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20042026
most citedPUSHing Core-Collapse Supernovae to Explosions in Spherical Symmetry III: Nucleosynthesis Yields

117 citations · 464 across the 17 of their papers we have counts for

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Showing astro-ph.HEShow all

8 papers · 1 filter

astro-ph.HE2026

Core-Collapse Supernovae from Single and Binary-Stripped Massive Stars - I. Explodability and Nucleosynthesis

J. M. Pollin, S. Curtis, C. Fröhlich +6

Binary interaction can substantially alter massive-star evolution and pre-supernova structure, changing core-collapse outcomes and nucleosynthetic yields. We compare explodability…

astro-ph.HE2025★ 1 cited

Turbulence in Core-Collapse Supernovae

David Calvert, Michael Redle, Bibek Gautam +4

It is understood in a general sense that turbulent fluid motion below the shock front in a core-collapse supernova stiffens the effective equation of state of the fluid and aids in…

astro-ph.HE2021★ 8 cited

A New Constraint on the Nuclear Equation of State from Statistical Distributions of Compact Remnants of Supernovae

Mikhail M. Meskhi, Noah E. Wolfe, Zhenyu Dai +4

Understanding how matter behaves at the highest densities and temperatures is a major open problem in both nuclear physics and relativistic astrophysics. This physics is often enca…

astro-ph.HE2019★ 3 cited

Impact of Uncertainties in Astrophysical Reaction Rates on Nucleosynthesis in the Process

T. Rauscher, N. Nishimura, G. Cescutti +3

The process appears in proton-rich, hot matter which is expanding in a neutrino wind and may be realised in explosive environments such as core-collapse supernovae or in outfl…

astro-ph.HE2019★ 5 cited

Catching Element Formation In The Act

Chris L. Fryer, Frank Timmes, Aimee L. Hungerford +216

Gamma-ray astronomy explores the most energetic photons in nature to address some of the most pressing puzzles in contemporary astrophysics. It encompasses a wide range of objects…

astro-ph.HE2017★ 10 cited

The Neutrino Signal From Pair Instability Supernovae

Warren P. Wright, Matthew S. Gilmer, Carla Fröhlich +1

A very massive star with a carbon-oxygen core in the range of M M is expected to undergo a very different kind of explosion known as a…

astro-ph.HE2016★ 4 cited

Explosion Dynamics of Parametrized Spherically Symmetric Core-Collapse Supernova Simulations

Kevin Ebinger, Sanjana Sinha, Carla Fröhlich +6

We report on a method, PUSH, for triggering core-collapse supernova (CCSN) explosions of massive stars in spherical symmetry. This method provides a framework to study many importa…

astro-ph.HE2011★ 24 cited

Nucleosynthesis in core-collapse supernova explosions triggered by a quark-hadron phase transition

Nobuya Nishimura, Tobias Fischer, Friedrich-Karl Thielemann +7

We explore heavy element nucleosynthesis in the explosion of massive stars which are triggered by a quark-hadron phase transition during the early post bounce phase of core-collaps…