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Stochastic Gravitational Wave Background from Cosmological Supernovae
Alessandra Buonanno, Guenter Sigl, Georg G. Raffelt +2
Based on new developments in the understanding of supernovae (SNe) as gravitational-wave (GW) sources we estimate the GW background from all cosmic SNe. For a broad range of freque…
Nucleosynthesis in the Hot Convective Bubble in Core-Collapse Supernovae
J. Pruet, S. E. Woosley, R. Buras +2
As an explosion develops in the collapsed core of a massive star, neutrino emission drives convection in a hot bubble of radiation, nucleons, and pairs just outside a proto-neutron…
Relativistic outflows from remnants of compact object mergers and their viability for short gamma-ray bursts
M. A. Aloy, H. -T. Janka, E. Mueller
We present the first general relativistic hydrodynamic models of the launch and evolution of relativistic jets and winds, driven by thermal energy deposition, possibly due to neutr…
Neutrino signatures of supernova shock and reverse shock propagation
R. Tomas, M. Kachelriess, G. Raffelt +3
A few seconds after bounce in a core-collapse supernova, the shock wave passes the density region corresponding to resonant neutrino oscillations with the ``atmospheric'' neutrino…
Neutron Star Formation and Birth Properties
Hans-Thomas Janka
Our current knowledge of neutron star formation, progenitors, and natal masses, spins, magnetic fields, and space velocities is briefly reviewed from a theorist's perspective. More…