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 matter equation of state
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 …
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 …
The radius of PSR J0740+ 6620 from NICER and XMM-Newton data
PSR J0740+ 6620 has a gravitational mass of 2.08±0.07 M⊙, which is the highest reliably
determined mass of any neutron star. As a result, a measurement of its radius will provide …
determined mass of any neutron star. As a result, a measurement of its radius will provide …
A strangely light neutron star within a supernova remnant
To constrain the equation of state of cold dense matter, astrophysical measurements are
essential. These are mostly based on observations of neutron stars in the X-ray band, and …
essential. These are mostly based on observations of neutron stars in the X-ray band, and …
A nicer view of the nearest and brightest millisecond pulsar: Psr j0437–4715
We report Bayesian inference of the mass, radius, and hot X-ray emitting region properties—
using data from the Neutron Star Interior Composition ExploreR (NICER)—for the brightest …
using data from the Neutron Star Interior Composition ExploreR (NICER)—for the brightest …
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 …
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 …
Exploring QCD matter in extreme conditions with Machine Learning
In recent years, machine learning has emerged as a powerful computational tool and novel
problem-solving perspective for physics, offering new avenues for studying strongly …
problem-solving perspective for physics, offering new avenues for studying strongly …