Neutron stars provide a cosmic laboratory to study the nature of dark matter particles and
their interactions. Dark matter can be captured by neutron stars via scattering, where kinetic …

Dark matter particles will be captured in neutron stars if they undergo scattering interactions
with nucleons or leptons. These collisions transfer the dark matter kinetic energy to the star …

Neutron stars harbour matter under extreme conditions, providing a unique testing ground
for fundamental interactions. We recently developed an improved treatment of dark matter …

The capture of dark matter, and its subsequent annihilation, can heat old, isolated neutron
stars. In order for kinetic heating to be achieved, the captured dark matter must undergo …

Prospects of establishing the radii of massive neutron stars in PSR J1614–2230 and PSR
J0740+ 6620 from Neutron Star Interior Composition ExploreR and Chandra observatories …

The first inspiral of two neutron stars observed in gravitational waves was remarkably close,
allowing the kind of simultaneous gravitational wave and electromagnetic observation that …

We discuss the hard dense loop resummation at finite quark mass and evaluate the
equation of state (EoS) of cold and dense QCD matter in β equilibrium. The resummation in …

Parity preserving relativistic fluids in four spacetime dimensions admit seven independent
thermodynamic susceptibilities at the second order in the hydrodynamic derivative …

Increasingly precise astrophysical observations of the last decade in combination with
intense theoretical studies allow for drawing a conclusion about potential quark matter …

The equation of state provided by effective models of strongly interacting matter should
comply with the restrictions imposed by current astrophysical observations of compact stars …