Cultural advice

The Australian National University acknowledges, celebrates and pays our respects to the Ngunnawal and Ngambri people of the Canberra region and to all First Nations Australians on whose traditional lands we meet and work, and whose cultures are among the oldest continuing cultures in human history.

Aboriginal and Torres Strait Islander peoples are advised that ANU Library collections may include images, names, voices, and other representations of deceased persons.

Material in the collection may contain terms, language or views that reflect the period in which the item was created and may be considered inappropriate today.

A subgrid-scale model for deflagration-to-detonation transitions in Type la supernova explosion simulations Numerical implementation

dc.contributor.authorCiaraldi-Schoolmann, F
dc.contributor.authorSeitenzahl, Ivo
dc.contributor.authorRopke, Friedrich
dc.date.accessioned2018-11-29T22:52:09Z
dc.date.available2018-11-29T22:52:09Z
dc.date.issued2013
dc.date.updated2018-11-29T07:43:58Z
dc.description.abstractDelayed detonations of Chandrasekhar-mass white dwarfs are a promising model for normal Type Ia supernova explosions. In these white dwarfs, the burning starts out as a subsonic deflagration and turns at a later phase of the explosion into a supersonic detonation. The mechanism of the underlying deflagration-to-detonation transition (DDT) is unknown in detail, but necessary conditions have been recently determined. The region of detonation initiation cannot be spatially resolved in multidimensional full-star simulations of the explosion.
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn0004-6361
dc.identifier.urihttp://hdl.handle.net/1885/152093
dc.publisherSpringer
dc.sourceAstronomy and Astrophysics
dc.titleA subgrid-scale model for deflagration-to-detonation transitions in Type la supernova explosion simulations Numerical implementation
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issueA117
local.contributor.affiliationCiaraldi-Schoolmann, F, Max-Planck-Institut für Astrophysik
local.contributor.affiliationSeitenzahl, Ivo, College of Science, ANU
local.contributor.affiliationRopke, Friedrich, Universitat Wurzburg
local.contributor.authoruidSeitenzahl, Ivo, u5472295
local.description.notesImported from ARIES
local.identifier.absfor020100 - ASTRONOMICAL AND SPACE SCIENCES
local.identifier.absseo970102 - Expanding Knowledge in the Physical Sciences
local.identifier.ariespublicationu4571891xPUB64
local.identifier.citationvolume559
local.identifier.doi10.1051/0004-6361/201321480
local.identifier.scopusID2-s2.0-84888362743
local.identifier.thomsonID000327847200117
local.type.statusPublished Version

Downloads

Original bundle

Now showing 1 - 1 of 1
Loading...
Thumbnail Image
Name:
01_Ciaraldi-Schoolmann_A_subgrid-scale_model_for_2013.pdf
Size:
1.1 MB
Format:
Adobe Portable Document Format