activity
20062026
most citedCASTRO: A New Compressible Astrophysical Solver. I. Hydrodynamics and Self-Gravity

288 citations · 2.9k across the 60 of their papers we have counts for

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Showing astro-ph.HEShow all

20 papers · 1 filter

astro-ph.HE2016★ 39 cited

White Dwarf Mergers on Adaptive Meshes I. Methodology and Code Verification

Max P. Katz, Michael Zingale, Alan C. Calder +3

The Type Ia supernova progenitor problem is one of the most perplexing and exciting problems in astrophysics, requiring detailed numerical modeling to complement observations of th…

astro-ph.HE2015★ 21 cited

Low Mach Number Modeling of Convection in Helium Shells on Sub-Chandrasekhar White Dwarfs II: Bulk Properties of Simple Models

Adam M. Jacobs, Michael Zingale, Andy Nonaka +2

The dynamics of helium shell convection driven by nuclear burning establish the conditions for runaway in the sub-Chandrasekhar mass, double detonation model for Type Ia supernovae…

astro-ph.HE2014

Comparisons of Two- and Three-Dimensional Convection in Type I X-ray Bursts

M. Zingale, C. M. Malone, A. Nonaka +2

We perform the first detailed three-dimensional simulation of low Mach number convection preceding thermonuclear ignition in a mixed H/He X-ray burst. Our simulations include a mod…

astro-ph.HE2014

Pair-Instability Supernovae of Non-Zero Metallicity Stars

Ke-Jung Chen, Alexander Heger, Stan Woosley +2

Observational evidence suggests that some very massive stars in the local Universe may die as pair-instability supernovae. We present 2D simulations of the pair-instability superno…

astro-ph.HE2014★ 32 cited

Multidimensional Modeling of Type I X-ray Bursts. II. Two-Dimensional Convection in a Mixed H/He Accretor

C. M. Malone, M. Zingale, A. Nonaka +2

Type I X-ray Bursts (XRBs) are thermonuclear explosions of accreted material on the surfaces of a neutron stars in low mass X-ray binaries. Prior to the ignition of a subsonic burn…

astro-ph.HE2014★ 68 cited

Pair Instability Supernovae of Very Massive Population III Stars

Ke-Jung Chen, Alexander Heger, Stan Woosley +2

Numerical studies of primordial star formation suggest that the first stars in the universe may have been very massive. Stellar models indicate that non-rotating Population III sta…