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g factor of the 2 + 1 state of 168 Hf

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dc.contributor.authorWolf, A.
dc.contributor.authorBerant, Z
dc.contributor.authorWerner, V.
dc.contributor.authorHeinz, A.
dc.contributor.authorCasten, R.F.
dc.contributor.authorCasperson, R.J.
dc.contributor.authorBrenner, D.S.
dc.contributor.authorChevrier, R.
dc.contributor.authorMcCarthy, D.
dc.contributor.authorIlie, G.
dc.contributor.authorWilliams, Elizabeth
dc.date.accessioned2015-12-10T22:58:27Z
dc.date.issued2012
dc.date.updated2015-12-10T08:06:55Z
dc.description.abstractThe g factor of the 21+ state of 168Hf was measured using the perturbed angular correlation technique in a static external magnetic field. The result, g(21+)=0.17(3), is discussed in relation to the systematics of the previously reported g factors in the
dc.identifier.issn0556-2813
dc.identifier.urihttp://hdl.handle.net/1885/60861
dc.publisherAmerican Physical Society
dc.rightsAuthor/s retain copyrighten_AU
dc.sourcePhysical Review C: Nuclear Physics
dc.titleg factor of the 2 + 1 state of 168 Hf
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue3
local.bibliographicCitation.lastpage4
local.bibliographicCitation.startpage1
local.contributor.affiliationWolf, A., Yale University
local.contributor.affiliationBerant, Z, Yale University
local.contributor.affiliationWerner, V., Yale University
local.contributor.affiliationHeinz, A., Yale University
local.contributor.affiliationCasten, R.F., Yale University
local.contributor.affiliationCasperson, R.J., Yale University
local.contributor.affiliationBrenner, D.S., Yale University
local.contributor.affiliationChevrier, R., Yale University
local.contributor.affiliationMcCarthy, D., University of Surrey
local.contributor.affiliationIlie, G., Yale University
local.contributor.affiliationWilliams, Elizabeth, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidWilliams, Elizabeth, u5199930
local.description.notesImported from ARIES
local.identifier.absfor020202 - Nuclear Physics
local.identifier.ariespublicationu4155331xPUB569
local.identifier.citationvolume85
local.identifier.doi10.1103/PhysRevC.85.037304
local.identifier.scopusID2-s2.0-84859113861
local.type.statusPublished Version

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