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Identification of significant E 0 strength in the 22+→21+ transitions of 58,60,62 Ni

Authors :
Evitts, L.J.
Garnsworthy, A.B.
Kibédi, T.
Smallcombe, J.
Reed, M.W.
Brown, B.A.
Stuchbery, A.E.
Lane, G.J.
Eriksen, T.K.
Akber, A.
Alshahrani, B.
de Vries, M.
Gerathy, M.S.M.
Holt, J.D.
Lee, B.Q.
McCormick, B.P.
Mitchell, A.J.
Moukaddam, M.
Mukhopadhyay, S.
Palalani, N.
Palazzo, T.
Peters, E.E.
Ramirez, A.P.D.
Stroberg, S.R.
Tornyi, T.
Yates, S.W.
Source :
Physics Letters B
Publication Year :
2018
Publisher :
Elsevier, 2018.

Abstract

The E 0 transition strength in the 22+→21+ transitions of 58,60,62 Ni have been determined for the first time following a series of measurements at the Australian National University (ANU) and the University of Kentucky (UK). The CAESAR Compton-suppressed HPGe array and the Super-e solenoid at ANU were used to measure the δ(E2/M1) mixing ratio and internal conversion coefficient of each transition following inelastic proton scattering. Level half-lives, δ(E2/M1) mixing ratios and γ -ray branching ratios were measured at UK following inelastic neutron scattering. The new spectroscopic information was used to determine the E 0 strengths. These are the first 2+→2+ E 0 transition strengths measured in nuclei with spherical ground states and the E 0 component is found to be unexpectedly large; in fact, these are amongst the largest E 0 transition strengths in medium and heavy nuclei reported to date.

Details

Language :
English
Database :
OpenAIRE
Journal :
Physics Letters B
Accession number :
edsair.od......3000..e8439e5a820226a10669231d0908a8fb