2024ApJ...977..242K


Query : 2024ApJ...977..242K

2024ApJ...977..242K - Astrophys. J., 977, 242 (2024/December-3)

Leptohadronic Scenarios for TeV Extensions of Gamma-Ray Burst Afterglow Spectra.

KLINGER M., YUAN C., TAYLOR A.M. and WINTER W.

Abstract (from CDS):

Recent multiwavelength observations of gamma-ray burst afterglows observed in the TeV energy range challenge the simplest synchrotron self-Compton (SSC) interpretation of this emission and are consistent with a single power-law component spanning over 8 orders of magnitude in energy. To interpret this generic behavior in the single-zone approximation without adding further free parameters, we perform an exhaustive parameter space study using the public, time-dependent, multimessenger transport software AM3. This description accounts for the radiation from nonthermal protons and the leptohadronic cascade induced by pp and pγ interactions. We summarise the main scenarios that we have found (SSC, Extended-syn, Proton-syn, pp-cascade, and pγ-cascade) and discuss their advantages and limitations. We find that possible high-density environments, as may be typical for surrounding molecular cloud material, offer an alternative explanation for producing flat hard (source) spectra up to and beyond energies of 10 TeV.

Abstract Copyright: © 2024. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Gamma-ray bursts - Non-thermal radiation sources - Astronomical radiation sources - Cosmic rays - X-ray astronomy - Gamma-ray astronomy - Theoretical models - Radiative transfer simulations - Relativistic jets - Shocks - Particle astrophysics

Simbad objects: 5

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Number of rows : 5
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 SN 2019oyw SN* 02 58 10.510 -08 57 27.20           ~ 218 0
2 GRB 190114C gB 03 38 01.18 -26 56 47.8           ~ 343 0
3 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 19090 0
4 SN 2013cq SN* 11 32 32.84 +27 41 56.2           SNIc 613 1
5 GRB 221009A gB 19 13 03.85 +19 46 22.7           ~ 433 0

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