Stellar structure models in modified theories of gravity: Lessons and challenges
The understanding of stellar structure represents the crossroads of our theories of the
nuclear force and the gravitational interaction under the most extreme conditions observably …
nuclear force and the gravitational interaction under the most extreme conditions observably …
CompOSE reference manual: Version 3.01, CompStar Online Supernovæ Equations of State, “harmonising the concert of nuclear physics and astrophysics”, https …
CompOSE Core Team, S Typel, M Oertel… - The European Physical …, 2022 - Springer
Abstract CompOSE (CompStar Online Supernovae Equations of State) is an online
repository of equations of state (EoS) for use in nuclear physics and astrophysics, eg, in the …
repository of equations of state (EoS) for use in nuclear physics and astrophysics, eg, in the …
Overview of KAGRA: KAGRA science
KAGRA is a newly build gravitational wave observatory, a laser interferometer with 3 km arm
length, located in Kamioka, Gifu, Japan. In this paper, one of a series of articles featuring …
length, located in Kamioka, Gifu, Japan. In this paper, one of a series of articles featuring …
Spanning the full range of neutron star properties within a microscopic description
The high-density behavior of nuclear matter is analyzed within a relativistic mean field
description with nonlinear meson interactions. To assess the model parameters and their …
description with nonlinear meson interactions. To assess the model parameters and their …
Relativistic description of dense matter equation of state and compatibility with neutron star observables: a Bayesian approach
The general behavior of the nuclear equation of state (EOS), relevant for the description of
neutron stars (NSs), is studied within a Bayesian approach applied to a set of models based …
neutron stars (NSs), is studied within a Bayesian approach applied to a set of models based …
On the deconfinement phase transition in neutron-star mergers
We study in detail the nuclear aspects of a neutron-star merger in which deconfinement to
quark matter takes place. For this purpose, we make use of the Chiral Mean Field (CMF) …
quark matter takes place. For this purpose, we make use of the Chiral Mean Field (CMF) …
On the maximum mass and oblateness of rotating neutron stars with generic equations of state
A considerable effort has been dedicated recently to the construction of generic equations of
state (EOSs) for matter in neutron stars. The advantage of these approaches is that they can …
state (EOSs) for matter in neutron stars. The advantage of these approaches is that they can …
Perturbative QCD and the neutron star equation of state
We construct a physics-agnostic approach to the neutron star (NS) equation of state (EoS)
based on a sound speed model, which connects both low-density information from nuclear …
based on a sound speed model, which connects both low-density information from nuclear …
Spin effects on neutron star fundamental-mode dynamical tides: Phenomenology and comparison to numerical simulations
J Steinhoff, T Hinderer, T Dietrich, F Foucart - Physical Review Research, 2021 - APS
Gravitational waves from neutron star binary inspirals contain information on strongly
interacting matter in unexplored, extreme regimes. Extracting this requires robust theoretical …
interacting matter in unexplored, extreme regimes. Extracting this requires robust theoretical …
Exploring robust correlations between fermionic dark matter model parameters and neutron star properties: A two-fluid perspective
We investigate the probable existence of dark matter in the interior of neutron stars. Despite
the current state of knowledge, the observational properties of neutron stars have not …
the current state of knowledge, the observational properties of neutron stars have not …