2016
DOI: 10.22606/adap.2016.13006
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Rotating Black Holes in Microscopic Theory: the Implications for Periodic Source M82X-2

Abstract: 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 bein… Show more

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Cited by 5 publications
(9 citation statements)
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References 14 publications
(30 reference statements)
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“…The resulting bilinear form of norm d s 2 of infinitesimal displacement on V 4 describes the metric of the stationary and axisymmetric space V 4 [2] in the most commonly used 3 + 1 formalisms. In the 3 + 1 formalism, as usual, 3+1 foliations of spacetime V 4 by space-like 3-slices {Σ t } play an important role.…”
Section: Axisymmetric 4d Spacetimementioning
confidence: 99%
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“…The resulting bilinear form of norm d s 2 of infinitesimal displacement on V 4 describes the metric of the stationary and axisymmetric space V 4 [2] in the most commonly used 3 + 1 formalisms. In the 3 + 1 formalism, as usual, 3+1 foliations of spacetime V 4 by space-like 3-slices {Σ t } play an important role.…”
Section: Axisymmetric 4d Spacetimementioning
confidence: 99%
“…In the case of stationary and axisymmetric space V 4 , the dimensionless potentials of the 1D gravitation filed x 0 , the frame-dragging potential x 1 , and the ID fieldx, are generated by the stress-energy tensor of isolated spinning fluid T → 0 [2]. The existence of a global vacuum solution, χ (≡ x 0 , x 1 ), outside of the matter (x = 0), amounts to solving the field equations in a nearly Newtonian weak source limit: T → 0.…”
Section: Axisymmetric 4d Spacetimementioning
confidence: 99%
See 3 more Smart Citations