2026-09-20T01:50:55Zhttps://iris.unitn.it/oai/requestoai:iris.unitn.it:11572/3681662026-04-03T00:47:59Zcom_11572_237821com_11572_101871col_11572_237822ou_ou00011
General relativistic magnetohydrodynamic simulations of binary neutron star mergers
Kawamura, Takumu
Kawamura, Takumu
Giacomazzo, Bruno
Settore FIS/02 - Fisica Teorica, Modelli e Metodi Matematici
In this thesis I present results of my fully general relativistic magnetohydrodynamic (GRMHD) binary neutron star merger (BNS) simulations, conducted by using the numerical code "Whisky" under various conditions, such as, different Equation of State (EOS) for neutron matter (APR4, Ideal fluid and H4 EOSs), masses (with equal/unequal masses for two neutron stars), different magnetic field configurations (both fields of two neutron stars aligned with the inspiral axis, one aligned and one anti-aligned, and both anti-aligned) to investigate the effect of these parameters on the dynamics of the simulations and possibility of forming relativistic jets, which is thought to be one of the necessary conditions for the central engine of short gamma-ray bursts (SGRBs).
2017
info:eu-repo/semantics/doctoralThesis
https://hdl.handle.net/11572/368166
http://dx.doi.org/10.15168/11572_368166
10.15168/11572_368166
eng
firstpage:1
lastpage:81
numberofpages:81
info:eu-repo/semantics/openAccess
Università degli studi di Trento
place:TRENTO
license:Tutti i diritti riservati (All rights reserved)
license:Tutti i diritti riservati (All rights reserved)
license uri:iris.PRI01