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dc.date.accessioned2019-02-19T15:00:41Z
dc.date.available2019-02-19T15:00:41Z
dc.date.created2015-04-15T13:24:54Z
dc.date.issued2015
dc.identifier.citationKheswa, Bonginkosi Vincent Wiedeking, Mathis Giacoppo, Francesca Goriely, Stephan Guttormsen, Magne Sveen Larsen, Ann-Cecilie Bello Garrote, Frank Leonel Eriksen, Tomas Kvalheim Görgen, Andreas Hagen, Trine Wiborg Koehler, Paul Edward Klintefjord, Malin Nyhus, Hilde-Therese Papka, P. Renstrøm, Therese Rose, Sunniva Johanne Sahin, Eda Siem, Sunniva Tornyi, Tamas Gabor . Galactic production of 138La: Impact of 138,139La statistical properties. Physics Letters B. 2015, 744, 268-272
dc.identifier.urihttp://hdl.handle.net/10852/66661
dc.description.abstractThe γ-ray strength functions and nuclear level densities of 138La and 139La have been measured below the neutron separation energies. These new data were used to calculate astrophysical Maxwellian-averaged () cross-sections to investigate the production and destruction of the p-nucleus 138La in the photodisintegration process. The results confirm the underproduction of 138La in the p-process with respect to the observed abundances and strongly support the ν-process through capture on 138Ba as the main contributor to the synthesis of 138La in Type II supernovae.en_US
dc.languageEN
dc.publisherNorth-Holland
dc.rightsAttribution 4.0 International
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.titleGalactic production of 138La: Impact of 138,139La statistical propertiesen_US
dc.typeJournal articleen_US
dc.creator.authorKheswa, Bonginkosi Vincent
dc.creator.authorWiedeking, Mathis
dc.creator.authorGiacoppo, Francesca
dc.creator.authorGoriely, Stephan
dc.creator.authorGuttormsen, Magne Sveen
dc.creator.authorLarsen, Ann-Cecilie
dc.creator.authorBello Garrote, Frank Leonel
dc.creator.authorEriksen, Tomas Kvalheim
dc.creator.authorGörgen, Andreas
dc.creator.authorHagen, Trine Wiborg
dc.creator.authorKoehler, Paul Edward
dc.creator.authorKlintefjord, Malin
dc.creator.authorNyhus, Hilde-Therese
dc.creator.authorPapka, P.
dc.creator.authorRenstrøm, Therese
dc.creator.authorRose, Sunniva Johanne
dc.creator.authorSahin, Eda
dc.creator.authorSiem, Sunniva
dc.creator.authorTornyi, Tamas Gabor
cristin.unitcode185,15,4,20
cristin.unitnameKjerne- og energifysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode1
dc.identifier.cristin1237353
dc.identifier.bibliographiccitationinfo:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Physics Letters B&rft.volume=744&rft.spage=268&rft.date=2015
dc.identifier.jtitlePhysics Letters B
dc.identifier.volume744
dc.identifier.startpage268
dc.identifier.endpage272
dc.identifier.doihttp://dx.doi.org/10.1016/j.physletb.2015.03.065
dc.identifier.urnURN:NBN:no-69850
dc.type.documentTidsskriftartikkelen_US
dc.type.peerreviewedPeer reviewed
dc.source.issn0370-2693
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/66661/1/Kheswa_PLB_2015.pdf
dc.type.versionPublishedVersion


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