On the GeV Emission of the Type I BdHN GRB 130427A
We propose that the inner engine of a type I binary-driven hypernova (BdHN) is composed of Kerr black hole (BH) in a non-stationary state, embedded in a uniform magnetic field B_0 aligned with the BH rotation axis and surrounded by an ionized plasma of extremely low density of 10^−14 g cm−3. Using GRB 130427A as a prototype, we show that this inner engine acts in a sequence of elementary impulses. Electrons accelerate to ultrarelativistic energy near the BH horizon, propagating along the polar axis, θ = 0, where they can reach energies of ~10^18 eV, partially contributing to ultrahigh-energy cosmic rays. When propagating with $\theta \ne 0$ through the magnetic field B_0, they produce GeV and TeV radiation through synchroton emission. The mass of BH, M = 2.31M ⊙, its spin, α = 0.47, and the value of magnetic field B_0 = 3.48 × 10^10 G, are determined self consistently to fulfill the energetic and the transparency requirement. The repetition time of each elementary impulse of energy ${ \mathcal E }\sim {10}^{37}$ erg is ~10^−14 s at the beginning of the process, then slowly increases with time evolution. In principle, this "inner engine" can operate in a gamma-ray burst (GRB) for thousands of years. By scaling the BH mass and the magnetic field, the same inner engine can describe active galactic nuclei.
2019
2020-07-15 15:00:11
1033
black hole physics, binaries, gamma-ray burst, neutron stars, supernovae, Astrophysics - High Energy Astrophysical Phenomena
r6
Remo
Ruffini
70
Rahim
Moradi
70
Jorge Armando
Rueda
70
Carlo Luciano
Bianco
70
Christian
Cherubini
70
Simonetta
Filippi
70
Yen-Chen
Chen
70
Mile
Karlica
70
Narek
Sahakyan
70
Yu
Wang
70
She Sheng
Xue
70
Laura
Beccera
70
COBISS_ID
3
23009283
DOI
15
https://doi.org/10.3847/1538-4357/ab4ce6
NUK URN
18
URN:SI:UNG:REP:BXWOORI6
Ruffini_2019_ApJ_886_82.pdf
1141168
Predstavitvena datoteka
2020-07-15 15:00:31