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General relativistic electromagnetic and massive vector field effects with gamma-ray burst production

Tamburini, Fabrizio (author)
ZKM Centre for Art and Technologies for Media, Germany
De Laurentis, Mariafelicia (author)
Goethe University, Germany; Tomsk State Pedagogical University, Russia; TUSUR Tomsk State University of Control Systems and Radioelectronics, Russia; Istituto Nazionale di Fisica Nucleare Sezione di Napoli, Italy
Amati, Lorenzo (author)
Istituto Nazionale di Astrofisica, Italy; International Center for Relativistic Astrophysics, Italy
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Thidé, Bo (author)
RISE,Acreo,Swedish Institute of Space Physics, Sweden
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 (creator_code:org_t)
2017
2017
English.
In: Physical Review D. - 2470-0010 .- 2470-0029. ; 96:10
  • Journal article (peer-reviewed)
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  • We propose a new energy extraction mechanism from the rotational energy of a Kerr-Newman black hole by a gravitating massive photon field generated by electromagnetic and gravitational field coupling effects. Numerical studies show that this mechanism that depends on the black hole rotation parameter, a, shows a clear dependence on the black hole mass, M, and charge, Q, and can extract energies up to 1054 erg for a black hole of the solar mass size. With this mechanism we can set a lower bound on the coupling ξ∼10-38 between electromagnetic and gravitational fields that might be used to explain the hypothetical extremely high energy release, >1053 erg, suggested by the observations of some gamma-ray bursts in the controversial "energy crisis" problem if and when gamma-ray bursts seem not to show evidence for collimated emission.

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