2021/10/06 by L. Mastrototaro, G. Lambiase, Mastrototaro, L. +1
Physics and Astronomy · #FOS: Physical sciences #High Energy Astrophysical Phenomena (astro-ph.HE) #astro-ph.HE
paper · pdf · doi:10.48550/arxiv.2110.02996
12 pages, Contributed to Marcel Grossmann Meeting, Rome, 05 Jul. 2021. arXiv admin note: text overlap with arXiv:2009.08722
arxiv created 2021/10/06 · arxiv updated 2021/10/08
We present our studies on the neutrino pairs annihilation into electron-positron pairs (ν ν→ e-e+) near the surface of a neutron star in the framework of extended theories of gravity. The latter modifies the maximum energy deposition rate near to the photonsphere and it might be several orders of magnitude greater than that computed in the framework of General Relativity. These results provide a rising in the Gamma-Ray Bursts energy emitted from a close binary neutron star system and might be a fingerprint of modified theories of gravity, changing our view of astrophysical phenomena.