Dense nuclear matter equation of state from heavy-ion collisions
The nuclear equation of state (EOS) is at the center of numerous theoretical and
experimental efforts in nuclear physics. With advances in microscopic theories for nuclear …
experimental efforts in nuclear physics. With advances in microscopic theories for nuclear …
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 …
Science with the Einstein Telescope: a comparison of different designs
Abstract The Einstein Telescope (ET), the European project for a third-generation
gravitational-wave detector, has a reference configuration based on a triangular shape …
gravitational-wave detector, has a reference configuration based on a triangular shape …
Tidal deformabilities and radii of neutron stars from the observation of GW170817
We use gravitational-wave observations of the binary neutron star merger GW170817 to
explore the tidal deformabilities and radii of neutron stars. We perform a Bayesian parameter …
explore the tidal deformabilities and radii of neutron stars. We perform a Bayesian parameter …
Neutron stars and the nuclear equation of state
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 …
and phenomenological models, which are employed to construct the equation of state of …
How well do we know the neutron-matter equation of state at the densities inside neutron stars? A Bayesian approach with correlated uncertainties
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 …
Constraining neutron-star matter with microscopic and macroscopic collisions
Interpreting high-energy, astrophysical phenomena, such as supernova explosions or
neutron-star collisions, requires a robust understanding of matter at supranuclear densities …
neutron-star collisions, requires a robust understanding of matter at supranuclear densities …
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 …
High-quality two-nucleon potentials up to fifth order of the chiral expansion
We present NN potentials through five orders of chiral effective field theory ranging from
leading order (LO) to next-to-next-to-next-to-next-to-leading order (N 4 LO). The construction …
leading order (LO) to next-to-next-to-next-to-next-to-leading order (N 4 LO). The construction …
Chiral interactions up to next-to-next-to-next-to-leading order and nuclear saturation
We present an efficient Monte Carlo framework for perturbative calculations of infinite
nuclear matter based on chiral two-, three-, and four-nucleon interactions. The method …
nuclear matter based on chiral two-, three-, and four-nucleon interactions. The method …