WDs and neutron stars are far-reaching and multi-faceted laboratories in the hunt for dark
matter. We review detection prospects of wave-like, particulate, macroscopic and black hole …

We review the current status and recent progress of microscopic many-body approaches
and phenomenological models, which are employed to construct the equation of state of …

We review the present status of the search for a phase transition and critical point as well as
anomalous transport phenomena in Quantum Chromodynamics (QCD), with an emphasis …

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 range of quantum field theoretical phenomena driven by external magnetic fields and their
applications in relativistic systems and quasirelativistic condensed matter ones, such as …

Matter at high density and low temperature is expected to be a color superconductor, which
is a degenerate Fermi gas of quarks with a condensate of Cooper pairs near the Fermi …

The ultimate goal of studying isospin physics via heavy-ion reactions with neutron-rich,
stable and/or radioactive nuclei is to explore the isospin dependence of in-medium nuclear …

In this work, we estimate how much bulk viscosity driven by Urca processes is likely to affect
the gravitational wave signal of a neutron star coalescence. In the late inspiral, we show that …

We introduce a parametrized high-density equation of state (EOS) in order to systematize
the study of constraints placed by astrophysical observations on the nature of neutron-star …

Using the concept of cracking we explore the influence that density fluctuations and local
anisotropy have on the stability of local and non-local anisotropic matter configurations in …