Abstract
We summarize a new model that explains the high-energy (photon energies of gigaelectronvolts – GeV) observed in the energetic long-duration gamma-ray bursts (GRBs). The model shows that the gravitomagnetic interaction of a Kerr black hole (BH) with a surrounding magnetic field generates GeV radiation in the vicinity of the BH event horizon extracting the (rotational) energy of the BH.
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Schedule a callMore From: Astronomical and Astrophysical Transactions, Vol. 33, No. 3
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