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Beta-decay half-lives of 110 neutron-rich nuclei across the N=82 shell gap: implications for the mechanism and universality of the astrophysical r process.

Lorusso, G; Nishimura, S*; Xu, Z Y*; Jungclaus, A*; Shimizu, Y*; Simpson, G S*; Soderstrom, P A*; Watanabe, H*; Browne, F*; Doornenbal, P*; Gey, G*; Jung, H S*; Meyer, B*; Sumikama, T*; Taprogge, J*; Vajta, Z*; Wu, J*; Baba, H*; Benzoni, G*; Chae, K Y*; Crespi, F C L*; Fukuda, N*; Gernhauser, R*; Inabe, N*; Kajino, T*; Kameda, D*; Kim, G D*; Kim, Y K*; Kojouharov, I*; Kondev, F G*; Kubo, T*; Kurz, N*; Kwon, Y K*; Lane, G J*; Li, Z*; Montaner-Piza, A*; Moschner, K*; Naqvi, F*; Niikura, M*; Nishibata, H*; Odahara, A*; Patel, Z*; Podolyak, Z*; Sakurai, H*; Schaffner, H*; Schury, P*; Shibagaki, S*; Steiger, K*; Suzuki, H*; Takeda, H*; Wendt, A*; Yagi, A*; Yoshinaga, K* (2015) Beta-decay half-lives of 110 neutron-rich nuclei across the N=82 shell gap: implications for the mechanism and universality of the astrophysical r process. Phys. Rev. Lett., 114 (19). 192501

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Abstract

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Item Type: Article
Subjects: Ionising Radiation
Ionising Radiation > Radioactivity
Identification number/DOI: 10.1103/PhysRevLett.114.192501
Last Modified: 02 Feb 2018 13:13
URI: http://eprintspublications.npl.co.uk/id/eprint/6665

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