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 …

PSR J0740+ 6620 has a gravitational mass of 2.08±0.07 M⊙, which is the highest reliably
determined mass of any neutron star. As a result, a measurement of its radius will provide …

We report on Bayesian estimation of the radius, mass, and hot surface regions of the
massive millisecond pulsar PSR J0740+ 6620, conditional on pulse-profile modeling of …

We report on Bayesian parameter estimation of the mass and equatorial radius of the
millisecond pulsar PSR J0030+ 0451, conditional on pulse-profile modeling of Neutron Star …

Neutron stars are not only of astrophysical interest, but are also of great interest to nuclear
physicists because their attributes can be used to determine the properties of the dense …

To constrain the equation of state of cold dense matter, astrophysical measurements are
essential. These are mostly based on observations of neutron stars in the X-ray band, and …

The last decade has shown us that the observational properties of neutron stars are
remarkably diverse. From magnetars to rotating radio transients, from radio pulsars to …

Neutrinos play a crucial role in the collapse and explosion of massive stars, governing the
infall dynamics of the stellar core, triggering and fueling the explosion and driving the …

We determine an empirical dense matter equation of state (EOS) from a heterogeneous data
set of six neutron stars: three Type-I X-ray bursters with photospheric radius expansion …

In 2019 the NICER collaboration published the first mass and radius inferred for PSR
J0030+ 0451, thanks to NICER observations, and consequent constraints on the equation of …