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dc.date.accessioned2015-01-23T09:37:20Z
dc.date.available2015-01-23T09:37:20Z
dc.date.created2014-12-03T19:09:43Z
dc.date.issued2014
dc.identifier.citationSpyrou, A. Liddick, S.N. Larsen, Ann-Cecilie Guttormsen, Magne Sveen Cooper, K. Dombos, A.C. Morrissey, D.J. Naqvi, F. Perdikakis, G. Quinn, S.J. Renstrøm, Therese Rodriguez, J.A. Simon, A. Sumithrarachchi, C.S. Zegers, R.G.T. . Novel technique for Constraining r-Process (n, γ) Reaction Rates. Physical Review Letters. 2014, 113(232502)
dc.identifier.urihttp://hdl.handle.net/10852/41899
dc.description.abstractA novel technique has been developed, which will open exciting new opportunities for studying the very neutron-rich nuclei involved in the r process. As a proof of principle, the γ spectra from the β decay of 76Ga have been measured with the SuN detector at the National Superconducting Cyclotron Laboratory. The nuclear level density and γ-ray strength function are extracted and used as input to Hauser-Feshbach calculations. The present technique is shown to strongly constrain the 75Ge(n,γ)76Ge cross section and reaction rate. © 2014 American Physical Society
dc.languageEN
dc.publisherAmerican Physical Society
dc.relation.ispartofTherese Renstrøm (2015). Probing Statistical Properties of Ni, Ge, Nd and Sm isotopes. Doctoral thesis. http://urn.nb.no/URN:NBN:no-54017
dc.relation.urihttp://urn.nb.no/URN:NBN:no-54017
dc.titleNovel technique for Constraining r-Process (n, γ) Reaction Rates
dc.typeJournal article
dc.creator.authorSpyrou, A.
dc.creator.authorLiddick, S.N.
dc.creator.authorLarsen, Ann-Cecilie
dc.creator.authorGuttormsen, Magne Sveen
dc.creator.authorCooper, K.
dc.creator.authorDombos, A.C.
dc.creator.authorMorrissey, D.J.
dc.creator.authorNaqvi, F.
dc.creator.authorPerdikakis, G.
dc.creator.authorQuinn, S.J.
dc.creator.authorRenstrøm, Therese
dc.creator.authorRodriguez, J.A.
dc.creator.authorSimon, A.
dc.creator.authorSumithrarachchi, C.S.
dc.creator.authorZegers, R.G.T.
cristin.unitcode185,15,4,0
cristin.unitnameFysisk institutt
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode2
dc.identifier.cristin1180657
dc.identifier.bibliographiccitationinfo:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Physical Review Letters&rft.volume=113&rft.spage=&rft.date=2014
dc.identifier.jtitlePhysical Review Letters
dc.identifier.volume113
dc.identifier.doihttp://dx.doi.org/10.1103/PhysRevLett.113.232502
dc.identifier.urnURN:NBN:no-46306
dc.type.documentTidsskriftartikkel
dc.type.peerreviewedPeer reviewed
dc.source.issn0031-9007
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/41899/1/Spyrou_PhysRevLett.113.232502.pdf
dc.type.versionPublishedVersion
cristin.articleid232502


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