Pulsation of Spherically Symmetric Systems in General Relativity
arXiv:gr-qc/9506027 · doi: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.
21 pages, latex, no figures
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- Self-adjoint wave equations for dynamical perturbations of self-gravitating fields
- Einstein-Yang-Mills solitons: towards new degrees of freedom
- On the instabilities of the static, spherically symmetric SU(2) Einstein-Yang-Mills-Dilaton solitons and black holes
- Can Dirac fermions Destroy Yang-Mills Black Hole?