Journal
PHYSICAL REVIEW C
Volume 108, Issue 1, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevC.108.015802
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The correlation between charge radii differences in mirror nuclei pairs and neutron skin thickness was studied using a finite range simple effective interaction model. Precisely measured charge radii difference data in mirror pairs such as 34Ar-34S, 36Ca-36S, 38Ca-38Ar, and 54Ni-54Fe were used to determine an upper limit for the slope parameter of nuclear symmetry energy, L, at around 100 MeV. The upper limit of L was found to be consistent with the upper bound of the NICER PSR J0740+6620 constraint for the radius R1.4 of 1.4M0 neutron stars at the 1σ level. The lower bound of the NICER R1.4 data constrains the lower limit of L to approximately 70 MeV. The tidal deformability 1.4 constraint extracted from the GW170817 event at the 2σ level and recent PREX-2 and CREX data on neutron skin thickness are discussed within the range of L = 70-100 MeV.
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 34Ar-34S, 36Ca-36S, 38Ca-38Ar, and 54Ni-54Fe mirror pairs are used to ascertain an upper limit for the slope parameter of the nuclear symmetry energy L & AP; 100 MeV. This limiting value of L is found to be consistent with the upper bound of the NICER PSR J0740+6620 constraint at 1 & sigma; level for the radius R1.4 of 1.4M0 neutron stars. The lower bound of the NICER R1.4 data constrains the lower limit of L to & AP;70 MeV. Within the range for L = 70-100 MeV the tidal deformability 1.4 constraint, which is extracted from the GW170817 event at 2 & sigma; level, and the recent PREX-2 and CREX data on the neutron skin thickness are discussed.
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