From hadrons to quarks in neutron stars: a review
In recent years our understanding of neutron stars has advanced remarkably, thanks to
research converging from many directions. The importance of understanding neutron star …
research converging from many directions. The importance of understanding neutron star …
Gravitational waves from neutron star mergers and their relation to the nuclear equation of state
L Baiotti - Progress in Particle and Nuclear Physics, 2019 - Elsevier
In this article, I introduce ideas and techniques to extract information about the equation of
state of matter at very high densities from gravitational waves emitted before, during and …
state of matter at very high densities from gravitational waves emitted before, during and …
Gravitational-wave constraints on the neutron-star-matter Equation of State
The detection of gravitational waves originating from a neutron-star merger, GW170817, by
the LIGO and Virgo Collaborations has recently provided new stringent limits on the tidal …
the LIGO and Virgo Collaborations has recently provided new stringent limits on the tidal …
Evidence for quark-matter cores in massive neutron stars
The theory governing the strong nuclear force—quantum chromodynamics—predicts that at
sufficiently high energy densities, hadronic nuclear matter undergoes a deconfinement …
sufficiently high energy densities, hadronic nuclear matter undergoes a deconfinement …
New constraints on radii and tidal deformabilities of neutron stars from GW170817
We explore in a parameterized manner a very large range of physically plausible equations
of state (EOSs) for compact stars for matter that is either purely hadronic or that exhibits a …
of state (EOSs) for compact stars for matter that is either purely hadronic or that exhibits a …
On the sound speed in neutron stars
S Altiparmak, C Ecker, L Rezzolla - The astrophysical journal …, 2022 - iopscience.iop.org
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 …
numerous implications on the behavior of matter at large densities and hence on …
How well do we know the neutron-matter equation of state at the densities inside neutron stars? A Bayesian approach with correlated uncertainties
C Drischler, RJ Furnstahl, JA Melendez, DR Phillips - Physical Review Letters, 2020 - APS
We introduce a new framework for quantifying correlated uncertainties of the infinite-matter
equation of state derived from chiral effective field theory (χ EFT). Bayesian machine …
equation of state derived from chiral effective field theory (χ EFT). Bayesian machine …
Multimessenger constraints for ultradense matter
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 …
the properties of strongly interacting matter under the most extreme conditions. In order to …
A NICER view of PSR J0030+ 0451: Implications for the dense matter equation of state
G Raaijmakers, TE Riley, AL Watts… - The Astrophysical …, 2019 - iopscience.iop.org
Both the mass and radius of the millisecond pulsar PSR J0030+ 0451 have been inferred
via pulse-profile modeling of X-ray data obtained by NASA's Neutron Star Interior …
via pulse-profile modeling of X-ray data obtained by NASA's Neutron Star Interior …
Constraining the dense matter equation of state with joint analysis of NICER and LIGO/Virgo measurements
G Raaijmakers, SK Greif, TE Riley… - The Astrophysical …, 2020 - iopscience.iop.org
Abstract The Neutron Star Interior Composition Explorer collaboration recently published a
joint estimate of the mass and the radius of PSR J0030+ 0451, derived via X-ray pulse …
joint estimate of the mass and the radius of PSR J0030+ 0451, derived via X-ray pulse …