Astronomy and Astrophysics – Astrophysics
Scientific paper
1999-09-22
Astropart.Phys.13:295-300,2000
Astronomy and Astrophysics
Astrophysics
Latex 8 pages; no figures; UMD-PP-00-024
Scientific paper
10.1016/S0927-6505(99)00127-9
Mirror matter models have been suggested recently as an explanation of neutrino puzzles and microlensing anomalies. We show that mirror supernovae can be a copious source of energetic gamma rays if one assumes that the quantum gravity scale is in the TeV range. We show that under certain assumptions plausible in the mirror models, the gamma energies could be degraded to the 10 MeV range (and perhaps even further) so as to provide an explanation of observed gamma ray bursts. This mechanism for the origin of the gamma ray bursts has the advantage that it neatly avoids the ``baryon load problem''.
Mohapatra Rabindra N.
Nussinov Shmuel
Teplitz Vigdor L.
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