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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 …
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 …
Constraints on the dense matter equation of state and neutron star properties from NICER's mass–radius estimate of PSR J0740+ 6620 and multimessenger …
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 …
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 …
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 …
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 …
Constraints on nuclear symmetry energy parameters
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 …
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 …
Equations of state for supernovae and compact stars
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 …
Combined Theoretical Analysis of the Parity-Violating Asymmetry for and
The recent experimental determination of the parity violating asymmetry A PV in Ca 48 and
Pb 208 at Jefferson Lab is important for our understanding on how neutrons and protons …
Pb 208 at Jefferson Lab is important for our understanding on how neutrons and protons …