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 …
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 …
Precision Determination of the Neutral Weak Form Factor of
We report a precise measurement of the parity-violating (PV) asymmetry A PV in the elastic
scattering of longitudinally polarized electrons from Ca 48. We measure A PV= 2668±106 …
scattering of longitudinally polarized electrons from Ca 48. We measure A PV= 2668±106 …
Implications of PREX-2 on the equation of state of neutron-rich matter
Laboratory experiments sensitive to the equation of state of neutron rich matter in the vicinity
of nuclear saturation density provide the first rung in a “density ladder” that connects …
of nuclear saturation density provide the first rung in a “density ladder” that connects …
Ab initio predictions link the neutron skin of 208Pb to nuclear forces
Heavy atomic nuclei have an excess of neutrons over protons, which leads to the formation
of a neutron skin whose thickness is sensitive to details of the nuclear force. This links …
of a neutron skin whose thickness is sensitive to details of the nuclear force. This links …
Impact of the PSR radius constraint on the properties of high-density matter
X-ray pulse profile modeling of PSR J 0740+ 6620, the most massive known pulsar, with
data from the NICER and XMM-Newton observatories recently led to a measurement of its …
data from the NICER and XMM-Newton observatories recently led to a measurement of its …
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 …
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 …
GW190814: Impact of a 2.6 solar mass neutron star on the nucleonic equations of state
Is the secondary component of GW190814 the lightest black hole or the heaviest neutron
star ever discovered in a double compact-object system [Abbott et al. Astrophys. J. 896, L44 …
star ever discovered in a double compact-object system [Abbott et al. Astrophys. J. 896, L44 …
Information Content of the Parity-Violating Asymmetry in
The parity-violating asymmetry A PV in Pb 208, recently measured by the PREX-2
Collaboration, is studied using modern relativistic (covariant) and nonrelativistic energy …
Collaboration, is studied using modern relativistic (covariant) and nonrelativistic energy …