Matches in SemOpenAlex for { <https://semopenalex.org/work/W4384204216> ?p ?o ?g. }
- W4384204216 abstract "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 over a wide mass region. The so far precisely measured charge radii difference data within their experimental uncertainty ranges in the $^{34}mathrm{Ar}text{ensuremath{-}}^{34}mathrm{S}$, $^{36}mathrm{Ca}text{ensuremath{-}}^{36}mathrm{S}$, $^{38}mathrm{Ca}text{ensuremath{-}}^{38}mathrm{Ar}$, and $^{54}mathrm{Ni}text{ensuremath{-}}^{54}mathrm{Fe}$ mirror pairs are used to ascertain an upper limit for the slope parameter of the nuclear symmetry energy $Lensuremath{approx}100$ MeV. This limiting value of $L$ is found to be consistent with the upper bound of the NICER PSR $mathrm{J}0740+6620$ constraint at $1ensuremath{sigma}$ level for the radius ${R}_{1.4}$ of $1.4{M}_{ensuremath{bigodot}}$ neutron stars. The lower bound of the NICER ${R}_{1.4}$ data constrains the lower limit of $L$ to $ensuremath{approx}70$ MeV. Within the range for $L=70--100$ MeV the tidal deformability ${mathrm{ensuremath{Lambda}}}^{1.4}$ constraint, which is extracted from the GW170817 event at $2ensuremath{sigma}$ level, and the recent PREX-2 and CREX data on the neutron skin thickness are discussed." @default.
- W4384204216 created "2023-07-14" @default.
- W4384204216 creator A5006794204 @default.
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- W4384204216 creator A5038386185 @default.
- W4384204216 creator A5050839169 @default.
- W4384204216 date "2023-07-13" @default.
- W4384204216 modified "2023-10-14" @default.
- W4384204216 title "Correlations between charge radii differences of mirror nuclei and stellar observables" @default.
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- W4384204216 doi "https://doi.org/10.1103/physrevc.108.015802" @default.
- W4384204216 hasPublicationYear "2023" @default.