Black Hole in Binary System is the Source of Cosmic Gamma-Ray Bursts and Their Counterparts
Alexander Vasilievich Kuznetsov

TL;DR
This paper links cosmic gamma-ray bursts to black hole binaries, demonstrating how their properties and observed data can be used to identify sources, measure black hole masses, and clarify the true origin of GRBs.
Contribution
It introduces a novel method to determine the source locations of GRBs and measure black hole masses using relativistic effects observed in GRB clusters.
Findings
GRB sources are identified with black hole binaries
A technique for measuring black hole masses is developed
The cosmological origin of GRBs is challenged
Abstract
Discovery of GRB clusters allows us to determine coordinates and characteristics of their sources. The objects radiating GRBs are reliably identified with black hole binaries, including the Galactic binaries. One of the unusual GRB properties, which are determined by black hole, is revealed in that the measured arrival direction of GRB does not coincide with the real location of its source. Just this fact allows us to find the objects radiating GRBs. On the basis of the general relativity theory's effects, observed in the GRB clusters, the technique of the black hole masses measurement is developed. The calculated black hole masses for the majority of known Galactic BH binaries are presented. It is briefly shown how the incorrect interpretations of observational facts result in an erroneous idea of the GRB cosmological origin. In fact, two problems are solved in the paper: the GRB…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsGamma-ray bursts and supernovae · Astronomy and Astrophysical Research · Astrophysical Phenomena and Observations
