Bulletin of the American Physical Society
5th Joint Meeting of the APS Division of Nuclear Physics and the Physical Society of Japan
Volume 63, Number 12
Tuesday–Saturday, October 23–27, 2018; Waikoloa, Hawaii
Session MM: Nuclear Structure A=30-60
2:00 PM–4:45 PM,
Saturday, October 27, 2018
Hilton
Room: Queen's 6
Chair: Adam Fritsch, Gonzaga University
Abstract ID: BAPS.2018.HAW.MM.1
Abstract: MM.00001 : Shell-model Interpretation of the Intruder States in 38Cl *
2:00 PM–2:15 PM
Presenter:
Rebeka Sultana Lubna
(Florida State Univ)
Authors:
Rebeka Sultana Lubna
(Florida State Univ)
Konstantinos Kravvaris
(Florida State Univ)
Samuel L Tabor
(Florida State Univ)
Vandana Tripathi
(Florida State Univ)
Alexander Volya
(Florida State Univ)
Elizabeth Rubino
(Florida State Univ)
Maria Anastasiou
(Florida State Univ)
Benjamin Asher
(Florida State Univ)
Lagy T Baby
(Florida State Univ)
Jonathan Baron
(Florida State Univ)
David Dwaine Caussyn
(Florida State Univ)
David Clarke
(Florida State Univ)
Jesus Perello
(Florida State Univ)
Nabin Rijal
(Florida State University)
Kalisa Villafana
(Florida State University)
James Allmond
(Oak Ridge National Lab)
The excited states in 38Cl were populated by the 26Mg(18O, αpnγ)38Cl fusion evaporation reaction at Elab=50 MeV in John. D. Fox laboratory, Florida State University. The experimental observations have been interpreted by shell model calculations using FSU-A interaction, currently being developed by our group [1]. In this interaction, we have chosen the approach of fitting experimental data started from an existing interaction. The single particle energies of the fp shell orbitals along with the monopole terms from the sd-pf cross shell two body matrix elements were adjusted to fit the experimental data compiled from the nuclei ranging from 23Ne to 40K. The interaction well explains 0hbarΩ and 1hbarΩ states in 38Cl. FSU-A also predicts 0p-0h and 1p-1h states of the nearby isotopes which will also be discussed along with future plans to refine this interaction to make it more universal.
[1] R. S. Lubna, K. Kravvaris, A. Volya, S.L. Tabor, V. Tripathi
*This material is based upon in part of the works supported by the U.S. National Science Foundation under grant No. PHY-1401574(FSU) and PHY-1712953(FSU) and by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics under contract No. DE-SC-0009883(FSU) and DE-C05-00OR22725(ORNL).\\
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.HAW.MM.1
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