Afficher la notice abrégée

The 92Zr(n,γ ) reaction and its implications for stellar nucleosynthesis

dc.contributor.authorTAGLIENTE, G.
dc.contributor.authorM. MILAZZO, P.
dc.contributor.authorFUJII, K.
dc.contributor.authorABBONDANNO, U.
hal.structure.identifierInstitut de Recherches sur les lois Fondamentales de l'Univers [IRFU]
dc.contributor.authorAERTS, G.
dc.contributor.authorALVAREZ, H.
hal.structure.identifierInstitut de Recherches sur les lois Fondamentales de l'Univers [IRFU]
dc.contributor.authorALVAREZ-VELARDE, F.
hal.structure.identifierInstitut de Recherches sur les lois Fondamentales de l'Univers [IRFU]
dc.contributor.authorANDRIAMONJE, S.
hal.structure.identifierInstitut de Recherches sur les lois Fondamentales de l'Univers [IRFU]
dc.contributor.authorANDRZEJEWSKI, J.
dc.contributor.authorAUDOUIN, L.
dc.contributor.authorBADUREK, G.
hal.structure.identifierDépartement Recherches Subatomiques [DRS-IPHC]
dc.contributor.authorBAUMANN, P.
dc.contributor.authorBECVAR, F.
dc.contributor.authorBELLONI, F.
hal.structure.identifierInstitut de Recherches sur les lois Fondamentales de l'Univers [IRFU]
dc.contributor.authorBERTHOUMIEUX, E.
dc.contributor.authorBISTERZO, S.
dc.contributor.authorCALVINO, F.
dc.contributor.authorCALVIANI, M.
dc.contributor.authorCANO-OTT, D.
dc.contributor.authorCAPOTE, R.
dc.contributor.authorCARRAPICO, C.
dc.contributor.authorCENNINI, P.
dc.contributor.authorCHEPEL, V.
dc.contributor.authorCHIAVERI, E.
dc.contributor.authorCOLONNA, N.
dc.contributor.authorCORTES, G.
dc.contributor.authorCOUTURE, A.
dc.contributor.authorCOX, J.
dc.contributor.authorDAHLFORS, M.
hal.structure.identifierDépartement Recherches Subatomiques [DRS-IPHC]
dc.contributor.authorDAVID, S.
dc.contributor.authorDILLMANN, I.
dc.contributor.authorDOMINGO-PARDO, C.
hal.structure.identifierInstitut de Recherches sur les lois Fondamentales de l'Univers [IRFU]
dc.contributor.authorDRIDI, W.
dc.contributor.authorDURAN, I.
dc.contributor.authorELEFTHERIADIS, C.
dc.contributor.authorEMBID-SEGURA, M.
dc.contributor.authorFERRARI, Anthony
dc.contributor.authorFERREIRA-MARQUES, R.
dc.contributor.authorFURMAN, W.
dc.contributor.authorGALLINO, R.
dc.contributor.authorGONCALVES, I.
dc.contributor.authorGONZALEZ-ROMERO, E.
dc.contributor.authorGRAMEGNA, F.
dc.contributor.authorGUERRERO, C.
hal.structure.identifierInstitut de Recherches sur les lois Fondamentales de l'Univers [IRFU]
dc.contributor.authorGUNSING, F.
hal.structure.identifierCentre d'Etudes Nucléaires de Bordeaux Gradignan [CENBG]
dc.contributor.authorHAAS, B.
dc.contributor.authorHAIGHT, R.
dc.contributor.authorHEIL, M.
dc.contributor.authorHERRERA-MARTINEZ, A.
dc.contributor.authorIGASHIRA, M.
dc.contributor.authorJERICHA, E.
dc.contributor.authorKAPPELER, F.
dc.contributor.authorKADI, Y.
dc.contributor.authorKARADIMOS, D.
dc.contributor.authorKARAMANIS, D.
hal.structure.identifierDépartement Recherches Subatomiques [DRS-IPHC]
dc.contributor.authorKERVENO, M.
dc.contributor.authorKOSSIONIDES, E.
dc.contributor.authorKRTICKA, M.
dc.contributor.authorLAMBOUDIS, C.
dc.contributor.authorLEEB, H.
dc.contributor.authorLINDOTE, A.
dc.contributor.authorLOPES, I.
dc.contributor.authorLOZANO, M.
hal.structure.identifierDépartement Recherches Subatomiques [DRS-IPHC]
dc.contributor.authorLUKIC, S.
dc.contributor.authorMARGANIEC, J.
dc.contributor.authorMARRONE, S.
dc.contributor.authorMART'INEZ, T.
dc.contributor.authorMASSIMI, C.
dc.contributor.authorMASTINU, P.
dc.contributor.authorMENGONI, A.
dc.contributor.authorMOREAU, C.
dc.contributor.authorMOSCONI, M.
dc.contributor.authorNEVES, F.
dc.contributor.authorOBERHUMMER, H.
dc.contributor.authorO'BRIEN, S.
dc.contributor.authorPANCIN, J.
dc.contributor.authorPAPACHRISTODOULOU, C.
dc.contributor.authorPAPADOPOULOS, C.
dc.contributor.authorPARADELA, C.
dc.contributor.authorPATRONIS, N.
dc.contributor.authorPAVLIK, A.
hal.structure.identifierPôle Universitaire Léonard de Vinci
dc.contributor.authorPAVLOPOULOS, P.
hal.structure.identifierInstitut de Recherches sur les lois Fondamentales de l'Univers [IRFU]
dc.contributor.authorPERROT, L.
dc.contributor.authorT. PIGNI, M.
dc.contributor.authorPLAG, R.
dc.contributor.authorPLOMPEN, A.
hal.structure.identifierInstitut de Recherches sur les lois Fondamentales de l'Univers [IRFU]
dc.contributor.authorPLUKIS, A.
dc.contributor.authorPOCH, A.
dc.contributor.authorPRAENA, J.
dc.contributor.authorPRETEL, C.
dc.contributor.authorQUESADA, J.
dc.contributor.authorRAUSCHER, T.
dc.contributor.authorREIFARTH, R.
dc.contributor.authorROSETTI, M.
dc.contributor.authorRUBBIA, C.
hal.structure.identifierDépartement Recherches Subatomiques [DRS-IPHC]
dc.contributor.authorRUDOLF, G.
dc.contributor.authorRULLHUSEN, P.
dc.contributor.authorSALGADO, J.
dc.contributor.authorSANTOS, C.
dc.contributor.authorSARCHIAPONE, L.
dc.contributor.authorSAVVIDIS, I.
hal.structure.identifierInstitut de Physique Nucléaire d'Orsay [IPNO]
dc.contributor.authorSTEPHAN, C.
dc.contributor.authorL. TAIN, J.
hal.structure.identifierInstitut de Physique Nucléaire d'Orsay [IPNO]
dc.contributor.authorTASSAN-GOT, L.
dc.contributor.authorTAVORA, L.
dc.contributor.authorTERLIZZI, R.
dc.contributor.authorVANNINI, G.
dc.contributor.authorVAZ, P.
dc.contributor.authorVENTURA, A.
dc.contributor.authorVILLAMARIN, D.
dc.contributor.authorC. VINCENTE, M.
dc.contributor.authorVLACHOUDIS, V.
dc.contributor.authorVLASTOU, R.
dc.contributor.authorVOSS, F.
dc.contributor.authorWALTER, S.
dc.contributor.authorWENDLER, H.
dc.contributor.authorWIESCHER, M.
dc.contributor.authorWISSHAK, K.
dc.date.issued2010-05
dc.identifier.issn2469-9985
dc.description.abstractEnBecause the relatively small neutron capture cross sections of the zirconium isotopes are difficult to measure, the results of previous measurements are often not adequate for a number of problems in astrophysics and nuclear technology. Therefore, the 92Zr(n,γ ) cross section has been remeasured at the CERN n TOF facility, providing a set of improved parameters for 44 resonances in the neutron energy range up to 40 keV.With this information the cross-section uncertainties in the keV region could be reduced to 5% as required for s-process nucleosynthesis studies and technological applications.
dc.language.isoen
dc.publisherAmerican Physical Society
dc.title.enThe 92Zr(n,γ ) reaction and its implications for stellar nucleosynthesis
dc.typeArticle de revue
dc.identifier.doi10.1103/PhysRevC.81.055801
dc.subject.halPhysique [physics]/Physique Nucléaire Expérimentale [nucl-ex]
bordeaux.journalPhysical Review C
bordeaux.page055801
bordeaux.volume81
bordeaux.peerReviewedoui
hal.identifierin2p3-00495974
hal.version1
hal.popularnon
hal.audienceNon spécifiée
hal.origin.linkhttps://hal.archives-ouvertes.fr//in2p3-00495974v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Physical%20Review%20C&rft.date=2010-05&rft.volume=81&rft.spage=055801&rft.epage=055801&rft.eissn=2469-9985&rft.issn=2469-9985&rft.au=TAGLIENTE,%20G.&M.%20MILAZZO,%20P.&FUJII,%20K.&ABBONDANNO,%20U.&AERTS,%20G.&rft.genre=article


Fichier(s) constituant ce document

FichiersTailleFormatVue

Il n'y a pas de fichiers associés à ce document.

Ce document figure dans la(les) collection(s) suivante(s)

Afficher la notice abrégée