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arXiv · 1810.07089

Half-Lives of Neutron Rich $^{130}$Cd and $^{131}$In

Abstract

The half-lives of isotopes around the $N=82$ shell closure are an important ingredient in astrophysical simulations and strongly influence the magnitude of the second $r$-process abundance peak in the $A\sim130$ region. The most neutron-rich $N=82$ nuclei are not accessible to the current generation of radioactive beam facilities and $r$-process simulations must therefore rely on calculations of the half-lives of the isotopes involved. Half-life measurements of the experimentally accessible nuclei in this region are important in order to benchmark these calculations. The half-life of $^{130}$Cd is particularly important as it is used to tune the Gamow-Teller quenching in shell-model calculations for the $\beta$ decay of other nuclei in this region. In this work, the GRIFFIN $\gamma$-ray spectrometer at the TRIUMF-ISAC facility was used to measure the half-life of $^{130}_{~48}$Cd$_{82}$ to be $T_{1/2}= 126(4)$ ms. In addition, the half-lives of the three $\beta$ decaying states of $^{131}_{~49}$In$_{82}$ were measured to be $T_{1/2}(1/2^-)=328(15)$ ms, $T_{1/2}(9/2^+)=265(8)$ ms, and $T_{1/2}(21/2^+)=323(50)$ ms, respectively, providing an important benchmark for half-life calculations in this region.

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R. Dunlop, C. E. Svensson, C. Andreoiu, G. C. Ball, N. Bernier, V. Bildstein, H. Bidaman, P. Boubel, C. Burbadge, R. Caballero-Folch, I. Dillmann, M. R. Dunlop, L. J. Evitts, F. H. Garcia, A. B. Garnsworthy, P. E. Garrett, G. Hackman, S. Hallam, J. Henderson, S. Ilyushkin, A. Jungclaus, R. Krücken, J. Lassen, R. Li, E. MacConnachie, A. D. MacLean, E. McGee, M. Moukaddam, D. Mücher, B. Olaizola, K. Ortner, E. Padilla-Rodal, J. Park, O. Paetkau, J. L. Pore, A. J. Radich, P. Ruotsalainen, J. Smallcombe, J. K. Smith, A. Teigelhöfer, J. Turko, K. Whitmore, T. Zidar. 2018-10-16. Half-Lives of Neutron Rich $^{130}$Cd and $^{131}$In. https://arxiv.org/abs/1810.07089

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