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Near-yrast, medium-spin, excited states ofRb91,Rb93, andRb95

Authors :
W. Urban
John Durell
A. Scherillo
A. Złomaniec
Kamila Sieja
A. G. Smith
J. F. Smith
T. Rząca-Urban
John P. Greene
J. A. Dare
H. Faust
B. J. Varley
I. Ahmad
R. Orlandi
J. Jolie
I. Tsekhanovich
Gary Simpson
Torsten Soldner
A. Linneman
Source :
Physical Review C. 82
Publication Year :
2010
Publisher :
American Physical Society (APS), 2010.

Abstract

The medium-spin structure of the nuclei {sup 93}Rb and {sup 95}Rb is studied following the neutron-induced fission of {sup 235}U at the PF1B neutron guide, using the FIFI spectrometer, and at the Lohengrin mass spectrometer of the Institut Laue-Langevin Grenoble. These nuclei, plus {sup 91}Rb, are also studied following the spontaneous fission of {sup 248}Cm and {sup 252}Cf sources, using the EUROGAM-II and Gammasphere detector arrays, respectively. A high-spin isomeric state, with a half-life of 111(11) ns, is found in {sup 93}Rb at an excitation energy of 4422.4 keV, which most likely corresponds to the fully aligned [{pi}(g{sub 9/2}) x {nu}(g{sub 7/2}h{sub 11/2})]{sub 27/2}{sup -} configuration. An analogous configuration is proposed for the 5297.9-keV level observed in {sup 91}Rb. A new E3 decay branch of the 1133.9-keV isomer in {sup 91}Rb is found, for which the rather low transition rate of B(E3)=3.8(10) W.u. is determined. The energy of the isomeric state of {sup 95}Rb is now proposed to be at 810.6 keV, with a spin of (9/2{sup +}), and its half-life determined to be T{sub 1/2}=94(7) ns. A cascade of prompt transitions is observed on top of the 810.6-keV isomer in {sup 95}Rb. The near-yrast structures of {sup 91}Rb, {supmore » 93}Rb, and {sup 95}Rb are compared to the results of shell-model calculations, which support the proposed 27/2{sup -} interpretation of states in {sup 91}Rb and {sup 93}Rb. An analogous 27/2{sup -} state is expected to occur in {sup 95}Rb, as a long-lived isomer at 3.24 MeV. No such isomeric decay could be observed in a measurement using the Lohengrin spectrometer, which shows that, if it exists, its population, following the fission of {sup 235}U, is at least four times lower than that of the analogous 27/2{sup -} isomer in {sup 97}Y.« less

Details

ISSN :
1089490X and 05562813
Volume :
82
Database :
OpenAIRE
Journal :
Physical Review C
Accession number :
edsair.doi...........0bf5c3d4dd6cd9b0ed9369880d4d1fe1