PARK, J.; KRÜCKEN, R.; BLAZHEV, A.; LUBOS, D.; GERNHÄUSER, R.; LEWITOWICZ, M.; NISHIMURA, S.; AHN, D.; BABA, H.; BLANK, B.; BOUTACHKOV, P.; BROWNE, F.; ČELIKOVIĆ, I.; DE FRANCE, G.; DOORNENBAL, P.; FAESTERMANN, T.; FANG, Y.; FUKUDA, N.; GIOVINAZZO, J.; GOEL, N.; GÓRSKA, M.; GRAWE, H.; ILIEVA, S.; INABE, N.; ISOBE, T.; JUNGCLAUS, A.; KAMEDA, D.; KIM, G.; KIM, Y.-K.; KOJOUHAROV, I.; KUBO, T.; KURZ, N.; KWON, Y.; LORUSSO, G.; MOSCHNER, K.; MURAI, D.; NISHIZUKA, I.; PATEL, Z.; RAJABALI, M.; RICE, S.; SAKURAI, H.; SCHAFFNER, H.; SHIMIZU, Y.; SINCLAIR, L.; SÖDERSTRÖM, P.-A.; STEIGER, K.; SUMIKAMA, T.; SUZUKI, H.; TAKEDA, H.; WANG, Z.; WATANABE, H.; WU, J.; XU, Z.

doi:10.1103/PhysRevC.102.014304

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PARK, J.
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KRÜCKEN, R.

BLAZHEV, A.

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Physical Review C. 2020-07-06, vol. 102, n° 1, p. 014304

American Physical Society

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We report on new γ-ray spectroscopy results from β decays of In99 and Sn101. 30 new γ rays were observed following the β decay of In99, and inconsistencies in the literature with respect to the γ rays following the β decay of Sn101 were addressed with two confirmed cases and two new transitions. The experimental γ-ray energies, intensities, and coincidence relationships are discussed with shell model calculations, where theoretical β-decay branching ratios from the parent nuclei and γ-ray cascades of excited states from the daughter nuclei were combined to generate hypothetical βγ spectra and βγγ coincidence matrices. The most intense β-delayed γ-ray branches in both Cd99 and In101 were well reproduced with this approach, and several γ rays were assigned to new excited states based on their good agreement with shell model predictions. (APS)< Réduire

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Spectroscopy of $^{99}\mathrm{Cd}$ and $^{101}\mathrm{In}$ from ${\beta}$ decays of $^{99}\mathrm{In}$ and $^{101}\mathrm{Sn}$

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