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 …
Equations of state for supernovae and compact stars
M Oertel, M Hempel, T Klähn, S Typel - Reviews of Modern Physics, 2017 - APS
A review is given of various theoretical approaches for the equation of state (EoS) of dense
matter, relevant for the description of core-collapse supernovae, compact stars, and compact …
matter, relevant for the description of core-collapse supernovae, compact stars, and compact …
Constraints on the dense matter equation of state and neutron star properties from NICER's mass–radius estimate of PSR J0740+ 6620 and multimessenger …
G Raaijmakers, SK Greif, K Hebeler… - The Astrophysical …, 2021 - iopscience.iop.org
In recent years our understanding of the dense matter equation of state (EOS) of neutron
stars has significantly improved by analyzing multimessenger data from radio/X-ray pulsars …
stars has significantly improved by analyzing multimessenger data from radio/X-ray pulsars …
Neutron stars and the nuclear matter equation of state
JM Lattimer - Annual Review of Nuclear and Particle Science, 2021 - annualreviews.org
Neutron stars provide a window into the properties of dense nuclear matter. Several recent
observational and theoretical developments provide powerful constraints on their structure …
observational and theoretical developments provide powerful constraints on their structure …
Chiral effective field theory and nuclear forces
We review how nuclear forces emerge from low-energy QCD via chiral effective field theory.
The presentation is accessible to the non-specialist. At the same time, we also provide …
The presentation is accessible to the non-specialist. At the same time, we also provide …
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 …
Nonparametric constraints on neutron star matter with existing and upcoming gravitational wave and pulsar observations
Observations of neutron stars, whether in binaries or in isolation, provide information about
the internal structure of the most extreme material objects in the Universe. In this work, we …
the internal structure of the most extreme material objects in the Universe. In this work, we …
Astrophysical Constraints on the Symmetry Energy and the Neutron Skin of with Minimal Modeling Assumptions
The symmetry energy and its density dependence are crucial inputs for many nuclear
physics and astrophysics applications, as they determine properties ranging from the …
physics and astrophysics applications, as they determine properties ranging from the …
Equation of state and neutron star properties constrained by nuclear physics and observation
Microscopic calculations of neutron matter based on nuclear interactions derived from chiral
effective field theory, combined with the recent observation of a 1.97±0.04 M☉ neutron star …
effective field theory, combined with the recent observation of a 1.97±0.04 M☉ neutron star …
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 …