Radiation-mediated shocks in GRB prompt emission

Fuente: arXiv
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Autori principali: Alamaa, Filip, Ryde, Felix, Lundman, Christoffer
Natura: Preprint
Pubblicazione: 2024
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author Alamaa, Filip
Ryde, Felix
Lundman, Christoffer
author_facet Alamaa, Filip
Ryde, Felix
Lundman, Christoffer
contents The debate regarding the emission mechanism in gamma-ray bursts has been long-standing. Here, we study the spectral signatures of photospheric emission, accounting for subphotospheric dissipation by a radiation-mediated shock. The shocks are modeled using the Kompaneets RMS approximation (KRA). We find that the resulting observed spectra are soft, broad, and exhibit an additional break at lower energies. When fitting a collection of 150 mock data samples generated by the model, we obtain a distribution of the low-energy index $α$ that is similar to the observed one. These results are promising and show that dissipative photospheric models can account for many of the observed properties of prompt gamma-ray burst emission.
format Preprint
id arxiv_https___arxiv_org_abs_2403_03529
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Radiation-mediated shocks in GRB prompt emission
Alamaa, Filip
Ryde, Felix
Lundman, Christoffer
High Energy Astrophysical Phenomena
The debate regarding the emission mechanism in gamma-ray bursts has been long-standing. Here, we study the spectral signatures of photospheric emission, accounting for subphotospheric dissipation by a radiation-mediated shock. The shocks are modeled using the Kompaneets RMS approximation (KRA). We find that the resulting observed spectra are soft, broad, and exhibit an additional break at lower energies. When fitting a collection of 150 mock data samples generated by the model, we obtain a distribution of the low-energy index $α$ that is similar to the observed one. These results are promising and show that dissipative photospheric models can account for many of the observed properties of prompt gamma-ray burst emission.
title Radiation-mediated shocks in GRB prompt emission
topic High Energy Astrophysical Phenomena
url https://arxiv.org/abs/2403.03529