Constraining equation of state of nuclear matter by charge-changing cross section measurements of mirror nuclei

The nuclear symmetry energy plays a key role in determining the equation of state (EoS) of dense, neutron-rich matter, which connects the atomic nuclei with the hot and dense matter in universe, thus has been the subject of intense investigations in laboratory experiments, astronomy observations and...

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Published inPhysics letters. B Vol. 833; p. 137333
Main Authors Xu, Jun-Yao, Li, Zheng-Zheng, Sun, Bao-Hua, Niu, Yi-Fei, Roca-Maza, Xavier, Sagawa, Hiroyuki, Tanihata, Isao
Format Journal Article
LanguageEnglish
Published Elsevier 01.10.2022
Subjects
Charge-changing cross section
Equation of state of nuclear matter
Mirror nuclei
Symmetry energy
Online AccessGet full text
ISSN0370-2693
DOI10.1016/j.physletb.2022.137333

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Abstract The nuclear symmetry energy plays a key role in determining the equation of state (EoS) of dense, neutron-rich matter, which connects the atomic nuclei with the hot and dense matter in universe, thus has been the subject of intense investigations in laboratory experiments, astronomy observations and theories. Various probes have been proposed to constrain the symmetry energy and its density dependence. Currently, the extensive data yield already a good and consistent constraint to the symmetry energy (Esym(ρ)) at saturation density, but do not yet give a consistent result of one critical EoS parameter, L, the density dependence of the symmetry energy. In this work, we report a new probe of L at saturation density. A good linear correlation is found between L and the charge changing cross section difference (Δσcc) of mirror nuclei 30Si-30S for both the Skyrme-Hartree-Fock theory (SHF) and covariant (relativistic) density functionals (CDF). We found that the pairing effect for this mirror pair is essential to get a consistent correlation between L and Δσcc in both the SHF and CDF. Here, the cross sections are calculated on the same target and at the same energy using the zero-range optical-limit Glauber model. The linearity is found to be in the same precision as those found between L and neutron skin thickness or proton radius difference.
AbstractList The nuclear symmetry energy plays a key role in determining the equation of state (EoS) of dense, neutron-rich matter, which connects the atomic nuclei with the hot and dense matter in universe, thus has been the subject of intense investigations in laboratory experiments, astronomy observations and theories. Various probes have been proposed to constrain the symmetry energy and its density dependence. Currently, the extensive data yield already a good and consistent constraint to the symmetry energy (Esym(ρ)) at saturation density, but do not yet give a consistent result of one critical EoS parameter, L, the density dependence of the symmetry energy. In this work, we report a new probe of L at saturation density. A good linear correlation is found between L and the charge changing cross section difference (Δσcc) of mirror nuclei 30Si-30S for both the Skyrme-Hartree-Fock theory (SHF) and covariant (relativistic) density functionals (CDF). We found that the pairing effect for this mirror pair is essential to get a consistent correlation between L and Δσcc in both the SHF and CDF. Here, the cross sections are calculated on the same target and at the same energy using the zero-range optical-limit Glauber model. The linearity is found to be in the same precision as those found between L and neutron skin thickness or proton radius difference.
ArticleNumber 137333
Author Li, Zheng-Zheng
Xu, Jun-Yao
Roca-Maza, Xavier
Niu, Yi-Fei
Sagawa, Hiroyuki
Tanihata, Isao
Sun, Bao-Hua
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SubjectTerms Charge-changing cross section
Equation of state of nuclear matter
Mirror nuclei
Symmetry energy
Title Constraining equation of state of nuclear matter by charge-changing cross section measurements of mirror nuclei
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