We summarize our current knowledge of neutron-star masses and radii. Recent
instrumentation and computational advances have resulted in a rapid increase in the …

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 attempt to understand the physics of the structure of stars and their change in time–their
evolution–has been bothering many physicists and astronomers ever since the last century …

Abstract Rayleigh–Taylor (RT) and Richtmyer–Meshkov (RM) instabilities are well-known
pathways towards turbulent mixing layers, in many cases characterized by significant mass …

This overview paper describes the legacy prospect and discovery potential of the Dark
Energy Survey (DES) beyond cosmological studies, illustrating it with examples from the …

Quasinormal modes are eigenmodes of dissipative systems. Perturbations of classical
gravitational backgrounds involving black holes or branes naturally lead to quasinormal …

Supernova theory, numerical and analytic, has made remarkable progress in the past
decade. This progress was made possible by more sophisticated simulation tools, especially …

Knowledge of the progenitors of core-collapse supernovae is a fundamental component in
understanding the explosions. The recent progress in finding such stars is reviewed. The …

The nature of dark matter and properties of neutrinos are among the most pressing issues in
contemporary particle physics. The dual-phase xenon time-projection chamber is the …

Abstract The Jiangmen Underground Neutrino Observatory (JUNO) is a 20 kton liquid
scintillator detector in a laboratory at 700-m underground. An excellent energy resolution …