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dc.contributor.authorWeber, C.
dc.contributor.authorElomaa, V. -V.
dc.contributor.authorFerrer, R.
dc.contributor.authorFroehlich, C.
dc.contributor.authorAckermann, D.
dc.contributor.authorAystoe, J.
dc.contributor.authorAudi, G.
dc.contributor.authorBatist, L.
dc.contributor.authorBlaum, K.
dc.contributor.authorBlock, M.
dc.contributor.authorChaudhuri, A.
dc.contributor.authorDworschak, M.
dc.contributor.authorEliseev, S.
dc.contributor.authorEronen, T.
dc.contributor.authorHager, U.
dc.contributor.authorHakala, J.
dc.contributor.authorHerfurth, F.
dc.contributor.authorHessberger, F. P.
dc.contributor.authorHofmann, S.
dc.contributor.authorJokinen, A.
dc.contributor.authorKankainen, A.
dc.contributor.authorKluge, H. -J.
dc.contributor.authorLanganke, K.
dc.contributor.authorMartin, A.
dc.contributor.authorMartinez-Pinedo, G.
dc.contributor.authorMazzocco, M.
dc.contributor.authorMoore, I. D.
dc.contributor.authorNeumayr, J. B.
dc.contributor.authorNovikov, Yu. N.
dc.contributor.authorPenttilae, H.
dc.contributor.authorPlass, W. R.
dc.contributor.authorPopov, A. V.
dc.contributor.authorRahaman, S.
dc.contributor.authorRauscher, T.
dc.contributor.authorRauth, C.
dc.contributor.authorRissanen, J.
dc.contributor.authorRodriguez, D.
dc.contributor.authorSaastamoinen, A.
dc.contributor.authorScheidenberger, C.
dc.contributor.authorSchweikhard, L.
dc.contributor.authorSeliverstov, D. M.
dc.contributor.authorSonoda, T.
dc.contributor.authorThielemann, F. -K.
dc.contributor.authorThirolf, P. G.
dc.contributor.authorVorobjev, G. K.
dc.date.accessioned2013-04-12T10:59:45Z
dc.date.available2013-04-12T10:59:45Z
dc.date.issued2008-11
dc.identifier.citationWeber , C , Elomaa , V -V , Ferrer , R , Froehlich , C , Ackermann , D , Aystoe , J , Audi , G , Batist , L , Blaum , K , Block , M , Chaudhuri , A , Dworschak , M , Eliseev , S , Eronen , T , Hager , U , Hakala , J , Herfurth , F , Hessberger , F P , Hofmann , S , Jokinen , A , Kankainen , A , Kluge , H -J , Langanke , K , Martin , A , Martinez-Pinedo , G , Mazzocco , M , Moore , I D , Neumayr , J B , Novikov , Y N , Penttilae , H , Plass , W R , Popov , A V , Rahaman , S , Rauscher , T , Rauth , C , Rissanen , J , Rodriguez , D , Saastamoinen , A , Scheidenberger , C , Schweikhard , L , Seliverstov , D M , Sonoda , T , Thielemann , F -K , Thirolf , P G & Vorobjev , G K 2008 , ' Mass measurements in the vicinity of the r p-process and the nu p-process paths with the Penning trap facilities JYFLTRAP and SHIPTRAP ' , Physical Review C (nuclear physics) , vol. 78 , no. 5 , 054310 . https://doi.org/10.1103/PhysRevC.78.054310
dc.identifier.issn2469-9985
dc.identifier.urihttp://hdl.handle.net/2299/10392
dc.description.abstractThe masses of very neutron-deficient nuclides close to the astrophysical r p- and nu p-process paths have been determined with the Penning trap facilities JYFLTRAP at JYFL/Jyvaskyla and SHIPTRAP at GSI/Darmstadt. Isotopes from yttrium (Z=39) to palladium (Z=46) have been produced in heavy-ion fusion-evaporation reactions. In total, 21 nuclides were studied, and almost half of the mass values were experimentally determined for the first time: (88)Tc, (90-92)Ru, (92-94)Rh, and (94,95)Pd. For the (95)Pd(m), (21/2(+)) high-spin state, a first direct mass determination was performed. Relative mass uncertainties of typically delta m/m=5x10(-8) were obtained. The impact of the new mass values has been studied in nu p-process nucleosynthesis calculations. The resulting reaction flow and the final abundances are compared with those obtained with the data of the Atomic Mass Evaluation 2003.en
dc.format.extent18
dc.format.extent460384
dc.language.isoeng
dc.relation.ispartofPhysical Review C (nuclear physics)
dc.subjectEND-POINT
dc.subjectCARBON CLUSTERS
dc.subjectDELAYED PROTON EMISSION
dc.subjectATOMIC MASSES
dc.subjectCLASSICAL CANONICAL FORMALISM
dc.subjectHIGH-SPIN
dc.subjectBETA-DECAY
dc.subjectNEUTRON-DEFICIENT ISOTOPES
dc.subjectSHELL-MODEL CALCULATIONS
dc.subject2-PROTON RADIOACTIVITY
dc.titleMass measurements in the vicinity of the r p-process and the nu p-process paths with the Penning trap facilities JYFLTRAP and SHIPTRAPen
dc.contributor.institutionCentre for Astrophysics Research (CAR)
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.description.statusPeer reviewed
rioxxterms.versionofrecord10.1103/PhysRevC.78.054310
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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