Advances in Astrophysics

Download PDF (5484.6 KB) PP. 162 - 183 Pub. Date: August 18, 2017

DOI: 10.22606/adap.2017.23003

• Gagik Ter-Kazarian^*
  Phys. Dept.College of Science, SQU, POBox 36, Postal Code 123, Al-Khoud, OMAN
• Saleh Al Shidhani
  Phys. Dept.College of Science, SQU, POBox 36, Postal Code 123, Al-Khoud, OMAN

Recently observed rare mighty X-ray coherent pulsations coming from M82X-2 impose a significant challenge in breaking the Eddington limit. Alternative approach to circumvent the obstacles was studied in [1,2] by addressing the M82X-2 as a spinning intermediate mass black hole, resided in final stage of growth. This approach employs the microscopic theory of black hole (MTBH), which explores a spontaneous breaking of gravitation gauge symmetry at huge energies. The preceding developments of this theory are proved to be quite fruitful for addressing the growth and merging phenomena of the black hole seeds. It explains as well the origin of ZeV-neutrinos, which are of vital interest for the source of ultra-high energy particles. In the present work, we further expose the assertions made in previous model via a computation of essential astrophysical corrections introduced by the rotation to 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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