97 citations · 246 across the 10 of their papers we have counts for
10 papers
hyperons in core-collapse supernovae: Equilibration and neutrino opacities
Ruben Zatini, Jorge Martin Camalich, Pasquale Dario Serpico +1
Strange hadrons are commonly included in dense-matter equation-of-state models by imposing chemical equilibrium, but the weak-interaction timescales required to establish it in cor…
ESO Expanding Horizon White Paper: Revealing the properties of matter at supranuclear densities with gravitational waves
Tim Dietrich, Tanja Hinderer, Micaela Oertel +40
Understanding dense matter under extreme conditions is one of the most fundamental puzzles in modern physics. Complex interactions give rise to emergent, collective phenomena. Whil…
Occurrence of fast neutrino flavor conversions in QCD phase-transition supernovae
Zewei Xiong, Meng-Ru Wu, Noshad Khosravi Largani +2
Core-collapse supernovae undergoing a first-order quantum chromodynamics (QCD) phase transition experience the collapse of the central proto-neutron star that leads to a second bou…
The Science of the Einstein Telescope
Adrian Abac, Raul Abramo, Simone Albanesi +485
Einstein Telescope (ET) is the European project for a gravitational-wave (GW) observatory of third-generation. In this paper we present a comprehensive discussion of its science ob…
Hyperons during proto-neutron star deleptonization and the emission of dark flavoured particles
Tobias Fischer, Jorge Martin Camalich, Hristijan Kochankovski +1
Complementary to high-energy experimental efforts, indirect astrophysical searches of particles beyond the standard model have long been pursued. The present article follows the la…
Fast neutrino flavor conversions in a supernova: Emergence, evolution, and effects
Zewei Xiong, Meng-Ru Wu, Manu George +4
Fast flavor conversions (FFCs) of neutrinos, which can occur in core-collapse supernovae (CCSNe), are multiangle effects. They depend on the angular distribution of the neutrino's…
Neutron stars in accreting systems -- signatures of the QCD phase transition
Noshad Khosravi Largani, Tobias Fischer, Shota Shibagaki +2
Neutron stars (NS) that are born in binary systems with a main-sequence star companion can experience mass transfer, resulting in the accumulation of material at the surface of the…
Quark matter in high-mass neutron stars?
R. Lastowiecki, D. Blaschke, T. Fischer +1
The recent measurements of the masses of the pulsars PSR J1614-2230 and PSR J0348-0432 provide independent proof for the existence of neutron stars with masses in range of 2 $M_\od…
Supernova neutrinos and nucleosynthesis
G. Martínez-Pinedo, T. Fischer, L. Huther
Observations of metal-poor stars indicate that at least two different nucleosynthesis sites contribute to the production of r-process elements. One site is responsible for the prod…
Large-scale calculations of supernova neutrino-induced reactions in Z=8-82 target nuclei
N. Paar, H. Tutman, T. Marketin +1
Background: In the environment of high neutrino-fluxes provided in core-collapse supernovae or neutron star mergers, neutrino-induced reactions with nuclei contribute to the nucleo…