2004
DOI: 10.1103/physrevc.70.029902
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Publisher’s Note: Shape coexistence and band crossings inPt174[Phys. Rev. C70, 014309 (2004)]

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Cited by 6 publications
(6 citation statements)
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“…More recently, Joss et al [61] studied the neutron-deficient 169−173 Pt nuclei obtaining more detailed information on the yrast bands for mass A = 170 and A = 172, and obtaining first information on side bands. Extra information on 174 Pt [62] and 178 Pt [63] has been obtained making use of the Gammasphere array, in particular, extending the yrast band up to spins (26 + ) and (24 + ), respectively. The yrast band in 178 Pt was extended by Soramel et al [64] up to spin (18 + ) using fusion-evaporation reactions.…”
Section: The Experimental Data In the Even-even Pt Nucleimentioning
confidence: 99%
“…More recently, Joss et al [61] studied the neutron-deficient 169−173 Pt nuclei obtaining more detailed information on the yrast bands for mass A = 170 and A = 172, and obtaining first information on side bands. Extra information on 174 Pt [62] and 178 Pt [63] has been obtained making use of the Gammasphere array, in particular, extending the yrast band up to spins (26 + ) and (24 + ), respectively. The yrast band in 178 Pt was extended by Soramel et al [64] up to spin (18 + ) using fusion-evaporation reactions.…”
Section: The Experimental Data In the Even-even Pt Nucleimentioning
confidence: 99%
“…9 Present address: Department of Physics, University of York, Heslington, YO1 5DD, UK. examples of this type of coexistence are exhibited by the N = 96 isotones 174 Pt [3,4] and 172 Os [5], which both exhibit yrast states with anomalous level spacings attributed to band mixing. It is interesting to investigate how the evolution of the yrast structures develop in the lighter (N 96) isotopes.…”
mentioning
confidence: 99%
“…This α energy is in the region of the energies of the 170 Ir α decays and is another source of contamination in the 170 Ir data that has to be considered. However, since the level scheme of 174 Pt is well known [18] it was possible to distinguish these γ rays from those belonging to 170 Ir. In Table I we have listed the energies and the relative intensities of the γ rays assigned 044312-2 to 170 Ir.…”
Section: Data Analysis and Resultsmentioning
confidence: 99%