Lifetime measurements of states of S 35 , S 36 , S 37 , and S 38 using the AGATA ? -ray tracking spectrometer
Lifetime measurements of states of S 35 , S 36 , S 37 , and S 38 using the AGATA ? -ray tracking spectrometer
复制标题
使用 AGATA? 对 S 35、S 36、S 37 和 S 38 状态进行寿命测量。
DOI:
10.1103/physrevc.106.024314
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发表时间:
2022
影响因子:
3.1
通讯作者:
Grocutt L
中科院分区:
文献类型:
--
作者:
Grocutt L
Lifetimes or lifetime limits of a small number of excited states of the sulfur isotopes with mass numbers, 36, 37, and 38 have been measured using the differential recoil-distance method. The isotopes of sulfur were populated in binary grazing reactions initiated by a beam ofions of energy 225 MeV incident on a thintarget which was mounted in the Cologne plunger apparatus. The combination of the PRISMA magnetic spectrometer and an early implementation of the AGATA-ray tracking array was used to detectrays in coincidence with projectile-like nuclear species. Lifetime measurements of populated states were measured within the range from about 1 to 100 ps. The number of states for which lifetime measurements or lifetime limits were possible was limited by statistics. For, the lifetime was determined for the firststate at 1572 keV; the result is compared with a previous published lifetime value. The lifetime of thestate ofat 4193 keV was determined and compared with earlier measurements. No previous lifetime information exists for the () state at 6690 keV; a lifetime measurement with large associated error was made in the present work. For, the states for which lifetime limits were established were those at 646 keV withand at 2776 keV with; there are no previously published lifetime values for excited states of. Finally, a lifetime limit was established for thestate ofat 3675 keV; no lifetime information exists for this state in the literature. Measured lifetime values were compared with the results of state-of-the-art shell-model calculations based on the PSDPF, SDPF-U, and FSU effective interactions. In addition, nuclear magnetic-dipole and electric-quadrupole moments, branching ratios, mixing ratios, and electromagnetic transition rates, where available, have been compared with shell-model values. The current work suffers from poor statistics; nevertheless, lifetime values and limits have been possible, allowing a useful discussion of the ability of state-of-the-art shell-model calculations to reproduce the experimental results.