Relativistic MHD simulations of merging and collapsing stars and effects on GRB transient

Fuente: arXiv
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Auteurs principaux: Janiuk, Agnieszka, Urrutia, Gerardo, Saji, Joseph, Plonka, Piotr
Format: Preprint
Publié: 2025
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author Janiuk, Agnieszka
Urrutia, Gerardo
Saji, Joseph
Plonka, Piotr
author_facet Janiuk, Agnieszka
Urrutia, Gerardo
Saji, Joseph
Plonka, Piotr
contents Compact binary mergers and the collapse of massive stars can produce intense transients observable across high-energy wavelengths. Events such as gamma-ray bursts and kilonova emissions are often accompanied by gravitational wave detections, making them crucial sources for multimessenger astrophysics. To explore these phenomena theoretically, state-of-the-art approaches of General Relativistic magnetohydrodynamic simulations are used. We present recent findings from our simulations, and discuss observational consequences of the stellar/post-merger environment on the gamma ray burst prompt emission properties.
format Preprint
id arxiv_https___arxiv_org_abs_2512_08489
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Relativistic MHD simulations of merging and collapsing stars and effects on GRB transient
Janiuk, Agnieszka
Urrutia, Gerardo
Saji, Joseph
Plonka, Piotr
High Energy Astrophysical Phenomena
Compact binary mergers and the collapse of massive stars can produce intense transients observable across high-energy wavelengths. Events such as gamma-ray bursts and kilonova emissions are often accompanied by gravitational wave detections, making them crucial sources for multimessenger astrophysics. To explore these phenomena theoretically, state-of-the-art approaches of General Relativistic magnetohydrodynamic simulations are used. We present recent findings from our simulations, and discuss observational consequences of the stellar/post-merger environment on the gamma ray burst prompt emission properties.
title Relativistic MHD simulations of merging and collapsing stars and effects on GRB transient
topic High Energy Astrophysical Phenomena
url https://arxiv.org/abs/2512.08489