General relativistic massive vector field effects in Gamma Ray Burst production
Fabrizio Tamburini, Mariafelicia De Laurentis, Lorenzo Amati, Bo, Thid\'e

TL;DR
This paper proposes a new energy extraction mechanism from rotating black holes using a massive photon field, potentially explaining the high energies observed in Gamma Ray Bursts without requiring collimation.
Contribution
It introduces a novel theoretical model for energy extraction from Kerr-Newman black holes via a massive photon field, with numerical validation of its stability and energy output.
Findings
Can extract energies up to 10^{54} erg from black holes.
Mechanism is stable across different black hole rotation parameters.
Provides a lower bound on electromagnetic-gravitational coupling.
Abstract
To explain the extremely high energy release, ~erg, suggested by the observations of some Gamma Ray Bursts (GRBs) we propose a new energy extraction mechanism from the rotation energy of a Kerr-Newman black hole (BH) by a massive photon field. Numerical results show that this mechanism is stable with respect to the black hole rotation parameter, , with a clear dependence on the BH mass, , and charge, , and can extract energies up to erg. The controversial "energy crisis" problem of GRBs that does not show evidence for collimated emission may benefit of this energy extraction mechanism. With these results we set a lower bound on the coupling between electromagnetic and gravitational fields.
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