Magnetorotational supernovae and jet formation

Autores
Bisnovatyi-Kogan, Gennady S.; Moiseenko, Sergey G; Ardelyan, Nikolai
Año de publicación
2015
Idioma
inglés
Tipo de recurso
documento de conferencia
Estado
versión publicada
Descripción
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
Materia
Ciencias Astronómicas
supernovae
jet formation
magnetorotational differential instability
Nivel de accesibilidad
acceso abierto
Condiciones de uso
http://creativecommons.org/licenses/by-nc-sa/4.0/
Repositorio
SEDICI (UNLP)
Institución
Universidad Nacional de La Plata
OAI Identificador
oai:sedici.unlp.edu.ar:10915/167850
Acceder
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oai_identifier_str oai:sedici.unlp.edu.ar:10915/167850
network_acronym_str SEDICI
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network_name_str SEDICI (UNLP)
spelling Magnetorotational supernovae and jet formationBisnovatyi-Kogan, Gennady S.Moiseenko, Sergey GArdelyan, NikolaiCiencias Astronómicassupernovaejet formationmagnetorotational differential instabilityA 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 Geofísicas2015-10info:eu-repo/semantics/conferenceObjectinfo:eu-repo/semantics/publishedVersionObjeto de conferenciahttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdf31-36http://sedici.unlp.edu.ar/handle/10915/167850enginfo:eu-repo/semantics/altIdentifier/isbn/978-987-24948-3-4info:eu-repo/semantics/reference/url/https://sedici.unlp.edu.ar/handle/10915/167830info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2026-05-27T11:38:51Zoai:sedici.unlp.edu.ar:10915/167850Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292026-05-27 11:38:52.068SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv Magnetorotational supernovae and jet formation
title Magnetorotational supernovae and jet formation
spellingShingle Magnetorotational supernovae and jet formation
Bisnovatyi-Kogan, Gennady S.
Ciencias Astronómicas
supernovae
jet formation
magnetorotational differential instability
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
dc.creator.none.fl_str_mv Bisnovatyi-Kogan, Gennady S.
Moiseenko, Sergey G
Ardelyan, Nikolai
author Bisnovatyi-Kogan, Gennady S.
author_facet Bisnovatyi-Kogan, Gennady S.
Moiseenko, Sergey G
Ardelyan, Nikolai
author_role author
author2 Moiseenko, Sergey G
Ardelyan, Nikolai
author2_role author
author
dc.subject.none.fl_str_mv Ciencias Astronómicas
supernovae
jet formation
magnetorotational differential instability
topic Ciencias Astronómicas
supernovae
jet formation
magnetorotational differential instability
dc.description.none.fl_txt_mv 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
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.
publishDate 2015
dc.date.none.fl_str_mv 2015-10
dc.type.none.fl_str_mv info:eu-repo/semantics/conferenceObject
info:eu-repo/semantics/publishedVersion
Objeto de conferencia
http://purl.org/coar/resource_type/c_5794
info:ar-repo/semantics/documentoDeConferencia
format conferenceObject
status_str publishedVersion
dc.identifier.none.fl_str_mv http://sedici.unlp.edu.ar/handle/10915/167850
url http://sedici.unlp.edu.ar/handle/10915/167850
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/isbn/978-987-24948-3-4
info:eu-repo/semantics/reference/url/https://sedici.unlp.edu.ar/handle/10915/167830
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
http://creativecommons.org/licenses/by-nc-sa/4.0/
Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
eu_rights_str_mv openAccess
rights_invalid_str_mv http://creativecommons.org/licenses/by-nc-sa/4.0/
Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
dc.format.none.fl_str_mv application/pdf
31-36
dc.source.none.fl_str_mv reponame:SEDICI (UNLP)
instname:Universidad Nacional de La Plata
instacron:UNLP
reponame_str SEDICI (UNLP)
collection SEDICI (UNLP)
instname_str Universidad Nacional de La Plata
instacron_str UNLP
institution UNLP
repository.name.fl_str_mv SEDICI (UNLP) - Universidad Nacional de La Plata
repository.mail.fl_str_mv alira@sedici.unlp.edu.ar
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score 13.468372

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