145 citations · 1.4k across the 35 of their papers we have counts for
34 papers
Ignition of detonation in accreted helium
Ami Glasner, Eli Livne, Elad Steinberg +2
Sub-Chandrasekhar CO white dwarfs accreting helium have been considered as candidates for Type Ia supernova(SNIa) progenitors since the early 1980s (helium shell mass $> 0.1 M_\odo…
Hybrid C-O-Ne White Dwarfs as Progenitors of Diverse SNe Ia
Pavel Denissenkov, James Truran, Falk Herwig +5
When carbon is ignited off-center in a CO core of a super-AGB star, its burning in a convective shell tends to propagate to the center. Whether the C flame will actually be able to…
Hybrid C-O-Ne white dwarfs as progenitors of type Ia supernovae: dependence on Urca process and mixing assumptions
P. Denissenkov, J. W. Truran, F. Herwig +5
When carbon is ignited off-centre in a CO core of a super-AGB star, its burning in a convective shell tends to propagate to the centre. Whether the C flame will actually be able to…
The Effect of the Pre-Detonation Stellar Internal Velocity Profile on the Nucleosynthetic Yields in Type Ia Supernova
Yeunjin Kim, G. C. Jordan, Carlo Graziani +3
A common model of the explosion mechanism of Type Ia supernovae is based on a delayed detonation of a white dwarf. A variety of models differ primarily in the method by which the d…
The C-flame Quenching by Convective Boundary Mixing in Super-AGB Stars and the Formation of Hybrid C/O/Ne White Dwarfs and SN Progenitors
Pavel A. Denissenkov, Falk Herwig, James W. Truran +1
After off-center C ignition in the cores of super-AGB stars the C flame propagates all the way down to the center, trailing behind it the C-shell convective zone, and thus building…
MESA and NuGrid Simulations of Classical Nova Outbursts and Nucleosynthesis
Pavel Denissenkov, Falk Herwig, Marco Pignatari +1
Classical novae are the results of surface thermonuclear explosions of hydrogen accreted by white dwarfs (WDs) from their low-mass main-sequence or red-giant binary companions. Che…