Testing general relativity with present and future astrophysical observations
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 …
predictions and turned out to be compatible with all experimental tests. Most of these tests …
The nuclear equation of state and neutron star masses
JM Lattimer - Annual Review of Nuclear and Particle Science, 2012 - annualreviews.org
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 …
have uncovered both massive and low-mass neutron stars and have also set constraints on …
[HTML][HTML] Physical characteristics and maximum allowable mass of hybrid star in the context of f (Q) gravity
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 …
strange quark matter (SQM) and ordinary baryonic matter (OBM) distribution. Here, we use …
Study of embedded class-I fluid spheres in f (R, T) gravity with Karmarkar condition
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 …
(R, T) gravity by employing the well-known Karmarkar condition, where R and T represent …
Limiting masses and radii of neutron stars and their implications
We combine the equation of state of dense matter up to twice nuclear saturation density n
sat obtained using chiral effective field theory (χ EFT) and recent observations of neutron …
sat obtained using chiral effective field theory (χ EFT) and recent observations of neutron …
The dense matter equation of state from neutron star radius and mass measurements
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 …
stars obtained during thermonuclear bursts or in quiescence. We incorporate, for the first …
Tidal deformability of neutron stars with realistic equations of state<? format?> and their gravitational wave signatures in binary inspiral
The early part of the gravitational wave signal of binary neutron-star inspirals can potentially
yield robust information on the nuclear equation of state. The influence of a star's internal …
yield robust information on the nuclear equation of state. The influence of a star's internal …
Towards understanding astrophysical effects of nuclear symmetry energy
Determining the Equation of State (EOS) of dense neutron-rich nuclear matter is a shared
goal of both nuclear physics and astrophysics. Except possible phase transitions, the density …
goal of both nuclear physics and astrophysics. Except possible phase transitions, the density …
The equation of state from observed masses and radii of neutron stars
AW Steiner, JM Lattimer, EF Brown - The Astrophysical Journal, 2010 - iopscience.iop.org
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 …
set of six neutron stars: three Type-I X-ray bursters with photospheric radius expansion …
The neutron star mass–radius relation and the equation of state of dense matter
AW Steiner, JM Lattimer, EF Brown - The Astrophysical Journal …, 2013 - iopscience.iop.org
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 …
EOSs generate unique mass versus radius (M–R) relations for neutron stars, the ultra-dense …