Differential analysis of incompressibility in neutron-rich nuclei
Abstract
Both the incompressibility KA of a finite nucleus of mass A and that (K∞) of infinite nuclear matter are fundamentally important for many critical issues in nuclear physics and astrophysics. While some consensus has been reached about K∞, accurate theoretical predictions and experimental extractions of Kτ characterizing the isospin dependence of KA have been very difficult. We propose a differential approach to extract Kτ and K∞ independently from the KA data of any two nuclei in a given isotope chain. Applying this method to the KA data from isoscalar giant monopole resonances (ISGMR) in even-even Pb, Sn, Cd, and Ca isotopes taken by Garg et al. at the Research Center for Nuclear Physics (RCNP), Osaka University, Japan, we find that the 106Cd–116Cd and 112Sn–124Sn pairs having the largest differences in isospin asymmetries in their respective isotope chains measured so far provide consistently the most accurate up-to-date Kτ value of Kτ = –616 ± 59 MeV and Kτ =–623 ± 86 MeV, respectively, largely independent of the remaining uncertainties of the surface and Coulomb terms in expanding KA, while the K∞ values extracted from different isotopes chains are all well within the current uncertainty range of the community consensus for K∞.more »
- Authors:
-
- Texas A & M Univ., Commerce, TX (United States)
- Yuncheng Univ. (China)
- Publication Date:
- Research Org.:
- Texas A & M Univ., Commerce, TX (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC)
- OSTI Identifier:
- 1837890
- Grant/Contract Number:
- SC0013702; SC0009971
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Physical Review C
- Additional Journal Information:
- Journal Volume: 104; Journal Issue: 3; Journal ID: ISSN 2469-9985
- Publisher:
- American Physical Society (APS)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 73 NUCLEAR PHYSICS AND RADIATION PHYSICS; Low & intermediate energy heavy-ion reactions; Nuclear many-body theory; Nuclear matter; 90 ≤ A ≤ 149
Citation Formats
Li, Bao-An, and Xie, Wen-Jie. Differential analysis of incompressibility in neutron-rich nuclei. United States: N. p., 2021.
Web. doi:10.1103/physrevc.104.034610.
Li, Bao-An, & Xie, Wen-Jie. Differential analysis of incompressibility in neutron-rich nuclei. United States. https://doi.org/10.1103/physrevc.104.034610
Li, Bao-An, and Xie, Wen-Jie. Thu .
"Differential analysis of incompressibility in neutron-rich nuclei". United States. https://doi.org/10.1103/physrevc.104.034610. https://www.osti.gov/servlets/purl/1837890.
@article{osti_1837890,
title = {Differential analysis of incompressibility in neutron-rich nuclei},
author = {Li, Bao-An and Xie, Wen-Jie},
abstractNote = {Both the incompressibility KA of a finite nucleus of mass A and that (K∞) of infinite nuclear matter are fundamentally important for many critical issues in nuclear physics and astrophysics. While some consensus has been reached about K∞, accurate theoretical predictions and experimental extractions of Kτ characterizing the isospin dependence of KA have been very difficult. We propose a differential approach to extract Kτ and K∞ independently from the KA data of any two nuclei in a given isotope chain. Applying this method to the KA data from isoscalar giant monopole resonances (ISGMR) in even-even Pb, Sn, Cd, and Ca isotopes taken by Garg et al. at the Research Center for Nuclear Physics (RCNP), Osaka University, Japan, we find that the 106Cd–116Cd and 112Sn–124Sn pairs having the largest differences in isospin asymmetries in their respective isotope chains measured so far provide consistently the most accurate up-to-date Kτ value of Kτ = –616 ± 59 MeV and Kτ =–623 ± 86 MeV, respectively, largely independent of the remaining uncertainties of the surface and Coulomb terms in expanding KA, while the K∞ values extracted from different isotopes chains are all well within the current uncertainty range of the community consensus for K∞. Moreover, the size and origin of the “soft Sn puzzle” is studied with respect to the “stiff Pb phenomenon.” Furthermore, it is found that the latter is favored due to a much larger (by ≈ 380 MeV) Kτ for Pb isotopes than for Sn isotopes, while K∞ from analyzing the KA data of Sn isotopes is only about 5 MeV less than that from analyzing the Pb data.},
doi = {10.1103/physrevc.104.034610},
journal = {Physical Review C},
number = 3,
volume = 104,
place = {United States},
year = {Thu Sep 09 00:00:00 EDT 2021},
month = {Thu Sep 09 00:00:00 EDT 2021}
}
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