Détail du document
Identifiant
oai:arXiv.org:2403.14996
Sujet
Astrophysics - High Energy Astroph...Auteur
Janiuk, Agnieszka Saji, Joseph Urrutia, GerardoCatégorie
sciences : astrophysique
Année
2024
Date de référencement
27/03/2024
Mots clés
binary mergers neutron kilonovaRésumé
Compact binary mergers are sources of gravitational waves, and can be accompanied by electromagnetic signals.
We discuss the possible features in the kilonova emissions which may help distinguish the black hole - neutron star mergers from the binary neutron stars.
In addition, the amount of ejected material may depend on whether the system undergoes the creation of a transient hyper-massive, differentially rotating neutron star.
In this context, the numerical simulations of post-merger systems and their outflows are important for our understanding of the nature of short GRB progenitor systems.
In this article, we present a suite of GR MHD simulations performed by the CTP PAS astrophysics group, to model the neutrino driven disk winds and their contribution to the kilonova emissions.
The contribution of the disk wind to the jet collimation and variability is also briefly discussed.
;Comment: 6 pages; submitted to the Proceedings of the Polish Astronomical Society Meeting 2023
Janiuk, Agnieszka,Saji, Joseph,Urrutia, Gerardo, 2024, What we can learn about compact binary mergers from their kilonova signals?
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