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 inarXiv.org
Main Authors Jun-Yao, Xu, Zheng-Zheng, Li, Bao-Hua, Sun, Yi-Fei Niu, Roca-Maza, Xavier, Sagawa, Hiroyuki, Tanihata, Isao
Format Paper Journal Article
LanguageEnglish
Published Ithaca Cornell University Library, arXiv.org 29.07.2022
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ISSN2331-8422
DOI10.48550/arxiv.2205.05276

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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 (\(E_\text{sym}(\rho)\)) 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 (\(\Delta\sigma_\text{cc}\)) of mirror nuclei \(^{30}\)Si-\(^{30}\)S 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 \(\Delta\sigma_\text{cc}\) 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 Physics Letter B 833 (2022)137333 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 ($E_\text{sym}(\rho)$) 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 ($\Delta\sigma_\text{cc}$) of mirror nuclei $^{30}$Si-$^{30}$S 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 $\Delta\sigma_\text{cc}$ 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.
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 (\(E_\text{sym}(\rho)\)) 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 (\(\Delta\sigma_\text{cc}\)) of mirror nuclei \(^{30}\)Si-\(^{30}\)S 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 \(\Delta\sigma_\text{cc}\) 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.
Author Zheng-Zheng, Li
Bao-Hua, Sun
Jun-Yao, Xu
Yi-Fei Niu
Roca-Maza, Xavier
Sagawa, Hiroyuki
Tanihata, Isao
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BackLink https://doi.org/10.48550/arXiv.2205.05276$$DView paper in arXiv
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Snippet 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...
Physics Letter B 833 (2022)137333 The nuclear symmetry energy plays a key role in determining the equation of state (EoS) of dense, neutron-rich matter, which...
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proquest
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SubjectTerms Astronomy
Equations of state
Linearity
Nuclear cross sections
Nuclear matter
Nuclei (nuclear physics)
Physics - Nuclear Theory
Saturation
Superhigh frequencies
Symmetry
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Title Constraining equation of state of nuclear matter by charge-changing cross section measurements of mirror nuclei
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