Precision Determination of the Neutral Weak Form Factor of

D Adhikari, H Albataineh, D Androic, KA Aniol… - Physical review …, 2022 - APS
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 …

Accurate Determination of the Neutron Skin Thickness of through Parity-Violation in Electron Scattering

D Adhikari, H Albataineh, D Androic, K Aniol… - Physical review …, 2021 - APS
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 …

[HTML][HTML] Neutron star equation of state: Quark mean-field (QMF) modeling and applications

A Li, ZY Zhu, EP Zhou, JM Dong, JN Hu… - Journal of High Energy …, 2020 - Elsevier
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 …

[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 …

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 …

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 …

Relativistic mean-field theories for neutron-star physics based on chiral effective field theory

MG Alford, L Brodie, A Haber, I Tews - Physical Review C, 2022 - APS
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 …

Nuclear and hybrid equations of state in light of the low-mass compact star in HESS J1731-347

L Brodie, A Haber - Physical Review C, 2023 - APS
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 …

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 …

Constraining a relativistic mean field model using neutron star mass–radius measurements I: nucleonic models

C Huang, G Raaijmakers, AL Watts… - Monthly Notices of …, 2024 - academic.oup.com
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 …