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

One century after its formulation, Einstein's general relativity (GR) has made remarkable
predictions and turned out to be compatible with all experimental tests. Most of these tests …

Neutron stars are valuable laboratories for the study of dense matter. Recent observations
have uncovered both massive and low-mass neutron stars and have also set constraints on …

In this study, we explore several new characteristics of a static anisotropic hybrid star with
strange quark matter (SQM) and ordinary baryonic matter (OBM) distribution. Here, we use …

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 this article, we explore some emerging properties of the stellar objects in the frame of the f
(R, T) gravity by employing the well-known Karmarkar condition, where R and T represent …

This work aims to investigate the behaviour of compact stars in the background of f (R, T)
f(R,T) theory of gravity. For current work, we consider the Krori‐Barua metric potential ie, ν …

The equation of state (EOS) of dense matter has been a long-sought goal of nuclear physics.
EOSs generate unique mass versus radius (M–R) relations for neutron stars, the ultra-dense …

We present a comprehensive study of spectroscopic radius measurements of twelve neutron
stars obtained during thermonuclear bursts or in quiescence. We incorporate, for the first …

We investigate the distribution of neutron star masses in different populations of binaries,
employing Bayesian statistical techniques. In particular, we explore the differences in …