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Advanced burning stages and fate of 8-10 Mo stars
Samuel Jones, Raphael Hirschi, Ken'ichi Nomoto +9
The stellar mass range 8<M/Mo<12 corresponds to the most massive AGB stars and the most numerous massive stars. It is host to a variety of supernova progenitors and is therefore ve…
Core-collapse supernova equations of state based on neutron star observations
Andrew W. Steiner, Matthias Hempel, Tobias Fischer
Many of the currently available equations of state for core-collapse supernova simulations give large neutron star radii and do not provide large enough neutron star masses, both o…
Probing the neutrino mass hierarchy with the rise time of a supernova burst
Pasquale Dario Serpico, Sovan Chakraborty, Tobias Fischer +3
The rise time of a Galactic supernova (SN) bar-nue lightcurve, observable at a high-statistics experiment such as the IceCube Cherenkov detector, can provide a diagnostic tool for…
Effect of collective neutrino flavor oscillations on vp-process nucleosynthesis
G. Martínez-Pinedo, B. Ziebarth, T. Fischer +1
The vp process is a primary nucleosynthesis process which occurs in core collapse supernovae. An essential role in this process is being played by electron antineutrinos. They gene…
Exploring the QCD phase transition in core collapse supernova simulations in spherical symmetry
T. Fischer, I. Sagert, M. Hempel +5
For finite chemical potential effective models of QCD predict a first order phase transition. In favour for the search of such a phase transition in nature, we construct an equatio…
Astrophysical Implications of the QCD phase transition
Jurgen Schaffner-Bielich, Irina Sagert, Matthias Hempel +5
The possible role of a first order QCD phase transition at nonvanishing quark chemical potential and temperature for cold neutron stars and for supernovae is delineated. For cold n…