4.5 Article

Temperature effects on neutron-capture cross sections and rates through electric dipole transitions in hot nuclei

期刊

PHYSICAL REVIEW C
卷 104, 期 4, 页码 -

出版社

AMER PHYSICAL SOC
DOI: 10.1103/PhysRevC.104.044332

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资金

  1. National Natural Science Foundation of China [12075104]
  2. Fun-damental Research Funds for the Central Universities [Lzujbky-2019-11]
  3. Romanian Ministry of Re-search and Innovation [PN 19 06 01 05]
  4. Extreme Light Infrastructure Nuclear Physics (ELI-NP) Phase II
  5. Romanian Government
  6. European Union through the European Regional De-velopment Fund-the Competitiveness Operational Program [1/07.07.2016, 1334]
  7. Institute of Atomic Physics (Magurele, Romania) under the ELI-RO program [ELI_15/16.10.2020]

向作者/读者索取更多资源

This study investigates the temperature evolution of electric dipole transition strengths of tin isotopes using self-consistent quasiparticle random phase approximation (QRPA) and finite-temperature RPA models based on a relativistic density functional. It was found that for lighter tin isotopes, temperature mainly affects at high temperatures, while for neutron-rich tin isotopes, the low-lying strength distributions become fragmented at lower temperatures. Additionally, the temperature effects on (n, gamma) cross sections were studied, showing significant enhancements for both light and neutron-rich tin isotopes.
The temperature evolution of electric dipole transition strengths of Sn isotopes is studied using self-consistent quasiparticle random phase approximation (QRPA) and finite-temperature RPA models based on a relativistic density functional. For tin isotopes lighter than Sn-132, temperature only shows its effect at high values of 2 MeV, while for neutron-rich tin isotopes heavier than Sn-132, the low-lying strength distributions get fragmented and spread to the lower-energy region already at temperature of 1 MeV. Using these electric dipole transition strengths as inputs for the TALYS code, the temperature effects on (n, gamma) cross sections are studied. For tin isotopes lighter than Sn-132, temperature causes an enhancement of neutron-capture cross section at high temperatures of 2 MeV, while for neutron-rich tin isotopes heavier than Sn-132, the cross section is largely enhanced already at temperature T = 1.0 MeV, and the bump of cross section caused by the pygmy dipole resonance also becomes broader. The change in neutron-capture rate can be as large as 70% for Sn-136, considering the temperature effects on electric dipole transition strength in the final compound nucleus with a temperature of 0.86 MeV (corresponding to T = 10 GK in the astrophysical environment). The change is around 20% for tin isotopes lighter than Sn-132 and above 40% for those heavier than Sn-132.

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