Measurement of reaction relevant to 0 decay searches of and astrophysical -process temperatures
Yu-Bing Li · Zhen-Dong An · Wei Jiang🇨🇳 · Cheng Li · Yu-Gang Ma🇨🇳 · Jie Ren🇨🇳 · Xi-Chao Ruan🇨🇳 · Rui-Rui Fan🇨🇳 · Jing-Yu Tang🇨🇳 · Xiang-Zhou Cai🇨🇳 · Hong-Wei Wang🇨🇳 · Chen-Chen Guo🇨🇳 and 4 other authors
The cross sections and resonance structures of (n,) reaction are critical to the neutrinoless double- (0) decay searches of , the -process nucleosynthesis of nuclear astrophysics, and Neutron Resonance Capture Analysis for determining the elemental and isotopic composition of archaeological and cultural heritage. We report a high-precision measurement of the neutron capture cross sections from 1~eV to 1~MeV, performed at the Back-n facility of the China Spallation Neutron Source using the Time-of-Flight method. In the resolved resonance region, nineteen resonance structures of (n,) reaction have been discovered for the first time, and inconsistencies between evaluated libraries has been resolved. Resonance parameters for the newly observed structures were extracted with the -matrix code SAMMY. These findings will help refine the theoretical predictions of half-lives and decay constants for the double- decay searches of . Astrophysical Maxwellian-averaged cross sections were calculated based on the averaged cross sections in the unresolved resonance region. And the (n,) reaction rates were derived over the astrophysically relevant temperature range in both the main and weak -processes nucleosynthesis. The present reaction rates deviate significantly from the recent theoretical predictions, and the uncertainties are significantly reduced.