Possible Alternate Scenario for short Duration GRBs
C Sivaram (1), Kenath Arun (2) ((1) Indian Institute of, Astrophysics, Bangalore; (2) Christ Junior College, Bangalore)

TL;DR
This paper proposes a new class of dark matter objects as potential sources of short-duration gamma-ray bursts and as a formation mechanism for sub-stellar black holes, addressing existing theoretical challenges.
Contribution
It introduces dark matter-based objects as an alternative explanation for short GRBs and black hole formation, offering a novel scenario beyond traditional baryonic models.
Findings
Dark matter objects could produce short GRBs without baryon load issues.
These objects may lead to the formation of sub-stellar black holes.
The proposed scenario provides an alternative to conventional black hole formation theories.
Abstract
In this paper we look at new class of objects made up entirely of dark matter particles. We look at these objects as possible candidate for short duration gamma ray bursts eliminating the baryon load problem. These could also provide a possible scenario for the formation of sub-stellar black holes, distinct from the usual Hawking black hole.
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Taxonomy
TopicsCosmology and Gravitation Theories · Gamma-ray bursts and supernovae · Particle physics theoretical and experimental studies
