most citedi-process nucleosynthesis and mass retention efficiency in He-shell flash evolution of rapidly accreting white dwarfs

115 citations · 271 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2016115 cited

i-process nucleosynthesis and mass retention efficiency in He-shell flash evolution of rapidly accreting white dwarfs

Pavel Denissenkov, Falk Herwig, Umberto Battino +4

Based on stellar evolution simulations, we demonstrate that rapidly accreting white dwarfs in close binary systems are an astrophysical site for the intermediate neutron-capture pr…

astro-ph.SR20141 cited

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…

astro-ph.SR201466 cited

The primordial and evolutionary abundance variations in globular-cluster stars: a problem with two unknowns

Pavel Denissenkov, Don VandenBerg, David Hartwick +3

We demonstrate that among the potential sources of the primordial abundance variations of the proton-capture elements in globular-cluster stars proposed so far, such as the hot-bot…

astro-ph.CO201426 cited

Dark Stars: Improved Models and First Pulsation Results

Tanja Rindler-Daller, Michael H. Montgomery, Katherine Freese +2

We use the stellar evolution code MESA to study dark stars. Dark stars (DSs), which are powered by dark matter (DM) self-annihilation rather than by nuclear fusion, may be the firs…

astro-ph.SR201463 cited

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…