Pulsations of spherically symmetric systems in general relativity
- 15 January 1996
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review D
- Vol. 53 (2) , 754-761
- https://doi.org/10.1103/physrevd.53.754
Abstract
The pulsation equations for spherically symmetric black hole and soliton solutions are brought into a standard form. The formulae apply to a large class of field theoretical matter models and can easily be worked out for specific examples. The close relation to the energy principle in terms of the second variation of the Schwarzschild mass is also established. The use of the general expressions is illustrated for the Einstein-Yang-Mills and the Einstein-Skyrme system.Comment: 21 pages, latex, no figureKeywords
All Related Versions
This publication has 23 references indexed in Scilit:
- New black hole solutions with hairPublished by Elsevier ,2002
- Linear stability of Einstein-Skyrme black holesPhysics Letters B, 1992
- A classical instability of Reissner-Nordström solutions and the fate of magnetically charged black holesPhysical Review Letters, 1992
- Stability analysis of self-gravitating skyrmionsPhysics Letters B, 1991
- Nonlinear perturbations of Einstein-Yang-Mills solitons and non-abelian black holesNuclear Physics B, 1991
- Colored black holesPhysical Review Letters, 1990
- Instability of a colored black hole solutionPhysics Letters B, 1990
- Spherically symmetric static SU(2) Einstein–Yang–Mills fieldsJournal of Mathematical Physics, 1990
- Instability of the Bartnik-McKinnon solution of the Einstein-Yang-Mills equationsPhysics Letters B, 1990
- Particlelike Solutions of the Einstein-Yang-Mills EquationsPhysical Review Letters, 1988