Prompt-delayed γ-ray spectroscopy of neutron-rich 119.121In isotopes
Abstract
The Z = 50 shell closure, near N = 82, is unique in the sense that it is the only shell closure with the spin-orbit partner orbitals, and , enclosing the magic gap. The interaction of the proton hole/particle in the above-mentioned orbitals with neutrons in the νh11/2 orbital is an important prerequisite to the understanding of the nuclear structure near N = 82 and the νπ interaction. To explore the structural similarity between the high-spin isomeric states in In (Z = 49), Sn (Z = 50), and Sb (Z = 51) isotopes from a microscopic point of view. In addition, to understand the role of a proton hole or particle in the spin-orbit partner orbitals, and , respectively, with neutron holes in the orbital on these aforementioned isomers. The fusion and transfer induced fission reaction with 6.2 MeV/u beam energy, using a unique setup consisting of AGATA, VAMOS++, and EXOGAM detectors, was used to populate through the fission process and study the neutron-rich isotopes. This setup enabled the prompt-delayed -ray spectroscopy of isotopes in the time range of . In the odd- isotopes, indications of a short half-life 19/2- isomeric state, in addition to the previously known 25/2+ isomeric state, were observed from the present data. Further, new prompt transitions above the 25/2+ isomer in were identified along with reevaluation of its half-life. The experimental data were compared with the theoretical results obtained in the framework of large-scale shell-model calculations in a restricted model space. Furthermore, the two-body matrix elements of residual interaction were modified to explain the excitation energies and the B(E2) transition probabilities in the neutron-rich In isotopes. The (i) decreasing trend of E (29/2+) - E (25/2+) in odd-In (with dominant configuration and maximum aligned spin of 29/2+) and (ii) increasing trend of E (27/2+) - E (23/2+) in odd-Sb (with dominant configuration and maximum aligned spin of 27/2+) with increasing neutron number could be understood as a consequence of hole-hole and particle-hole interactions, respectively.
- Authors:
-
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- Centre National de la Recherche Scientifique (CNRS), Caen (France). Centre de Recherche sur les Ions, les Matériaux et la Photonique (CIMAP), Grand Accelerateur National d'Ions Lourds (GANIL)
- Centre National de la Recherche Scientifique (CNRS), Caen (France). Centre de Recherche sur les Ions, les Matériaux et la Photonique (CIMAP), Grand Accelerateur National d'Ions Lourds (GANIL); Inst. Laue-Langevin, Grenoble (France)
- Univ. Paris-Saclay (France). IJCLab; Centre National de la Recherche Scientifique (CNRS), Paris (France). Inst. National de Physique Nucleaire et de Physique des Particules (IN2P3)
- Variable Energy Cyclotron Centre, Kolkata (India); Homi Bhabha National Inst., Mumbai (India)
- Inst. of Nuclear Physics (PAN), Krakow (Poland)
- Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
- Tata Inst. of Fundamental Research, Mumbai (India)
- Spanish National Research Council (CSIC) and Univ. of Valencia (Spain). Inst. de Fisica Corpuscular
- Publication Date:
- Research Org.:
- Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), Nuclear Physics (NP); Polish National Science Centre (NCN); Ministry of Science, Spain
- OSTI Identifier:
- 1783105
- Grant/Contract Number:
- AC02-05CH11231; 2016/22/M/ST2/00269; BES-2012-061407; SEV-2014-0398; FPA2017-84756-C4
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Physical Review C
- Additional Journal Information:
- Journal Volume: 102; Journal Issue: 1; Journal ID: ISSN 2469-9985
- Publisher:
- American Physical Society (APS)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 73 NUCLEAR PHYSICS AND RADIATION PHYSICS; Electromagnetic transitions; energy levels & level densities; isomer decays; lifetimes & widths; nuclear structure & decays; radiation detectors; shell model; spectrometers & spectroscopic techniques
Citation Formats
Biswas, S., Lemasson, A., Rejmund, M., Navin, A., Kim, Y. H., Michelagnoli, C., Stefan, I., Banik, R., Bednarczyk, P., Bhattacharya, Soumik, Bhattacharyya, S., Clément, E., Crawford, H. L., de France, G., Fallon, P., Frémont, G., Goupil, J., Jacquot, B., Li, H. J., Ljungvall, J., Maj, A., Ménager, L., Morel, V., Palit, R., Pérez-Vidal, R. M., and Ropert, J. Prompt-delayed γ-ray spectroscopy of neutron-rich 119.121In isotopes. United States: N. p., 2020.
Web. doi:10.1103/physrevc.102.014326.
Biswas, S., Lemasson, A., Rejmund, M., Navin, A., Kim, Y. H., Michelagnoli, C., Stefan, I., Banik, R., Bednarczyk, P., Bhattacharya, Soumik, Bhattacharyya, S., Clément, E., Crawford, H. L., de France, G., Fallon, P., Frémont, G., Goupil, J., Jacquot, B., Li, H. J., Ljungvall, J., Maj, A., Ménager, L., Morel, V., Palit, R., Pérez-Vidal, R. M., & Ropert, J. Prompt-delayed γ-ray spectroscopy of neutron-rich 119.121In isotopes. United States. https://doi.org/10.1103/physrevc.102.014326
Biswas, S., Lemasson, A., Rejmund, M., Navin, A., Kim, Y. H., Michelagnoli, C., Stefan, I., Banik, R., Bednarczyk, P., Bhattacharya, Soumik, Bhattacharyya, S., Clément, E., Crawford, H. L., de France, G., Fallon, P., Frémont, G., Goupil, J., Jacquot, B., Li, H. J., Ljungvall, J., Maj, A., Ménager, L., Morel, V., Palit, R., Pérez-Vidal, R. M., and Ropert, J. Wed .
"Prompt-delayed γ-ray spectroscopy of neutron-rich 119.121In isotopes". United States. https://doi.org/10.1103/physrevc.102.014326. https://www.osti.gov/servlets/purl/1783105.
@article{osti_1783105,
title = {Prompt-delayed γ-ray spectroscopy of neutron-rich 119.121In isotopes},
author = {Biswas, S. and Lemasson, A. and Rejmund, M. and Navin, A. and Kim, Y. H. and Michelagnoli, C. and Stefan, I. and Banik, R. and Bednarczyk, P. and Bhattacharya, Soumik and Bhattacharyya, S. and Clément, E. and Crawford, H. L. and de France, G. and Fallon, P. and Frémont, G. and Goupil, J. and Jacquot, B. and Li, H. J. and Ljungvall, J. and Maj, A. and Ménager, L. and Morel, V. and Palit, R. and Pérez-Vidal, R. M. and Ropert, J.},
abstractNote = {The Z = 50 shell closure, near N = 82, is unique in the sense that it is the only shell closure with the spin-orbit partner orbitals, πg9/2 and πg7/2, enclosing the magic gap. The interaction of the proton hole/particle in the above-mentioned orbitals with neutrons in the νh11/2 orbital is an important prerequisite to the understanding of the nuclear structure near N = 82 and the νπ interaction. To explore the structural similarity between the high-spin isomeric states in In (Z = 49), Sn (Z = 50), and Sb (Z = 51) isotopes from a microscopic point of view. In addition, to understand the role of a proton hole or particle in the spin-orbit partner orbitals, πg9/2 and πg7/2, respectively, with neutron holes in the νh11/2 orbital on these aforementioned isomers. The fusion and transfer induced fission reaction Be9(U238, f) with 6.2 MeV/u beam energy, using a unique setup consisting of AGATA, VAMOS++, and EXOGAM detectors, was used to populate through the fission process and study the neutron-rich In119,121 isotopes. This setup enabled the prompt-delayed γ-ray spectroscopy of isotopes in the time range of 100ns–200μs. In the odd-AIn119,121 isotopes, indications of a short half-life 19/2- isomeric state, in addition to the previously known 25/2+ isomeric state, were observed from the present data. Further, new prompt transitions above the 25/2+ isomer in In121 were identified along with reevaluation of its half-life. The experimental data were compared with the theoretical results obtained in the framework of large-scale shell-model calculations in a restricted model space. Furthermore, the (πg9/2νh11/2;I|H^|πg9/2νh11/2;I) two-body matrix elements of residual interaction were modified to explain the excitation energies and the B(E2) transition probabilities in the neutron-rich In isotopes. The (i) decreasing trend of E (29/2+) - E (25/2+) in odd-In (with dominant configuration πg9/2-1νh11/2-2 and maximum aligned spin of 29/2+) and (ii) increasing trend of E (27/2+) - E (23/2+) in odd-Sb (with dominant configuration πg7/2+1νh11/2-2 and maximum aligned spin of 27/2+) with increasing neutron number could be understood as a consequence of hole-hole and particle-hole interactions, respectively.},
doi = {10.1103/physrevc.102.014326},
journal = {Physical Review C},
number = 1,
volume = 102,
place = {United States},
year = {Wed Jul 29 00:00:00 EDT 2020},
month = {Wed Jul 29 00:00:00 EDT 2020}
}
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