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Imprints of neutrino-pair flavor conversions on nucleosynthesis in ejecta from neutron-star merger remnants
Meng-Ru Wu, Irene Tamborra, Oliver Just +1
The remnant of neutron star mergers is dense in neutrinos. By employing inputs from one hydrodynamical simulation of a binary neutron star merger remnant with a black hole of $3\ M…
Neutron-star radius constraints from GW170817 and future detections
Andreas Bauswein, Oliver Just, Hans-Thomas Janka +1
We introduce a new, powerful method to constrain properties of neutron stars (NSs). We show that the total mass of GW170817 provides a reliable constraint on the stellar radius if…
Intermediate-Mass-Elements in Young Supernova Remnants Reveal Neutron Star Kicks by Asymmetric Explosions
Satoru Katsuda, Mikio Morii, Hans-Thomas Janka +9
The birth properties of neutron stars yield important information on the still debated physical processes that trigger the explosion and on intrinsic neutron-star physics. These pr…
Bridging the Gap: From Massive Stars to Supernovae
Justyn R. Maund, Paul A. Crowther, Hans-Thomas Janka +1
Almost since the beginning, massive stars and their resultant supernovae have played a crucial role in the Universe. These objects produce tremendous amounts of energy and new, hea…
Diffuse Supernova Neutrino Background from extensive core-collapse simulations of - progenitors
Shunsaku Horiuchi, Kohsuke Sumiyoshi, Ko Nakamura +5
We revisit the diffuse supernova neutrino background in light of recent systematic studies of stellar core collapse that reveal the quantitative impacts of the progenitor condition…
Rotation-supported Neutrino-driven Supernova Explosions in Three Dimensions and the Critical Luminosity Condition
A. Summa, H. -Th. Janka, T. Melson +1
We present the first self-consistent, three-dimensional (3D) core-collapse supernova simulations performed with the Prometheus-Vertex code for a rotating progenitor star. Besides u…