Magnetorotational supernovae and jet formation

A magnetorotational mechanism of explosion is at work in core-collapse supernova. The main energy source is the rotational energy of the new born neutron star, and the magnetic field induces the transformation of this energy into the energy of the expanding shock wave. The amount of energy released...

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Detalles Bibliográficos
Autores principales:	Bisnovatyi-Kogan, Gennady S., Moiseenko, Sergey G, Ardelyan, Nikolai
Formato:	Objeto de conferencia
Lenguaje:	Inglés
Publicado:	2015
Materias:	Ciencias Astronómicas supernovae jet formation magnetorotational differential instability
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/167850
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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spelling	I19-R120-10915-1678502024-07-08T20:02:25Z http://sedici.unlp.edu.ar/handle/10915/167850 Magnetorotational supernovae and jet formation Bisnovatyi-Kogan, Gennady S. Moiseenko, Sergey G Ardelyan, Nikolai 2015-10 2016 2024-07-08T14:26:17Z en Ciencias Astronómicas supernovae jet formation magnetorotational differential instability A magnetorotational mechanism of explosion is at work in core-collapse supernova. The main energy source is the rotational energy of the new born neutron star, and the magnetic field induces the transformation of this energy into the energy of the expanding shock wave. The amount of energy released by this mechanism is enough to explain the observations. The development of the magnetorotational differential instability is studied. A jet is formed at a dipole-like magnetic field configuration. Facultad de Ciencias Astronómicas y Geofísicas Objeto de conferencia Objeto de conferencia http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) application/pdf 31-36
institution	Universidad Nacional de La Plata
institution_str	I-19
repository_str	R-120
collection	SEDICI (UNLP)
language	Inglés
topic	Ciencias Astronómicas supernovae jet formation magnetorotational differential instability
spellingShingle	Ciencias Astronómicas supernovae jet formation magnetorotational differential instability Bisnovatyi-Kogan, Gennady S. Moiseenko, Sergey G Ardelyan, Nikolai Magnetorotational supernovae and jet formation
topic_facet	Ciencias Astronómicas supernovae jet formation magnetorotational differential instability
description	A magnetorotational mechanism of explosion is at work in core-collapse supernova. The main energy source is the rotational energy of the new born neutron star, and the magnetic field induces the transformation of this energy into the energy of the expanding shock wave. The amount of energy released by this mechanism is enough to explain the observations. The development of the magnetorotational differential instability is studied. A jet is formed at a dipole-like magnetic field configuration.
format	Objeto de conferencia Objeto de conferencia
author	Bisnovatyi-Kogan, Gennady S. Moiseenko, Sergey G Ardelyan, Nikolai
author_facet	Bisnovatyi-Kogan, Gennady S. Moiseenko, Sergey G Ardelyan, Nikolai
author_sort	Bisnovatyi-Kogan, Gennady S.
title	Magnetorotational supernovae and jet formation
title_short	Magnetorotational supernovae and jet formation
title_full	Magnetorotational supernovae and jet formation
title_fullStr	Magnetorotational supernovae and jet formation
title_full_unstemmed	Magnetorotational supernovae and jet formation
title_sort	magnetorotational supernovae and jet formation
publishDate	2015
url	http://sedici.unlp.edu.ar/handle/10915/167850
work_keys_str_mv	AT bisnovatyikogangennadys magnetorotationalsupernovaeandjetformation AT moiseenkosergeyg magnetorotationalsupernovaeandjetformation AT ardelyannikolai magnetorotationalsupernovaeandjetformation
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Magnetorotational supernovae and jet formation

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