We investigate how current and proposed observations of neutron stars can lead to an
understanding of the state of their interiors and the key unknowns: the typical neutron star …

We investigate the structure of neutron stars shortly after they are born, when the entropy per
baryon is of order 1 or 2 and neutrinos are trapped on dynamical timescales. We find that the …

The structure of neutron stars is considered from theoretical and observational perspectives.
We demonstrate an important aspect of neutron star structure: the neutron star radius is …

Neutron stars are some of the densest manifestations of massive objects in the universe.
They are ideal astrophysical laboratories for testing theories of dense matter physics and …

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

In recent years, the number of pulsars with secure mass measurements has increased to a
level that allows us to probe the underlying neutron star (NS) mass distribution in detail. We …

We present an improved method for determining the mass of neutron stars in eclipsing X-ray
pulsar binaries and apply the method to six systems, namely, Vela X-1, 4U 1538-52, SMC X …

We present new results for pulsating neutron stars. We have calculated the
eigenfrequencies of the modes that one would expect to be the most important gravitational …

Rotating relativistic stars have been studied extensively in recent years, both theoretically
and observationally, because of the information they might yield about the equation of state …

We derive an equation of state (EOS) for strange matter, starting from an interquark potential
which (i) has asymptotic freedom built into it,(ii) shows confinement at zero density (ρB= 0) …