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 …
Accurate Determination of the Neutron Skin Thickness of through Parity-Violation in Electron Scattering
We report a precision measurement of the parity-violating asymmetry A PV in the elastic
scattering of longitudinally polarized electrons from Pb 208. We measure A PV= 550±16 …
scattering of longitudinally polarized electrons from Pb 208. We measure A PV= 550±16 …
[HTML][HTML] Neutron star equation of state: Quark mean-field (QMF) modeling and applications
Because of the development of many-body theories of nuclear matter, the long-standing,
open problem of the equation of state (EOS) of dense matter may be understood in the near …
open problem of the equation of state (EOS) of dense matter may be understood in the near …
[HTML][HTML] Equations of state for hot neutron stars
AR Raduta, F Nacu, M Oertel - The European Physical Journal A, 2021 - Springer
We review the equation of state (EoS) models covering a large range of temperatures,
baryon number densities and electron fractions presently available on the CompOSE …
baryon number densities and electron fractions presently available on the CompOSE …
Charge Radius of Neutron-Deficient and Symmetry Energy Constraints Using the Difference in Mirror Pair Charge Radii
SV Pineda, K König, DM Rossi, BA Brown, A Incorvati… - Physical Review Letters, 2021 - APS
The nuclear root-mean-square charge radius of Ni 54 was determined with collinear laser
spectroscopy to be R (Ni 54)= 3.737 (3) fm. In conjunction with the known radius of the mirror …
spectroscopy to be R (Ni 54)= 3.737 (3) fm. In conjunction with the known radius of the mirror …
Recent multimessenger constraints and the anisotropic neutron star
A Rahmansyah, A Sulaksono - Physical Review C, 2021 - APS
The impact of anisotropic pressure models in neutron stars (NSs) is increasing their
compactness. Therefore, for the relatively soft NS equation of state (EOS), we can still obtain …
compactness. Therefore, for the relatively soft NS equation of state (EOS), we can still obtain …
Relativistic mean-field theories for neutron-star physics based on chiral effective field theory
We describe and implement a procedure for determining the couplings of a relativistic mean-
field theory (RMFT) that is optimized for application to neutron star phenomenology. In the …
field theory (RMFT) that is optimized for application to neutron star phenomenology. In the …
Nuclear and hybrid equations of state in light of the low-mass compact star in HESS J1731-347
We sample over 500 relativistic mean-field theories constrained by chiral effective-field
theory and properties of isospin-symmetric nuclear matter and test them against known …
theory and properties of isospin-symmetric nuclear matter and test them against known …
Correlations between charge radii differences of mirror nuclei and stellar observables
P Bano, SP Pattnaik, M Centelles, X Viñas, TR Routray - Physical Review C, 2023 - APS
The correlation between the charge radii differences in mirror nuclei pairs and the neutron
skin thickness has been studied with the so-called finite range simple effective interaction …
skin thickness has been studied with the so-called finite range simple effective interaction …
Constraining a relativistic mean field model using neutron star mass–radius measurements I: nucleonic models
Measurements of neutron star mass and radius or tidal deformability deliver unique insight
into the equation of state (EOS) of cold dense matter. EOS inference is very often done using …
into the equation of state (EOS) of cold dense matter. EOS inference is very often done using …