Shape coexistence in 180Hg studied through the β decay of 180Tl
dc.contributor.author | ELSEVIERS, J. | |
hal.structure.identifier | Instituut voor Kern-en Stralingsfysica [IKS] | |
dc.contributor.author | N. ANDREYEV, A. | |
dc.contributor.author | ANTALIC, S. | |
dc.contributor.author | BARZAKH, A. | |
dc.contributor.author | BREE, N. | |
hal.structure.identifier | Instituut voor Kern-en Stralingsfysica [IKS] | |
dc.contributor.author | E. COCOLIOS, T. | |
dc.contributor.author | F. COMAS, V. | |
dc.contributor.author | DIRIKEN, J. | |
dc.contributor.author | FEDOROV, D. | |
dc.contributor.author | N. FEDOSSEYEV, V. | |
hal.structure.identifier | Institut de Physique Nucléaire d'Orsay [IPNO] | |
dc.contributor.author | FRANCHOO, S. | |
dc.contributor.author | A. HEREDIA, J. | |
hal.structure.identifier | Instituut voor Kern-en Stralingsfysica [IKS] | |
dc.contributor.author | HUYSE, M. | |
dc.contributor.author | IVANOV, O. | |
hal.structure.identifier | Institut Laue-Langevin [ILL] | |
dc.contributor.author | K¨OSTER, U. | |
dc.contributor.author | A. MARSH, B. | |
dc.contributor.author | D. PAGE, R. | |
dc.contributor.author | PATRONIS, N. | |
dc.contributor.author | SELIVERSTOV, M. | |
hal.structure.identifier | Aval du cycle et Energie Nucléaire [ACEN] | |
dc.contributor.author | TSEKHANOVICH, I. | |
dc.contributor.author | VAN DEN BERGH, P. | |
dc.contributor.author | VAN DE WALLE, J. | |
hal.structure.identifier | Instituut voor Kern-en Stralingsfysica [IKS] | |
dc.contributor.author | VAN DUPPEN, P. | |
hal.structure.identifier | Instituut voor Kern-en Stralingsfysica [IKS] | |
dc.contributor.author | VENHART, M. | |
dc.contributor.author | VERMOTE, S. | |
dc.contributor.author | VESELSK'Y, M. | |
dc.contributor.author | WAGEMANS, C. | |
dc.date.issued | 2011-09-07 | |
dc.identifier.issn | 0031-899X | |
dc.description.abstractEn | The β + /EC decay of 180Tl and excited states in the daughter nucleus 180Hg have been investigated at the CERN On-Line Isotope Mass Separator (ISOLDE) facility. Many new low-lying energy levels were observed in 180Hg, of which the most significant are the 0+ 2 at 419.6 keV and the 2+ 2 at 601.3 keV. The former is the bandhead of an excited band in 180Hg assumed originally to be of prolate nature. From the β feeding to the different states in 180Hg, the ground-state spin of 180Tl was deduced to be (4−,5−). | |
dc.language.iso | en | |
dc.publisher | American Physical Society (APS) | |
dc.title.en | Shape coexistence in 180Hg studied through the β decay of 180Tl | |
dc.type | Article de revue | |
dc.identifier.doi | 10.1103/PhysRevC.84.034307 | |
dc.subject.hal | Physique [physics]/Physique Nucléaire Expérimentale [nucl-ex] | |
bordeaux.journal | Physical Review | |
bordeaux.page | 034307 | |
bordeaux.volume | 84 | |
bordeaux.peerReviewed | oui | |
hal.identifier | in2p3-00655964 | |
hal.version | 1 | |
hal.popular | non | |
hal.audience | Non spécifiée | |
hal.origin.link | https://hal.archives-ouvertes.fr//in2p3-00655964v1 | |
bordeaux.COinS | ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Physical%20Review&rft.date=2011-09-07&rft.volume=84&rft.spage=034307&rft.epage=034307&rft.eissn=0031-899X&rft.issn=0031-899X&rft.au=ELSEVIERS,%20J.&N.%20ANDREYEV,%20A.&ANTALIC,%20S.&BARZAKH,%20A.&BREE,%20N.&rft.genre=article |
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