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 …

Neutron skins: weak elastic scattering and neutron stars

JM Mammei, CJ Horowitz, J Piekarewicz… - Annual Review of …, 2024 - annualreviews.org
The recently completed PREX-2 campaign measured the density distribution of neutrons in
the lead nucleus as a function of momentum transfer (the form factor), confirmed a relatively …

Observing the thermalization of dark matter in neutron stars

R Garani, A Gupta, N Raj - Physical Review D, 2021 - APS
A promising probe to unmask particle dark matter is to observe its effect on neutron stars, the
prospects of which depend critically on whether captured dark matter thermalizes in a timely …

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 …

Thermal evolution of neutron stars in soft X-ray transients with thermodynamically consistent models of the accreted crust

AY Potekhin, ME Gusakov… - Monthly Notices of the …, 2023 - academic.oup.com
Thermal emission of neutron stars in soft X-ray transients (SXTs) in a quiescent state is
believed to be powered by the heat deposited in the stellar crust due to nuclear reactions …

Quark Pauli principle and the transmutation of nuclear matter

L McLerran, GA Miller - Physical Review C, 2024 - APS
The phase space density, ρ Q, of quarks in nuclei is studied using realistic models of
unintegrated quark distributions, known as transverse momentum densities (TMDs). If this …

Giant planet formation in Palatini gravity

A Wojnar - Physical Review D, 2022 - APS
Some parts of the accretion model of the Jovian planets' formation are studied in the context
of Palatini gravity. We mainly focus on the critical core mass, that is, a mass for which there is …

Revisiting constraints on asymmetric dark matter from collapse in white dwarf stars

H Steigerwald, V Marra, S Profumo - Physical Review D, 2022 - APS
The runaway collapse phase of a small dark matter cluster inside a white dwarf star
encompasses a reversible stage, where heat can be transferred back and forth between …

Density dependence of the symmetry energy in the post–PREX-CREX era

BT Reed, FJ Fattoyev, CJ Horowitz, J Piekarewicz - Physical Review C, 2024 - APS
The recently published CREX results suggest a rather peculiar picture for the density
dependence of the symmetry energy. Whereas PREX favors a large neutron skin thickness …

Multicomponent multiscatter capture of dark matter

C Ilie, C Levy - Physical Review D, 2021 - APS
In recent years, the usefulness of astrophysical objects as dark matter (DM) probes has
become more and more evident, especially in view of null results from direct-detection and …