Perturbations of the spherically symmetric collapsar in the relativistic theory of gravitation: axial perturbations. I
arXiv:gr-qc/0405032
Abstract
Horizon solutions for the axial perturbations of the spherically symmetric metric are analyzed in the framework of the relativistic theory of gravitation. The gravitational perturbations can not be absorbed by the horizon that results in the excitation of the new type of the normal modes trapped by the Regge-Wheeler potential. The obtained results demonstrate testable differences between the collapsar and the black hole near-horizon physics.
11 pages, 1 colour figure, supplemented version, Maple 9 worksheet: http://ares.photonik.tuwien.ac.at/BHperturbations.html