Neutrino pair annihilation ($ν{\bar ν}\to e^-e^+$) in the presence of quintessence surrounding a black hole

G. Lambiase; L. Mastrototaro

doi:10.1140/epjc/s10052-021-09732-2

paper

Neutrino pair annihilation ( $ν ν ˉ \to e^{-} e^{+}$ ) in the presence of quintessence surrounding a black hole

arXiv:2012.09100 · doi:10.1140/epjc/s10052-021-09732-2

Abstract

Quintessence fields, introduced to explain the speed-up of the Universe, might affect the geometry of spacetime surrounding black holes, as compared to the standard Schwarzschild and Kerr geometries. In this framework, we study the neutrino pairs annihilation into electron-positron pairs ( $ν ν ˉ \to e^{-} e^{+}$ ) near the surface of a neutron star, focusing, in particular, on the Schwarzschild-like geometry in presence of quintessence fields. The effect of the latter is to increase the minimum photon-sphere radius ( $R_{p h}$ ), increasing in such a way the maximum energy deposition rate near to $R_{p h}$ . The rate turns out to be several orders of magnitude greater than the rate computed in the framework of General Relativity. These results might provide an efficient mechanism for the generation of GRBs and lead to constraints on the parameters of the quintessence model.

arXiv comment22 pages, 8 figures

Neutrino pair annihilation ( $ν ν ˉ \to e^{-} e^{+}$ ) in the presence of quintessence surrounding a black hole

Abstract

References in corpus (98)

Cited by in corpus (8)

Neutrino pair annihilation (ννˉ→e−e+) in the presence of quintessence surrounding a black hole

Abstract

References in corpus (98)

Cited by in corpus (8)

Neutrino pair annihilation ( $ν ν ˉ \to e^{-} e^{+}$ ) in the presence of quintessence surrounding a black hole