The production of about half of the heavy elements found in nature is assigned to a specific
astrophysical nucleosynthesis process: the rapid neutron-capture process (r process) …

What is the origin of the oxygen we breathe, the hydrogen and oxygen (in form of water
H2O) in rivers and oceans, the carbon in all organic compounds, the silicon in electronic …

A review is given of various theoretical approaches for the equation of state (EoS) of dense
matter, relevant for the description of core-collapse supernovae, compact stars, and compact …

The mergers of double neutron star (NS–NS) and black hole (BH)–NS binaries are
promising gravitational wave (GW) sources for Advanced LIGO and future GW detectors. The …

The production of elements by rapid neutron capture (r-process) in neutron-star mergers is
expected theoretically and is supported by multimessenger observations,–of gravitational …

We have conducted 19 state-of-the-art 3D core-collapse supernova simulations spanning a
broad range of progenitor masses. This is the largest collection of sophisticated 3D …

The coalescence of double neutron star (NS–NS) and black hole (BH)–NS binaries are
prime sources of gravitational waves (GW) for Advanced LIGO/Virgo and future ground …

The astrophysical rapid neutron capture process or 'r process' of nucleosynthesis is believed
to be responsible for the production of approximately half the heavy element abundances …

Recent studies suggest that binary neutron star (NS–NS) mergers robustly produce heavy r-
process nuclei above the atomic mass number A∼ 130 because their ejecta consist of …

We revise the bound from the supernova SN1987A on the coupling of ultralight axion-like
particles (ALPs) to photons. In a core-collapse supernova, ALPs would be emitted via the …