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 …
Transport model comparison studies of intermediate-energy heavy-ion collisions
Transport models are the main method to obtain physics information on the nuclear equation
of state and in-medium properties of particles from low to relativistic-energy heavy-ion …
of state and in-medium properties of particles from low to relativistic-energy heavy-ion …
Neutron star observations: Prognosis for equation of state constraints
JM Lattimer, M Prakash - Physics reports, 2007 - Elsevier
We investigate how current and proposed observations of neutron stars can lead to an
understanding of the state of their interiors and the key unknowns: the typical neutron star …
understanding of the state of their interiors and the key unknowns: the typical neutron star …
Recent progress and new challenges in isospin physics with heavy-ion reactions
The ultimate goal of studying isospin physics via heavy-ion reactions with neutron-rich,
stable and/or radioactive nuclei is to explore the isospin dependence of in-medium nuclear …
stable and/or radioactive nuclei is to explore the isospin dependence of in-medium nuclear …
Constraints on the symmetry energy and neutron skins from experiments and theory
The symmetry energy contribution to the nuclear equation of state impacts various
phenomena in nuclear astrophysics, nuclear structure, and nuclear reactions. Its …
phenomena in nuclear astrophysics, nuclear structure, and nuclear reactions. Its …
Constraints on nuclear symmetry energy parameters
JM Lattimer - Particles, 2023 - mdpi.com
A review is made of constraints on the nuclear symmetry energy parameters arising from
nuclear binding energy measurements, theoretical chiral effective field predictions of …
nuclear binding energy measurements, theoretical chiral effective field predictions of …
Strangeness in nuclei and neutron stars
We review the present status of the experimental and theoretical developments in the field of
strangeness in nuclei and neutron stars. We start by discussing the K ̄ N interaction, that is …
strangeness in nuclei and neutron stars. We start by discussing the K ̄ N interaction, that is …
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 …
Constraints on the density dependence of the symmetry energy
Collisions involving Sn 112 and Sn 124 nuclei have been simulated with the improved
quantum molecular dynamics transport model. The results of the calculations reproduce …
quantum molecular dynamics transport model. The results of the calculations reproduce …