  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.

General Relativity and Quantum Cosmology