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20002026
most citedThree-dimensional delayed-detonation models with nucleosynthesis for Type Ia supernovae

547 citations · 7.4k across the 72 of their papers we have counts for

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Showing 2013Show all

11 papers · 1 filter

astro-ph.HE2013★ 78 cited

SN 2010lp---a Type Ia supernova from a violent merger of two carbon--oxygen White Dwarfs

M. Kromer, R. Pakmor, S. Taubenberger +6

SN 2010lp is a subluminous Type Ia supernova (SN Ia) with slowly-evolving lightcurves. Moreover, it is the only subluminous SN Ia observed so far that shows narrow emission lines o…

astro-ph.SR2013★ 40 cited

Predicting the amount of hydrogen stripped by the supernova explosion for SN 2002cx-like SNe Ia

Zheng-Wei Liu, M. Kromer, M. Fink +5

The most favored progenitor scenarios for Type Ia supernovae (SNe Ia) involve the single-degenerate (SD) scenario and the double-degenerate scenario. The absence of stripped hydrog…

astro-ph.SR2013★ 142 cited

Solar abundance of manganese: a case for the existence of near Chandrasekhar-mass Type Ia supernova progenitors

Ivo R. Seitenzahl, Gabriele Cescutti, Friedrich K. Roepke +2

Context: Manganese is predominantly synthesised in Type Ia supernova (SN Ia) explosions. Owing to the entropy dependence of the Mn yield in explosive thermonuclear burning, SNe Ia…

astro-ph.CO2013★ 18 cited

Cosmological Parameter Estimation from SN Ia data: a Model-Independent Approach

S. Benitez-Herrera, E. E. O. Ishida, M. Maturi +4

We perform a model independent reconstruction of the cosmic expansion rate based on type Ia supernova data. Using the Union 2.1 data set, we show that the Hubble parameter behaviou…

astro-ph.HE2013★ 116 cited

Synthetic light curves and spectra for three-dimensional delayed-detonation models of Type Ia supernovae

S. A. Sim, I. R. Seitenzahl, M. Kromer +7

In a companion paper, Seitenzahl et al. (2013) presented a set of three-dimensional delayed detonation models for thermonuclear explosions of near-Chandrasekhar mass white dwarfs (…

astro-ph.SR2013★ 290 cited

Three-dimensional pure deflagration models with nucleosynthesis and synthetic observables for Type Ia supernovae

M. Fink, M. Kromer, I. R. Seitenzahl +6

We investigate whether pure deflagration models of Chandrasekhar-mass carbon-oxygen white dwarf stars can account for one or more subclass of the observed population of Type Ia sup…

astro-ph.SR2013★ 31 cited

A Subgrid-scale Model for Deflagration-to-Detonation Transitions in Type Ia Supernova Explosion Simulations - Numerical implementation

F. Ciaraldi-Schoolmann, I. R. Seitenzahl, F. K. Roepke

A promising model for normal Type Ia supernova (SN Ia) explosions are delayed detonations of Chandrasekhar-mass white dwarfs, in which the burning starts out as a subsonic deflagra…

astro-ph.SR2013★ 89 cited

The impact of Type Ia supernova explosions on helium companions in the Chandrasekhar-mass explosion scenario

Zheng-Wei Liu, Ruediger Pakmor, Ivo Seitenzahl +8

In the version of the SD scenario of SNe Ia studied here, a CO WD explodes close to the Chandrasekhar limit after accreting material from a non-degenerate He companion. In the pres…

astro-ph.SR2013★ 45 cited

The Effects of Variations in Nuclear Interactions on Nucleosynthesis in Thermonuclear Supernovae

Anuj Parikh, Jordi Jose, Ivo R. Seitenzahl +1

The impact of nuclear physics uncertainties on nucleosynthesis in thermonuclear supernovae has not been fully explored using comprehensive and systematic studies with multiple mode…

astro-ph.HE2013★ 74 cited

Combustion of a neutron star into a strange quark star: The neutrino signal

G. Pagliara, M. Herzog, F. K. Roepke

There are strong indications that the process of conversion of a neutron star into a strange quark star proceeds as a strong deflagration implying that in a few milliseconds almost…

astro-ph.SR2013★ 34 cited

Gamma-ray diagnostics of Type Ia supernovae: Predictions of observables from three-dimensional modeling

A. Summa, A. Ulyanov, M. Kromer +11

Besides the fact that the gamma-ray emission due to radioactive decays is responsible for powering the light curves of Type Ia supernovae (SNe Ia), gamma rays themselves are of par…