Neutron Physics of the Re/Os Clock. III. Resonance Analyses and Stellar (n,gamma) Cross Sections of 186,187,188Os
- FUJII K.
- MOSCONI M.
- MENGONI A.
- DOMINGO-PARDO C.
- KA¨PPELER F
- ABBONDANNO U.
- AERTS G.
- ALVAREZ POL H.
- ANDRIAMONJE S.
- ANDRZEJEWSKI J.
- ASSIMAKOPOULOS P.
- AUDOUIN L.
- BADUREK G.
- BAUMANN P.
- BECVAR F.
- BELLONI F.
- BERTHOUMIEUX E.
- BISTERZO S.
- CALVIANI M.
- CANO-OTT D.
- CAPOTE R.
- CARRILLO DE ALBORNOZ A.
- CENNINI P.
- CHEPEL V.
- CHIAVERI E.
- COLONNA N.
- CORTES G.
- COUTURE A.
- COX J.
- DAHLFORS M.
- DAVID S.
- DILLMANN I.
- DOLFINI R.
- DRIDI W.
- Duran-Escribano I.
- ELEFTHERIADIS C.
- EMBID-SEGURA M.
- EMBID-SEGURA M.
- FERRANT L.
- FERRARI A.
- FERREIRA-MARQUES R.
- FITZPATRICK L.
- Frais-Koelbl H.
- Frais-Koelbl H.
- FURMAN W.
- GALLINO R.
- GONCALVES I.
- GONZALEZ-ROMERO E.
- GOVERDOVSKI A.
- GRAMEGNA F.
- GRIESMAYER E.
- GUERRERO C.
- GUNSING F.
- HAAS B.
- HAIGHT R.
- HEIL M.
- HERRERA-MARTINEZ A.
- IGASHIRA M.
- ISAEV M.
- JERICHA E.
- KADI Y.
- KARAMANIS D.
- KARADIMOS Dimitrios
- KERVENO M.
- KETLEROV V.
- KOEHLER P.
- KONOVALOV V.
- KOSSIONIDES E.
- KRTICKA M.
- LAMBOUDIS C.
- LEEB H.
- LINDOTE A.
- LOPES I.
- LOZANO M.
- LUKIC S.
- MARGANIEC J.
- MARQUES L.
- MARRONE S.
- MASSIMI C.
- MASTINU P.
- Milazzo P.M.
- MOREAU C.
- NEVES F.
- OBERHUMMER H.
- OSHIMA M.
- O’Brien S.
- PANCIN J.
- PAPACHRISTODOULOU C.
- PAPADOPOULOS A
- PARADELA C.
- PATRONIS N.
- PAVLIK A.
- PAVLOPOULOS P.
- PERROT L.
- PLAG R.
- PLOMPEN Arjan
- PLUKIS A.
- POCH A.
- PRAENA J.
- PRETEL C.
- QUESADA J.
- RAUSCHER T.
- REIFARTH R.
- ROSETTI M.
- RUBBIA C.
- RUDOLF G.
- RULLHUSEN P.
- SALGADO J.
- SARCHIAPONE L.
- SAVVIDIS I.
- STEPHAN C.
- TAGLIENTE G.
- TAIN J.l.
- TASSAN-GOT L.
- TAVORA L.
- TERLIZZI R.
- VANNINI G.
- VAZ P.
- VENTURA A.
- VILLAMARIN D.
- VINCENTE M. C.
- VLACHOUDIS V.
- VLASTOU R.
- VOSS F.
- WALTER S.
- WENDLER H.
- WIESCHER M.
- WISSHAK K.
DOIAbstract
Neutron resonance analyses have been performed for the capture cross sections of 186Os, 187Os, and 188Os measured at the n TOF facility at CERN. Resonance parameters have been extracted up to 5, 3, and 8 keV, respectively, using the SAMMY code for a full R-matrix fit of the capture yields. From these results average resonance parameters were derived by a statistical analysis to provide a comprehensive experimental basis for modeling of the stellar neutron capture rates of these isotopes in terms of the Hauser-Feshbach statistical model. Consistent calculations for the capture and inelastic reaction channels are crucial for the evaluation of stellar enhancement factors to correct the Maxwellian averaged cross sections obtained from experimen...
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