First determination of $\beta$-delayed multiple neutron emission beyond A = 100 through direct neutron measurement: The P$_{2n}$ value of $^{136}$Sb
R. Caballero-Folch, I. Dillmann, J. Agramunt, J.L. Ta\'in, A. Algora,, J. \"Ayst\"o, F. Calvi\~no, L. Canete, G. Cort\`es, C. Domingo-Pardo, T., Eronen, E. Ganioglu, W. Gelletly, D. Gorelov, V. Guadilla, J. Hakala, A., Jokinen, A. Kankainen, V. Kolhinen, J. Koponen, M. Marta

TL;DR
This study reports the first direct measurement of the two-neutron emission probability (P2n) for the heavy, neutron-rich isotope 136Sb, providing crucial data for nuclear models and astrophysical r-process understanding.
Contribution
It presents the first direct measurement of P2n for 136Sb beyond A=100, testing theoretical predictions and improving nuclear decay data for heavy neutron-rich nuclei.
Findings
P2n of 136Sb is 0.14(3)%
P1n of 136Sb is 32.2(15)%
P2n is 44 times smaller than model predictions
Abstract
Background: -delayed multiple neutron emission has been observed for some nuclei with A100, with Rb being the heaviest 2n emitter measured to date. So far, only 25 P values have been determined for the 300 nuclei that may decay in this way. Accordingly, it is of interest to measure P values for the other possible multiple neutron emitters throughout the chart of the nuclides. It is of particular interest to make such measurement for nuclei with A100 to test the predictions of theoretical models and simulation tools for the decays of heavy nuclei in the region of very neutron-rich nuclei. In addition, the decay properties of these nuclei are fundamental for the understanding of astrophysical nucleosynthesis processes such as the -process, and safety inputs for nuclear reactors. Purpose: To determine for the first time the two neutron…
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