295 citations · 403 across the 2 of their papers we have counts for
4 papers
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…
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…
Strange quark matter in explosive astrophysical systems
I. Sagert, T. Fischer, M. Hempel +4
Explosive astrophysical systems, such as supernovae or compact star binary mergers, provide conditions where strange quark matter can appear. The high degree of isospin asymmetry a…
Protoneutron star evolution and the neutrino driven wind in general relativistic neutrino radiation hydrodynamics simulations
T. Fischer, S. C. Whitehouse, A. Mezzacappa +2
Massive stars end their life in an explosion event with kinetic energies of the order 1 Bethe. Immediately after the explosion has been launched, a region of low density and high e…