Structure of nearly degenerate dipole bands in Ag
Sethi, J, Palit, R, Saha, S, Trivedi, T, Donthi, R, Jadhav, S, Jain, HC, Naidu, BS, Bhat, GH, Sheikh, JA, Datta, P, Carroll, JJ, Litz, MS, Chattopadhyay, S, Garg, U, Karamian, S, Kumar, S, Mehta, D, Sihotra, S, Naik, Z and Walker, PM (2013) Structure of nearly degenerate dipole bands in Ag Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, 725 (1-3). pp. 85-91.
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The high spin negative parity states of Ag have been investigated with the B+Mo reaction at 39 MeV beam energy using the INGA facility at TIFR, Mumbai. From the γ-γ coincidence analysis, an excited negative parity band has been established and found to be nearly degenerate with the ground state band. The spin and parity of the levels are assigned using angular correlation and polarization measurements. This pair of degenerate bands in Ag is studied using the recently developed microscopic triaxial projected shell model approach. The observed energy levels and the ratio of the electromagnetic transition probabilities of these bands in this isotope are well reproduced by the present model. Further, it is shown that the partner band has a different quasiparticle structure as compared to the yrast band. © 2013 Elsevier B.V.
|Divisions :||Faculty of Engineering and Physical Sciences > Physics|
|Identification Number :||https://doi.org/10.1016/j.physletb.2013.06.054|
|Additional Information :||NOTICE: this is the author’s version of a work that was accepted for publication in Physics Letters, Section B. Changes resulting from the publishing process, such as peer review, editing, corrections, structural formatting, and other quality control mechanisms may not be reflected in this document. Changes may have been made to this work since it was submitted for publication. A definitive version was subsequently published in Physics Letters, Section B, 725(1-3), August 2013, DOI 10.1016/j.physletb.2013.06.054.|
|Depositing User :||Symplectic Elements|
|Date Deposited :||27 Sep 2013 17:33|
|Last Modified :||09 Jun 2014 13:41|
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