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arXiv 1612.04697nucl-ex
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Search for $2p$ decay of the first excited state of $^{17}$Ne

P. G. Sharov, A. A. Bezbakh, V. Chudoba, A. S. Fomichev, M. S. Golovkov, A. V. Gorshkov, L. V. Grigorenko, G. Kaminski, A. G. Knyazev, S. A. Krupko, M. Mentel, … 展开作者

P. G. Sharov, A. A. Bezbakh, V. Chudoba, A. S. Fomichev, M. S. Golovkov, A. V. Gorshkov, L. V. Grigorenko, G. Kaminski, A. G. Knyazev, S. A. Krupko, M. Mentel, E. Yu. Nikolskii, Yu. L. Parfenova, P. Pluchinski, S. A. Rymzhanova, S. I. Sidorchuk, R. S. Slepnev, S. V. Stepantsov, G. M. Ter-Akopian, R. Wolski, M. V. Zhukov

英文摘要:

Two-proton decay of the $^{17}$Ne low-lying states populated in the $^1$H($^{18}$Ne,$d$)$^{17}$Ne transfer reaction was studied. The two-proton width $Γ_{2p}$ of the $^{17}$Ne first excited $3/2^-$ state at $E^*=1.288$ MeV is of importance for the two-proton radioactivity theory and nuclear-astrophysics applications. A dedicated search for the two-proton emission of this state was performed leading to the new upper limit obtained for the width ratio $Γ_{2p}/Γ_γ < 1.6(3) \times 10^{-4}$. A novel, "combined mass" method is suggested and tested capable to improve the resolution of the experiment which is a prime significance for the study of nuclear states with extremely small particle-to-gamma width ratios $Γ_{\mathrm{part}}/Γ_γ$. The condition $Γ_{\mathrm{part}} \ll Γ_γ$ is quite common for the states of astrophysical interest which makes the proposed approach promising in this field.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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