Measurement of the B(E2) strengths of Ca36 and Ca

N. Dronchi, D. Weißhaar,B. A. Brown, A. Gade, R. J. Charity, L. G. Sobotka, K. W. Brown, W. Reviol, D. Bazin, P. Farris, A. M. Hill, J. Li, B. Longfellow, D. Rhodes, S. N. Paneru, S. A. Gillespie, A. Anthony, E. Rubino,S. Biswas

Physical Review C(2023)

引用 2|浏览0
暂无评分
摘要
The $B(E2,\phantom{\rule{0.16em}{0ex}}{0}_{1}^{+}\ensuremath{\rightarrow}{2}_{1}^{+})$ strengths of $^{36}\mathrm{Ca}$ and $^{38}\mathrm{Ca}$ are measured to be 131(20) ${e}^{2}{\mathrm{fm}}^{4}$ and 101(11) ${e}^{2}{\mathrm{fm}}^{4}$, respectively. The $B(E2)$ value for $^{36}\mathrm{Ca}$ required a measurement of the $p$/$\ensuremath{\gamma}$ branching ratio because the ${2}^{+}$ state is proton unbound. This branching ratio is ${B}_{p}=0.087(8)$. These $B(E2)$ and branching-ratio values can be reproduced in the shell-model with the ZMB2 interaction, an interaction that predicts the $Z=20$ $sd$-shell closure is incomplete with large proton $pf$-shell occupancies in the ground state. These occupancies are at odds with other shell-model and energy-density-functional calculations of $^{36}\mathrm{Ca}$. New data are used to provide an update on constraints of the density dependence of the symmetry energy through mirror charge-radii differences as well as to help reduce uncertainties of the astrophysical important $^{35}\mathrm{K}(p,\ensuremath{\gamma}$) reaction.
更多
查看译文
关键词
<mmlmath xmlnsmml=http//wwww3org/1998/math/mathml><mmlmrow><mmlmi>b</mmlmi><mmlmo></mmlmo><mmlmi>e</mmlmi><mmlmn>2</mmlmn><mmlmo>↑</mmlmo><mmlmo></mmlmo></mmlmrow></mmlmath>,strengths,measurement
AI 理解论文
溯源树
样例
生成溯源树,研究论文发展脉络
Chat Paper
正在生成论文摘要