Advances in Astrophysics

Download PDF (2562.3 KB) PP. 201 - 223 Pub. Date: November 1, 2016

DOI: 10.22606/adap.2016.13006

• Gagik Ter-Kazarian^*
  Ambartsumian Byurakan Astrophysical Observatory Byurakan 378433, Aragatsotn District, Armenia

In previous paper [1], we employ the microscopic theory of black hole to study the observed unusual high luminosity of NuSTAR X-ray pulsations from M82X-2 without the need for significant breaking of Eddington limit. Exploring a spontaneous breaking of gravitation gauge symmetry at huge energies, this theory has smeared out a central singularity of black hole replacing it by the equilibrium, so-called, superdense proto-matter core (SPC), subject to certain rules. In this framework, we think of a M82X-2 as being a spinning intermediate mass black hole. However, for rigorous theoretical solutions, in present report we analytically treat the microscopic model of stationary and axisymmetric rotating black hole. A ring singularity of the Kerr black hole cannot occur, which is now replaced by equilibrium SPC. We calculate the corrections to previous model, introduced by the rotation, of the characteristic phase profile of M82X-2.

Black hole physics, accretion: accretion discs, X-rays: binaries, X-rays: individual (NuSTAR J095551+6940.8).

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