Explosion of fast spinning Sub-Chandrasekhar mass white dwarfs
dc.contributor.author | Cabezón Gómez, Rubén Martín |
dc.contributor.author | García Senz, Domingo |
dc.contributor.other | Universitat Politècnica de Catalunya. Departament de Física |
dc.date.accessioned | 2020-03-20T11:21:42Z |
dc.date.issued | 2018 |
dc.identifier.citation | Cabezón, R.; García Senz, D. Explosion of fast spinning Sub-Chandrasekhar mass white dwarfs. A: Nuclei in the Cosmos-XV. "Proceedings, 15th International Symposium on Nuclei in the Cosmos (NIC-XV): Assergi, Italy, June 24-29, 2018". Springer International Publishing, 2018, p. 347-350. |
dc.identifier.uri | http://hdl.handle.net/2117/180723 |
dc.description.abstract | We study the explosion of rotating sub-Chandrasekhar mass white dwarfs using three-dimensional hydrodynamic simulations. High rotational speeds are assumed in order to significantly distort the initial spherical geometry of the white dwarf. Unlike spherically symmetric models, when He-ignition is located far from the spinning axis the detonation wave trains arrive asynchronously to the antipodes. Models considering different masses of the He-shell, He-ignition locations and rotational velocities are analyzed. We study independently both, the detonation of the He-shell, artificially avoiding carbon-ignition, and the complete detonation of the white dwarf. Our calculations support the viability of the Double Detonation mechanism when the white dwarf is spinning fast. |
dc.format.extent | 4 p. |
dc.language.iso | eng |
dc.publisher | Springer International Publishing |
dc.rights | Attribution-NonCommercial-NoDerivs 3.0 Spain |
dc.rights.uri | http://creativecommons.org/licenses/by-nc-nd/3.0/es/ |
dc.subject | Àrees temàtiques de la UPC::Física::Astronomia i astrofísica |
dc.subject.lcsh | Hydrodynamics |
dc.subject.other | Supernovae |
dc.subject.other | Rotation |
dc.subject.other | Hydrodynamics |
dc.title | Explosion of fast spinning Sub-Chandrasekhar mass white dwarfs |
dc.type | Conference lecture |
dc.subject.lemac | Hidrodinàmica |
dc.subject.lemac | Supernoves |
dc.contributor.group | Universitat Politècnica de Catalunya. GAA - Grup d'Astronomia i Astrofísica |
dc.identifier.doi | 10.1007/978-3-030-13876-9 |
dc.relation.publisherversion | https://link.springer.com/chapter/10.1007/978-3-030-13876-9_62 |
dc.rights.access | Restricted access - publisher's policy |
local.identifier.drac | 25845013 |
dc.description.version | Postprint (published version) |
dc.date.lift | 10000-01-01 |
local.citation.author | Cabezón, R.; García Senz, D. |
local.citation.contributor | Nuclei in the Cosmos-XV |
local.citation.publicationName | Proceedings, 15th International Symposium on Nuclei in the Cosmos (NIC-XV): Assergi, Italy, June 24-29, 2018 |
local.citation.startingPage | 347 |
local.citation.endingPage | 350 |
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