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Physics NotePublished

Weak-Scale Hidden Sector and Energy Transport in Fireball Models of Gamma-Ray Bursts

Durmus A. Demir; Herman J. Mosquera Cuesta

2000

Publication details

Authors
Durmus A. Demir; Herman J. Mosquera Cuesta
Type
Physics Note
Status
Published
Publication date
2000
Description
The annihilation of pairs of very weakly interacting particles in the neibourghood of gamma-ray sources is introduced here as a plausible mechanism to overcome the baryon load problem. This way we can explain how these very high energy gamma-ray bursts can be powered at the onset of very energetic events like supernovae (collapsars) explosions or coalescences of binary neutron stars. Our approach uses the weak-scale hidden sector models in which the Higgs sector of the standard model is extended to include a gauge singlet that only interacts with the Higgs particle. These particles would be produced either during the implosion of the red supergiant star core or at the aftermath of a neutron star binary merger. The whole energetics and timescales of the relativistic blast wave, the fireball, are reproduced.
Year
2000
Number
CBPF-NF-079/00
Linked to a thesis
No
Linked to a grant
No
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