Dynamics and Gravitational Wave Signature of Collapsar Formation

dc.contributor.authorOtt, C. D.
dc.contributor.authorReisswig, C.
dc.contributor.authorSchnetter, E.
dc.contributor.authorO'Connor, E.
dc.contributor.authorSperhake, U.
dc.contributor.authorLoffler, F.
dc.contributor.authorDiener, P.
dc.contributor.authorHawke, I.
dc.contributor.authorBurrows, A.
dc.contributor.authorAbdikamalov, Ernazar
dc.date.accessioned2015-12-21T09:44:43Z
dc.date.available2015-12-21T09:44:43Z
dc.date.issued2010
dc.description.abstractWe perform 3 + 1 general relativistic simulations of rotating core collapse in the context of the collapsar model for long gamma-ray bursts. We employ a realistic progenitor, rotation based on results of stellar evolution calculations, and a simpli ed equation of state. Our simulations track selfconsistently collapse, bounce, the postbounce phase, black hole formation, and the subsequent early hyperaccretion phase. We extract gravitational waves from the spacetime curvature and identify a unique gravitational wave signature associated with the early phase of collapsar formationru_RU
dc.identifier.citationOtt C. D., Reisswig C., Schnetter E., O'Connor E., Sperhake U., Loffler F., Diener P., Hawke I., Burrows A., Abdikamalov Ernazar; 2010; Dynamics and Gravitational Wave Signature of Collapsar Formation; http://arxiv.org/find/all/1/all:+Abdikamalov/0/1/0/all/0/1ru_RU
dc.identifier.urihttp://nur.nu.edu.kz/handle/123456789/916
dc.language.isoenru_RU
dc.subjectResearch Subject Categories::NATURAL SCIENCES::Physicsru_RU
dc.subjectcollapsarru_RU
dc.titleDynamics and Gravitational Wave Signature of Collapsar Formationru_RU
dc.typeArticleru_RU

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