Title:
High spin states in 63Cu

dc.contributor.authorS. Rai
dc.contributor.authorB. Mukherjee
dc.contributor.authorU.S. Ghosh
dc.contributor.authorA. Biswas
dc.contributor.authorA. Chakraborty
dc.contributor.authorA.K. Mondal
dc.contributor.authorS. Chakraborty
dc.contributor.authorG. Mukherjee
dc.contributor.authorI. Bala
dc.contributor.authorS. Muralithar
dc.contributor.authorR.P. Singh
dc.date.accessioned2026-02-07T08:46:52Z
dc.date.issued2018
dc.description.abstractHigh-spin states in 63Cu were investigated through in-beam γ-ray spectroscopic techniques using the 52Cr(18O,αp2n) fusion-evaporation reaction at a beam energy of 72.5 MeV. The γ-rays emitted by the excited nucleus were recorded in the coincidence mode using fourteen Compton suppressed Ge clover detectors of the Indian National Gamma-ray Array (INGA). Based on the γ-γ coincidence data, twenty-one new γ-ray transitions have been observed and placed --thereby extending the level scheme of 63Cu up to spin 25 / 2 ℏ and excitation energy ∼ 8. 36 MeV. Shell model calculations are performed in the f5 / 2pg9 / 2 model space with a 56Ni core using two effective interactions, viz. JUN45 and jj44b to interpret the observed excited states of this nucleus. A reasonable agreement is found between the experimental finding and the shell-model calculations --which implies that the excitations within the f5 / 2p3 / 2p1 / 2 orbitals are more dominant in defining the observed level structure than the excitation across the magic shell gap N= Z= 28. © 2018, SIF, Springer-Verlag GmbH Germany, part of Springer Nature.
dc.identifier.doi10.1140/epja/i2018-12518-2
dc.identifier.issn14346001
dc.identifier.urihttps://doi.org/10.1140/epja/i2018-12518-2
dc.identifier.urihttps://dl.bhu.ac.in/bhuir/handle/123456789/32361
dc.publisherSpringer New York LLC
dc.titleHigh spin states in 63Cu
dc.typePublication
dspace.entity.typeArticle

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