Nuclear structure of Te isotopes beyond neutron magic number N=82

B. Moon; A. Jungclaus; H. Naïdja; A. Gargano; R. Lozeva; C.-B. Moon; A. Odahara; G. S. Simpson; S. Nishimura; F. Browne; P. Doornenbal; G. Gey; J. Keatings; G. Lorusso; Z. Patel; S. Rice; M. Si; L. Sinclair; P. A. Söderström; T. Sumikama; J. Taprogge; H. Watanabe; J. Wu; Z. Y. Xu; A. Yagi; D. S. Ahn; H. Baba; F. L. Bello Garrote; S. Bönig; R. Daido; J. M. Daugas; F. Didierjean; F. Drouet; Y. Fang; N. Fukuda; R. Gernhäuser; B. Hong; E. Ideguchi; S. Ilieva; N. Inabe; T. Ishigaki; T. Isobe; H. S. Jung; D. Kameda; I. Kojouharov; T. Komatsubara; T. Kröll; T. Kubo; N. Kurz; Y. K. Kwon; C. S. Lee; P. Lee; Z. Li; A. Montaner-Pizá; S. Morimoto; K. Moschner; D. Mücher; D. Murai; M. Niikura; H. Nishibata; I. Nishizuka; R. Orlandi; H. Sakurai; H. Schaffner; Y. Shimizu; K. Steiger; H. Suzuki; H. Takeda; K. Tshoo; Zs. Vajta; A. Wendt; R. Yokoyama; K. Yoshinaga

doi:10.1103/PhysRevC.103.034320

Nuclear structure of Te isotopes beyond neutron magic number N=82

B. Moon
, A. Jungclaus^*
, H. Naïdja
, A. Gargano
, R. Lozeva
, C.-B. Moon^*
, A. Odahara
, G. S. Simpson
, S. Nishimura
, F. Browne
, P. Doornenbal
, G. Gey
, J. Keatings
, G. Lorusso
, Z. Patel
, S. Rice
, M. Si
, L. Sinclair
, P. A. Söderström
, T. Sumikama

J. Taprogge, H. Watanabe, J. Wu, Z. Y. Xu, A. Yagi, D. S. Ahn, H. Baba, F. L. Bello Garrote, S. Bönig, R. Daido, J. M. Daugas, F. Didierjean, F. Drouet, Y. Fang, N. Fukuda, R. Gernhäuser, B. Hong, E. Ideguchi, S. Ilieva, N. Inabe, T. Ishigaki, T. Isobe, H. S. Jung, D. Kameda, I. Kojouharov, T. Komatsubara, T. Kröll, T. Kubo, N. Kurz, Y. K. Kwon, C. S. Lee, P. Lee, Z. Li, A. Montaner-Pizá, S. Morimoto, K. Moschner, D. Mücher, D. Murai, M. Niikura, H. Nishibata, I. Nishizuka, R. Orlandi, H. Sakurai, H. Schaffner, Y. Shimizu, K. Steiger, H. Suzuki, H. Takeda, K. Tshoo, Zs. Vajta, A. Wendt, R. Yokoyama, K. Yoshinaga

^*Corresponding author for this work

Research output: Contribution to journal › Article › peer-review

7 Citations (Scopus)

40 Downloads (Pure)

Abstract

Newly observed decay schemes of the nuclei ¹³⁷Sb and ¹³⁸Sb are reported. The neutron-rich Sb isotopes were produced by the in-flight fragmentation of a 238U primary beam with an energy of 345 MeV/nucleon. Several new excited states of ¹³⁷Te with tentatively assigned spin-parities of (5/2^-), (9/2^-), and (7/2) have been established which play an important role in the evolution of neutron levels beyond N=82. The study of the ß decay of ¹³⁸Sb led to a considerable extension of the level scheme of ¹³⁸Te including the identification of several nonyrast states. The structure of ¹³⁷Te and ¹³⁸Te is discussed on the basis of large-scale shell-model calculations performed using two different effective interactions.

Original language	English
Article number	034320
Journal	Physical Review C
Volume	103
Issue number	3
DOIs	https://doi.org/10.1103/PhysRevC.103.034320
Publication status	Published - 24 Mar 2021

Access to Document

10.1103/PhysRevC.103.034320

2021 03 03 Moon et al Nuclear acceptedAccepted author manuscript, 3.72 MB

Cite this

Moon, B., Jungclaus, A., Naïdja, H., Gargano, A., Lozeva, R., Moon, C.-B., Odahara, A., Simpson, G. S., Nishimura, S., Browne, F., Doornenbal, P., Gey, G., Keatings, J., Lorusso, G., Patel, Z., Rice, S., Si, M., Sinclair, L., Söderström, P. A., ... Yoshinaga, K. (2021). Nuclear structure of Te isotopes beyond neutron magic number N=82. Physical Review C, 103(3), Article 034320. https://doi.org/10.1103/PhysRevC.103.034320

@article{61520600274048fa914b96f403cd8b9c,

title = "Nuclear structure of Te isotopes beyond neutron magic number N=82",

abstract = "Newly observed decay schemes of the nuclei 137Sb and 138Sb are reported. The neutron-rich Sb isotopes were produced by the in-flight fragmentation of a 238U primary beam with an energy of 345 MeV/nucleon. Several new excited states of 137Te with tentatively assigned spin-parities of (5/2-), (9/2-), and (7/2) have been established which play an important role in the evolution of neutron levels beyond N=82. The study of the {\ss} decay of 138Sb led to a considerable extension of the level scheme of 138Te including the identification of several nonyrast states. The structure of 137Te and 138Te is discussed on the basis of large-scale shell-model calculations performed using two different effective interactions. ",

author = "B. Moon and A. Jungclaus and H. Na{\"i}dja and A. Gargano and R. Lozeva and C.-B. Moon and A. Odahara and Simpson, \{G. S.\} and S. Nishimura and F. Browne and P. Doornenbal and G. Gey and J. Keatings and G. Lorusso and Z. Patel and S. Rice and M. Si and L. Sinclair and S{\"o}derstr{\"o}m, \{P. A.\} and T. Sumikama and J. Taprogge and H. Watanabe and J. Wu and Xu, \{Z. Y.\} and A. Yagi and Ahn, \{D. S.\} and H. Baba and \{Bello Garrote\}, \{F. L.\} and S. B{\"o}nig and R. Daido and Daugas, \{J. M.\} and F. Didierjean and F. Drouet and Y. Fang and N. Fukuda and R. Gernh{\"a}user and B. Hong and E. Ideguchi and S. Ilieva and N. Inabe and T. Ishigaki and T. Isobe and Jung, \{H. S.\} and D. Kameda and I. Kojouharov and T. Komatsubara and T. Kr{\"o}ll and T. Kubo and N. Kurz and Kwon, \{Y. K.\} and Lee, \{C. S.\} and P. Lee and Z. Li and A. Montaner-Piz{\'a} and S. Morimoto and K. Moschner and D. M{\"u}cher and D. Murai and M. Niikura and H. Nishibata and I. Nishizuka and R. Orlandi and H. Sakurai and H. Schaffner and Y. Shimizu and K. Steiger and H. Suzuki and H. Takeda and K. Tshoo and Zs. Vajta and A. Wendt and R. Yokoyama and K. Yoshinaga",

note = "Funding Information: This work was carried out at the RIBF operated by RIKEN Nishina Center and CNS, University of Tokyo. We acknowledge the EUROBALL Owners Committee for the loan of germanium detectors and the PreSpec Collaboration for the readout electronics of the cluster detectors. Part of the WAS3ABi was supported by the Rare Isotope Science Project (RISP) of the Institute for Basic Science (IBS) funded by the Ministry of Science, ICT and Future Planning (MSIP) and National Research Foundation (NRF) of the Republic of Korea (Grant No. 2013M7A1A1075764). This research was supported by NRF of the Republic of Korea (Grants No. 2019R1A6A3A03031564 and No. 2018R1A5A1025563), IBS of the Republic of Korea (Grants No. IBS-R031-D1 and No. IBS-R031-Y1), the Spanish Ministerio de Econom{\'i}a y Competitividad (Grant No. FPA2017-84756-C4-2-P), and JSPS KAKENHI of Japan (Grant No. 25247045). The support from FR-JP LIA is also acknowledged. C.S.L. acknowledges the support from NRF of the Republic of Korea (Grants No. 2017M2A2A6A02071071 and No. 2016R1D1A1A09917463). Z.V. acknowledges the supports from the National Research, Development and Innovation Fund of Hungary, financed under the K18 funding scheme with Project No. K128947 and by the European Regional Development Fund (Grant No. GINOP-2.3.3-15-2016-00034), as well as by the National Research, Development and Innovation Office NKFIH (Grant No. PD 124717). H.N. is grateful to F. Nowacki for sharing the NATHAN code used in the seniority part. Publisher Copyright: {\textcopyright}2021 American Physical Society. Copyright: Copyright 2021 Elsevier B.V., All rights reserved.",

year = "2021",

month = mar,

day = "24",

doi = "10.1103/PhysRevC.103.034320",

language = "English",

volume = "103",

journal = "Physical Review C",

issn = "2469-9985",

publisher = "American Physical Society",

number = "3",

}

Moon, B, Jungclaus, A, Naïdja, H, Gargano, A, Lozeva, R, Moon, C-B, Odahara, A, Simpson, GS, Nishimura, S, Browne, F, Doornenbal, P, Gey, G, Keatings, J, Lorusso, G, Patel, Z, Rice, S, Si, M, Sinclair, L, Söderström, PA, Sumikama, T, Taprogge, J, Watanabe, H, Wu, J, Xu, ZY, Yagi, A, Ahn, DS, Baba, H, Bello Garrote, FL, Bönig, S, Daido, R, Daugas, JM, Didierjean, F, Drouet, F, Fang, Y, Fukuda, N, Gernhäuser, R, Hong, B, Ideguchi, E, Ilieva, S, Inabe, N, Ishigaki, T, Isobe, T, Jung, HS, Kameda, D, Kojouharov, I, Komatsubara, T, Kröll, T, Kubo, T, Kurz, N, Kwon, YK, Lee, CS, Lee, P, Li, Z, Montaner-Pizá, A, Morimoto, S, Moschner, K, Mücher, D, Murai, D, Niikura, M, Nishibata, H, Nishizuka, I, Orlandi, R, Sakurai, H, Schaffner, H, Shimizu, Y, Steiger, K, Suzuki, H, Takeda, H, Tshoo, K, Vajta, Z, Wendt, A, Yokoyama, R & Yoshinaga, K 2021, 'Nuclear structure of Te isotopes beyond neutron magic number N=82', Physical Review C, vol. 103, no. 3, 034320. https://doi.org/10.1103/PhysRevC.103.034320

TY - JOUR

T1 - Nuclear structure of Te isotopes beyond neutron magic number N=82

AU - Moon, B.

AU - Jungclaus, A.

AU - Naïdja, H.

AU - Gargano, A.

AU - Lozeva, R.

AU - Moon, C.-B.

AU - Odahara, A.

AU - Simpson, G. S.

AU - Nishimura, S.

AU - Browne, F.

AU - Doornenbal, P.

AU - Gey, G.

AU - Keatings, J.

AU - Lorusso, G.

AU - Patel, Z.

AU - Rice, S.

AU - Si, M.

AU - Sinclair, L.

AU - Söderström, P. A.

AU - Sumikama, T.

AU - Taprogge, J.

AU - Watanabe, H.

AU - Wu, J.

AU - Xu, Z. Y.

AU - Yagi, A.

AU - Ahn, D. S.

AU - Baba, H.

AU - Bello Garrote, F. L.

AU - Bönig, S.

AU - Daido, R.

AU - Daugas, J. M.

AU - Didierjean, F.

AU - Drouet, F.

AU - Fang, Y.

AU - Fukuda, N.

AU - Gernhäuser, R.

AU - Hong, B.

AU - Ideguchi, E.

AU - Ilieva, S.

AU - Inabe, N.

AU - Ishigaki, T.

AU - Isobe, T.

AU - Jung, H. S.

AU - Kameda, D.

AU - Kojouharov, I.

AU - Komatsubara, T.

AU - Kröll, T.

AU - Kubo, T.

AU - Kurz, N.

AU - Kwon, Y. K.

AU - Lee, C. S.

AU - Lee, P.

AU - Li, Z.

AU - Montaner-Pizá, A.

AU - Morimoto, S.

AU - Moschner, K.

AU - Mücher, D.

AU - Murai, D.

AU - Niikura, M.

AU - Nishibata, H.

AU - Nishizuka, I.

AU - Orlandi, R.

AU - Sakurai, H.

AU - Schaffner, H.

AU - Shimizu, Y.

AU - Steiger, K.

AU - Suzuki, H.

AU - Takeda, H.

AU - Tshoo, K.

AU - Vajta, Zs.

AU - Wendt, A.

AU - Yokoyama, R.

AU - Yoshinaga, K.

N1 - Funding Information: This work was carried out at the RIBF operated by RIKEN Nishina Center and CNS, University of Tokyo. We acknowledge the EUROBALL Owners Committee for the loan of germanium detectors and the PreSpec Collaboration for the readout electronics of the cluster detectors. Part of the WAS3ABi was supported by the Rare Isotope Science Project (RISP) of the Institute for Basic Science (IBS) funded by the Ministry of Science, ICT and Future Planning (MSIP) and National Research Foundation (NRF) of the Republic of Korea (Grant No. 2013M7A1A1075764). This research was supported by NRF of the Republic of Korea (Grants No. 2019R1A6A3A03031564 and No. 2018R1A5A1025563), IBS of the Republic of Korea (Grants No. IBS-R031-D1 and No. IBS-R031-Y1), the Spanish Ministerio de Economía y Competitividad (Grant No. FPA2017-84756-C4-2-P), and JSPS KAKENHI of Japan (Grant No. 25247045). The support from FR-JP LIA is also acknowledged. C.S.L. acknowledges the support from NRF of the Republic of Korea (Grants No. 2017M2A2A6A02071071 and No. 2016R1D1A1A09917463). Z.V. acknowledges the supports from the National Research, Development and Innovation Fund of Hungary, financed under the K18 funding scheme with Project No. K128947 and by the European Regional Development Fund (Grant No. GINOP-2.3.3-15-2016-00034), as well as by the National Research, Development and Innovation Office NKFIH (Grant No. PD 124717). H.N. is grateful to F. Nowacki for sharing the NATHAN code used in the seniority part. Publisher Copyright: ©2021 American Physical Society. Copyright: Copyright 2021 Elsevier B.V., All rights reserved.

PY - 2021/3/24

Y1 - 2021/3/24

N2 - Newly observed decay schemes of the nuclei 137Sb and 138Sb are reported. The neutron-rich Sb isotopes were produced by the in-flight fragmentation of a 238U primary beam with an energy of 345 MeV/nucleon. Several new excited states of 137Te with tentatively assigned spin-parities of (5/2-), (9/2-), and (7/2) have been established which play an important role in the evolution of neutron levels beyond N=82. The study of the ß decay of 138Sb led to a considerable extension of the level scheme of 138Te including the identification of several nonyrast states. The structure of 137Te and 138Te is discussed on the basis of large-scale shell-model calculations performed using two different effective interactions.

AB - Newly observed decay schemes of the nuclei 137Sb and 138Sb are reported. The neutron-rich Sb isotopes were produced by the in-flight fragmentation of a 238U primary beam with an energy of 345 MeV/nucleon. Several new excited states of 137Te with tentatively assigned spin-parities of (5/2-), (9/2-), and (7/2) have been established which play an important role in the evolution of neutron levels beyond N=82. The study of the ß decay of 138Sb led to a considerable extension of the level scheme of 138Te including the identification of several nonyrast states. The structure of 137Te and 138Te is discussed on the basis of large-scale shell-model calculations performed using two different effective interactions.

UR - https://www.scopus.com/pages/publications/85104243153

U2 - 10.1103/PhysRevC.103.034320

DO - 10.1103/PhysRevC.103.034320

M3 - Article

AN - SCOPUS:85104243153

SN - 2469-9985

VL - 103

JO - Physical Review C

JF - Physical Review C

IS - 3

M1 - 034320

ER -

Nuclear structure of Te isotopes beyond neutron magic number N=82

Abstract

Access to Document

Other files and links

Fingerprint

Cite this