Radiative transfer and type Ia supernovae spectra analysis in the context of supernovae factory.

dc.contributor.advisorBaron, Edward,en_US
dc.contributor.authorBongard, Sebastien.en_US
dc.date.accessioned2013-08-16T12:19:53Z
dc.date.available2013-08-16T12:19:53Z
dc.date.issued2005en_US
dc.description.abstractWe showed the spectrum formation in SNeIa around maximum light to be a multi-layered process involving regions from 5000 km per s to 20000 km per s, interacting not only through scattering but also through pure emission. This new understanding allowed us to introduce a new spectral indicators we called RSiSu, which can be used to measure SNeIa blue magnitudes with a precision comparable to the stretch factor. This makes it possible to independently constraint the evolutionary effect on SNeIa that are of crucial importance for high z surveys.en_US
dc.description.abstractWe used the multi-purpose radiative transfer code phoenix, developed by P. Hauschildt, F. Allard and E. Baron to produce a grid of synthetic spectra sampling dates from 10 to 25 days after explosion and bolometric magnitudes from -18.0 to -19.7. We also developed an adaptive grid scheme in order to stabilize phoenix convergence.en_US
dc.description.abstractThis co-supervised dissertation was conducted in collaboration between The University of Oklahoma City (USA) and University Claude Bernard of Lyon (France). It addresses the radiative transfer issue in type Ia supernovae expanding envelopes, in the context of the SupernovaFactory.en_US
dc.format.extentxiii, 121 leaves :en_US
dc.identifier.urihttp://hdl.handle.net/11244/900
dc.noteAdviser: Edward Baron.en_US
dc.noteSource: Dissertation Abstracts International, Volume: 66-05, Section: B, page: 2630.en_US
dc.subjectLuminosity distance.en_US
dc.subjectSupernovae Spectra.en_US
dc.subjectPhysics, Astronomy and Astrophysics.en_US
dc.thesis.degreePh.D.en_US
dc.thesis.degreeDisciplineHomer L. Dodge Department of Physics and Astronomyen_US
dc.titleRadiative transfer and type Ia supernovae spectra analysis in the context of supernovae factory.en_US
dc.typeThesisen_US
ou.groupCollege of Arts and Sciences::Homer L. Dodge Department of Physics and Astronomy
ou.identifier(UMI)AAI3175350en_US

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