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dc.contributor.authorGAWLIK A.en_GB
dc.contributor.authorLEDERER-WOODS CLAUDIAen_GB
dc.contributor.authorANDRZEJEWSKI J.en_GB
dc.contributor.authorBATTINO U.en_GB
dc.contributor.authorFERREIRA P.en_GB
dc.contributor.authorGUNSING F.en_GB
dc.contributor.authorHEINITZ S.en_GB
dc.contributor.authorKRTICKA M.en_GB
dc.contributor.authorMASSIMI C.en_GB
dc.contributor.authorMINGRONE F.en_GB
dc.contributor.authorPERKOWSKI J.en_GB
dc.contributor.authorREIFARTH R.en_GB
dc.contributor.authorTATTERSALL A.en_GB
dc.contributor.authorVALENTA S.en_GB
dc.contributor.authorWEISS C.en_GB
dc.contributor.authorABERLE O.en_GB
dc.contributor.authorAUDOUIN L.en_GB
dc.contributor.authorBACAK M.en_GB
dc.contributor.authorBALIBREA J.en_GB
dc.contributor.authorBARBAGALLO Men_GB
dc.contributor.authorBARROS S.en_GB
dc.contributor.authorBECARES V.en_GB
dc.contributor.authorBECVAR F.en_GB
dc.contributor.authorBEINRUCKER C.en_GB
dc.contributor.authorBERTHOUMIEUX E.en_GB
dc.contributor.authorBILLOWES J.en_GB
dc.contributor.authorBOSNAR D.en_GB
dc.contributor.authorBROWN Sen_GB
dc.contributor.authorBRUGGER M.en_GB
dc.contributor.authorCAAMANO M.en_GB
dc.contributor.authorCALVIANI M.en_GB
dc.contributor.authorCALVIÑO F.en_GB
dc.contributor.authorCANO-OTT D.en_GB
dc.contributor.authorCARDELLA R.en_GB
dc.contributor.authorCASANOVAS A.en_GB
dc.contributor.authorCASTELLUCCIO D. M.en_GB
dc.contributor.authorCERUTTI F.en_GB
dc.contributor.authorCHEN Y. H.en_GB
dc.contributor.authorCHIAVERI E.en_GB
dc.contributor.authorCOLONNA N.en_GB
dc.contributor.authorCORTES-GIRALDO M. A.en_GB
dc.contributor.authorCORTÉS G. P.en_GB
dc.contributor.authorCOSENTINO LUIGIen_GB
dc.contributor.authorDAMONE L.en_GB
dc.contributor.authorDIAKAKI M.en_GB
dc.contributor.authorDIETZ M.en_GB
dc.contributor.authorDOMINGO-PARDO C.en_GB
dc.contributor.authorDRESSLER R.en_GB
dc.contributor.authorDUPONT E.en_GB
dc.contributor.authorDURAN I.en_GB
dc.contributor.authorFERNÁNDEZ-DOMÍNGEZ B.en_GB
dc.contributor.authorFERRARI A.en_GB
dc.contributor.authorFERRO-GONÇALVES I.en_GB
dc.contributor.authorFINOCCHIARO PAOLOen_GB
dc.contributor.authorFURMAN V.en_GB
dc.contributor.authorGARCIA A. R.en_GB
dc.contributor.authorGLODARIU T.en_GB
dc.contributor.authorGONCALVES I. F.en_GB
dc.contributor.authorGONZÁLEZ-ROMERO E.en_GB
dc.contributor.authorGOVERDOVSKI A.en_GB
dc.contributor.authorGRIESMAYER E.en_GB
dc.contributor.authorGUERRERO CARLOSen_GB
dc.contributor.authorGÖBEL K.en_GB
dc.contributor.authorHARADA H.en_GB
dc.contributor.authorHEFTRICH T.en_GB
dc.contributor.authorHEYSE JANen_GB
dc.contributor.authorJENKINS D. G.en_GB
dc.contributor.authorJERICHA E.en_GB
dc.contributor.authorKADI Y.en_GB
dc.contributor.authorKAPPELER F.en_GB
dc.contributor.authorKATABUCHI T.en_GB
dc.contributor.authorKAVRIGIN P.en_GB
dc.contributor.authorKETLEROV V.en_GB
dc.contributor.authorKHRYACHKOV VITALIen_GB
dc.contributor.authorKIMURA A.en_GB
dc.contributor.authorKIVEL N.en_GB
dc.contributor.authorKNAPOVA I.en_GB
dc.contributor.authorKOKKORIS M.en_GB
dc.contributor.authorKÄPPELER F.en_GB
dc.contributor.authorLEAL-CIDONCHA E.en_GB
dc.contributor.authorLEEB H.en_GB
dc.contributor.authorLERENDEGUI-MARCO J.en_GB
dc.contributor.authorLO MEO S.en_GB
dc.contributor.authorLONSDALE S.en_GB
dc.contributor.authorLOSITO R.en_GB
dc.contributor.authorMACINA D.en_GB
dc.contributor.authorMARGANIEC J.en_GB
dc.contributor.authorMARTÍNEZ T.en_GB
dc.contributor.authorMASTINU P.en_GB
dc.contributor.authorMASTROMARCO M.en_GB
dc.contributor.authorMATTEUCCI F.en_GB
dc.contributor.authorMAUGERI EMILIOen_GB
dc.contributor.authorMENDOZA E.en_GB
dc.contributor.authorMENGONI A.en_GB
dc.contributor.authorMILAZZO P.M.en_GB
dc.contributor.authorMIREA M.en_GB
dc.contributor.authorMONTESANO S.en_GB
dc.contributor.authorMUSUMARRA A.en_GB
dc.contributor.authorNOLTE R.en_GB
dc.contributor.authorOPREA A.en_GB
dc.contributor.authorPATRONIS N.en_GB
dc.contributor.authorPAVLIK A.en_GB
dc.contributor.authorPORRAS I.en_GB
dc.contributor.authorPRAENA J.en_GB
dc.contributor.authorQUESADA J.en_GB
dc.contributor.authorRAJEEV K.en_GB
dc.contributor.authorRAUSCHER T.en_GB
dc.contributor.authorRIEGO-PEREZ A.en_GB
dc.contributor.authorROUT Pen_GB
dc.contributor.authorRUBBIA C.en_GB
dc.contributor.authorRYAN J.en_GB
dc.contributor.authorSABATE-GILARTE Men_GB
dc.contributor.authorSAXENA A.en_GB
dc.contributor.authorSCHILLEBEECKX PETERen_GB
dc.contributor.authorSCHMIDT S.en_GB
dc.contributor.authorSCHUMANN D.en_GB
dc.contributor.authorSEDYSHEV P.en_GB
dc.contributor.authorSMITH A. G.en_GB
dc.contributor.authorSTAMATOPOULOS A.en_GB
dc.contributor.authorTAGLIENTE G.en_GB
dc.contributor.authorTAIN J.L.en_GB
dc.contributor.authorTARIFENO-SALDIVIA A.en_GB
dc.contributor.authorTASSAN-GOT L.en_GB
dc.contributor.authorTSINGANIS A.en_GB
dc.contributor.authorVANNINI G.en_GB
dc.contributor.authorVARIALE V.en_GB
dc.contributor.authorVAZ P.en_GB
dc.contributor.authorVENTURA A.en_GB
dc.contributor.authorVLACHOUDIS V.en_GB
dc.contributor.authorVLASTOU R.en_GB
dc.contributor.authorWALLNER A.en_GB
dc.contributor.authorWARREN S.en_GB
dc.contributor.authorWEIGAND M.en_GB
dc.contributor.authorWOLF C.en_GB
dc.contributor.authorWOODS P. J.en_GB
dc.contributor.authorWRIGHT T. J.en_GB
dc.contributor.authorZUGEC P.en_GB
dc.date.accessioned2020-09-02T00:05:08Z-
dc.date.available2020-09-01en_GB
dc.date.available2020-09-02T00:05:08Z-
dc.date.created2020-08-31en_GB
dc.date.issued2019en_GB
dc.date.submitted2020-06-03en_GB
dc.identifier.citationPHYSICAL REVIEW C vol. 100 no. 4 p. 045804en_GB
dc.identifier.issn2469-9985 (online)en_GB
dc.identifier.urihttps://publications.jrc.ec.europa.eu/repository/handle/JRC119827-
dc.description.abstractNeutron capture data on intermediate mass nuclei are of key importance to nucleosynthesis in the weak component of the slow neutron capture processes, which occurs in massive stars. The (n;γ)cross section on 70Ge, which is mainly produced in the s process, was measured at the neutron time-of-flight facility n_TOF at CERN. Resonance capture kernels were determined up to 40 keV neutron energy, and average cross sections up to 300 keV. Stellar cross sections were calculated from kT = 5 keV to kT = 100 keV. Results are in very good agreement with a previous measurement by Walter and Beer (1985), and recent evaluations. We have calculated isotopic abundances produced in the s process in a 25 solar mass star for two initial metallicities (below solar, and close to solar). While the low metallicity model reproduces best the solar system germanium isotopic abundances the close to solar model shows a good global match to solar system abundances between mass numbers A=60-80.en_GB
dc.description.sponsorshipJRC.G.2-Standards for Nuclear Safety, Security and Safeguardsen_GB
dc.format.mediumOnlineen_GB
dc.languageENGen_GB
dc.publisherAMER PHYSICAL SOCen_GB
dc.relation.ispartofseriesJRC119827en_GB
dc.titleMeasurement of the 70Ge(n;γ) cross section up to 300 keV at the CERN n_TOF facilityen_GB
dc.typeArticles in periodicals and booksen_GB
dc.identifier.doi10.1103/PhysRevC.100.045804 (online)en_GB
JRC Directorate:Nuclear Safety and Security

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