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dc.contributor.authorBlanco Iglesias, José Miguel
dc.contributor.authorGarcía Senz, Domingo
dc.contributor.authorCabezón Gómez, Rubén Martín
dc.contributor.otherUniversitat Politècnica de Catalunya. Doctorat en Física Computacional i Aplicada
dc.contributor.otherUniversitat Politècnica de Catalunya. Departament de Física
dc.date.accessioned2020-02-11T12:52:59Z
dc.date.available2020-02-11T12:52:59Z
dc.date.issued2019
dc.identifier.citationBlanco, J.; García Senz, D.; Cabezón, R. Building initial models of rotating white dwarfs with SPH. A: SPHERIC 2019. "Proceedings of the 14th SPHERIC International Workshop". 2019, p. 243-248.
dc.identifier.isbn978-0-902746-44-2
dc.identifier.urihttp://hdl.handle.net/2117/177437
dc.description.abstractA general procedure to build self-gravitational, rotating equilibrium structures with the Smoothed Particle Hydrodynamics (SPH) technique does not exist. In particular, obtaining stable rotating configurations for white dwarf (WD) stars is currently a major drawback of many astrophysical simulations. Rotating WDs with low internal temperatures are connected with both, explosive and implosive scenarios such as type Ia supernova explosions or neutron stars formation. Simulations of these events with SPH codes demand stable enough particle configurations as initial models. In this work we have developed and tested a relaxation method to obtain equilibrium configurations of rotating WDs. This method is straightforward and takes advantage of the excellent mass and angular momentum conservation properties of the SPH technique. Although we focus on rigid rotation and its potential applications to several Type Ia supernova scenarios, we also show that our proposal is also able to provide good initial models in differential rotation, which has the potential to benefit many other types of simulations where rotation plays a capital role, like disk evolution and stellar formation.
dc.format.extent6 p.
dc.language.isoeng
dc.rightsAttribution-NonCommercial-NoDerivs 3.0 Spain
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/es/
dc.subjectÀrees temàtiques de la UPC::Física
dc.subject.lcshHydrodynamics
dc.titleBuilding initial models of rotating white dwarfs with SPH
dc.typeConference lecture
dc.subject.lemacHidrodinàmica
dc.contributor.groupUniversitat Politècnica de Catalunya. GAA - Grup d'Astronomia i Astrofísica
dc.description.peerreviewedPeer Reviewed
dc.rights.accessOpen Access
local.identifier.drac25848439
dc.description.versionPostprint (published version)
local.citation.authorBlanco, J.; García Senz, D.; Cabezón, R.
local.citation.contributorSPHERIC 2019
local.citation.publicationNameProceedings of the 14th SPHERIC International Workshop
local.citation.startingPage243
local.citation.endingPage248


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Attribution-NonCommercial-NoDerivs 3.0 Spain
Except where otherwise noted, content on this work is licensed under a Creative Commons license : Attribution-NonCommercial-NoDerivs 3.0 Spain