activity
19982020
most citedNeutrino-induced nucleosynthesis of A>64 nuclei: The nu p-process

603 citations · 3.7k across the 28 of their papers we have counts for

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Showing astro-ph.HEShow all

12 papers · 1 filter

astro-ph.HE2020★ 56 cited

Muonization of supernova matter

Tobias Fischer, Gang Guo, Gabriel Martínez-Pinedo +2

The present article investigates the impact of muons on core-collapse supernovae, with particular focus on the early muon neutrino emission. While the presence of muons is well und…

astro-ph.HE2014★ 23 cited

MODA: a new algorithm to compute optical depths in multi-dimensional hydrodynamic simulations

A. Perego, E. Gafton, R. Cabezon +2

We introduce a new algorithm for the calculation of multidimensional optical depths in approximate radiative transport schemes, equally applicable to neutrinos and photons. Motivat…

astro-ph.HE2012★ 89 cited

On the Importance of the Equation of State for the Neutrino-Driven Supernova Explosion Mechanism

Yudai Suwa, Tomoya Takiwaki, Kei Kotake +3

By implementing widely-used equations of state (EOS) from Lattimer & Swesty (LS) and H. Shen et al. (SHEN) in core-collapse supernova simulations, we explore possible impacts of th…

astro-ph.HE2011★ 108 cited

Neutrino spectra evolution during proto-neutron star deleptonization

T. Fischer, G. Martínez-Pinedo, M. Hempel +1

The neutrino-driven wind, which occurs after the onset of a core-collapse supernova explosion, has long been considered as the possible site for the synthesis of heavy r-process el…

astro-ph.HE2011★ 38 cited

Neutrino processes in partially degenerate neutron matter

S. Bacca, K. Hally, M. Liebendörfer +3

We investigate neutrino processes for conditions reached in simulations of core-collapse supernovae. Where neutrino-matter interactions play an important role, matter is partially…

astro-ph.HE2011★ 295 cited

New Equations of State in Simulations of Core-Collapse Supernovae

Matthias Hempel, Tobias Fischer, Jürgen Schaffner-Bielich +1

We discuss three new equations of state (EOS) in core-collapse supernova simulations. The new EOS are based on the nuclear statistical equilibrium model of Hempel and Schaffner-Bie…