review D, 1992
- Formation of naked singularities: The violation of cosmic censorshipPhysical Review Letters, 1991
- A general relativistic code for rotating axisymmetric configurations and gravitational radiation: Numerical methods and testsComputer Physics Reports, 1987
- Gravitational-Wave Emission from Rotating Gravitational CollapsePhysical Review Letters, 1985
- General Relativistic Collapse of Axially Symmetric Stars Leading to the Formation of Rotating Black HolesProgress of Theoretical Physics, 1981