Exascale computing could soon enable a predictive theory of nuclear structure and
reactions rooted in the Standard Model, with quantifiable and systematically improvable …

Determining the sound speed cs in compact stars is an important open question with
numerous implications on the behavior of matter at large densities and hence on …

We demonstrate in a general and analytic way how high-density information about the
equation of state (EOS) of strongly interacting matter obtained using perturbative quantum …

Recent rapid progress in neutron-star (NS) observations offers great potential to constrain
the properties of strongly interacting matter under the most extreme conditions. In order to …

Over the last 40 years, an astonishing range of astrophysics has become accessible through
pulsar astronomy. The body of literature on this rapidly growing research area is vast and …

We have investigated the systematic differences introduced when performing a Bayesian-
inference analysis of the equation of state (EOS) of neutron stars employing either variable …

Motivated by the recent discovery of a compact object with mass in the range 2.5–2.67 M⊙
in the binary merger GW190814, we revisit the question of the maximum mass of neutron …

We perform a joint Bayesian inference of neutron-star mass and radius constraints based on
GW170817, observations of quiescent low-mass x-ray binaries (QLMXBs), photospheric …

The maximum mass of a non-rotating neutron star, M TOV, plays a very important role in
deciphering the structure and composition of neutron stars and in revealing the equation of …

A considerable effort has been dedicated recently to the construction of generic equations of
state (EOSs) for matter in neutron stars. The advantage of these approaches is that they can …