activity
20042019
most citedEquations of state for supernovae and compact stars

1.2k citations · 5.7k across the 55 of their papers we have counts for

collaborators

57 papers

astro-ph.SR2019★ 62 cited

PUSHing core-collapse supernovae to explosions in spherical symmetry IV: Explodability, remnant properties and nucleosynthesis yields of low metallicity stars

Kevin Ebinger, Sanjana Curtis, Somdutta Ghosh +5

In this fourth paper of the series, we use the parametrized, spherically symmetric explosion method PUSH to perform a systematic study of two sets of non-rotating stellar progenito…

nucl-th2018★ 13 cited

Asymmetric Nuclear Light Clusters In Supernova Matter

Andrey Yudin, Matthias Hempel, Sergei Blinnikov +2

We explore the appearance of light clusters at high densities of collapsing stellar cores. Special attention is paid to the unstable isotope H4, which was not included in previous…

astro-ph.SR2018★ 117 cited

PUSHing Core-Collapse Supernovae to Explosions in Spherical Symmetry III: Nucleosynthesis Yields

Sanjana Curtis, Kevin Ebinger, Carla Fröhlich +4

In a previously presented proof-of-principle study, we established a parametrized spherically symmetric explosion method (PUSH) that can reproduce many features of core-collapse su…

astro-ph.SR2018★ 89 cited

PUSHing Core-Collapse Supernovae to Explosions in Spherical Symmetry II: Explodability and Global Properties

Kevin Ebinger, Sanjana Curtis, Carla Fröhlich +4

In a previously presented proof-of-principle study we established a parametrized spherically symmetric explosion method (PUSH) that can reproduce many features of core-collapse sup…

astro-ph.HE2017★ 44 cited

The state of matter in simulations of core-collapse supernovae -- Reflections and recent developments

Tobias Fischer, Niels-Uwe Bastian, David Blaschke +7

In this review article we discuss selected developments regarding the role of the equation of state (EOS) in simulations of core-collapse supernovae. There are no first-principle c…

astro-ph.SR2017★ 49 cited

Nucleosynthesis in 2D Core-Collapse Supernovae of 11.2 and 17.0 M Progenitors: Implications for Mo and Ru Production

M. Eichler, K. Nakamura, T. Takiwaki +6

Core-collapse supernovae are the first polluters of heavy elements in the galactic history. As such, it is important to study the nuclear compositions of their ejecta, and understa…