Nature of the ultrarelativistic prompt emission phase of GRB 190114C
R. Moradi, J. A. Rueda, R. Ruffini, Liang Li, C. L. Bianco, S., Campion, C. Cherubini, S. Filippi, Y. Wang, S. S. Xue

TL;DR
This paper investigates the physical mechanisms behind the ultrarelativistic prompt emission phase of GRB 190114C, proposing a model involving a Kerr black hole, quantum vacuum polarization, and a sequence of plasma pulses that produce observed gamma-ray emissions.
Contribution
It introduces a detailed quantum electrodynamics-based model of the GRB's inner engine, linking quantum vacuum processes to observable gamma-ray emissions and black hole energy extraction.
Findings
Identification of a sequence of blackbody plus cutoff power-law spectra during UPE
Quantitative modeling of the black hole's energy extraction via PEMB pulses
Determination of Lorentz factors, baryon loads, and radii at transparency for each emission sequence
Abstract
We address the physical origin of the ultrarelativistic prompt emission (UPE) phase of GRB 190114C observed in the interval 1.9-3.99 s, by the Fermi-GBM in 10 keV-10 MeV . Thanks to high S/N ratio of Fermi-GBM data, a time resolved spectral analysis has evidenced a sequence of similar blackbody plus cutoff power-law spectra, on ever decreasing time intervals during the entire UPE phase. We assume that during the UPE phase, the inner engine of the GRB, composed of a Kerr black hole and a uniform test magnetic field B0, aligned with the BH rotation axis, operates in an overcritical field. We infer an pair electromagnetic plasma in presence of a baryon load, a PEMB pulse, originating from a vacuum polarization quantum process in the inner engine. This initially optically thick plasma self-accelerates, giving rise at the transparency radius to the MeV radiation observed by…
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