Measurement of the 70Ge(n;γ) cross section up to 300 keV at the CERN n_TOF facility
Neutron 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.
GAWLIK A.;
LEDERER-WOODS Claudia;
ANDRZEJEWSKI J.;
BATTINO U.;
FERREIRA P.;
GUNSING F.;
HEINITZ S.;
KRTICKA M.;
MASSIMI C.;
MINGRONE F.;
PERKOWSKI J.;
REIFARTH R.;
TATTERSALL A.;
VALENTA S.;
WEISS C.;
ABERLE O.;
AUDOUIN L.;
BACAK M.;
BALIBREA J.;
BARBAGALLO M;
BARROS S.;
BECARES V.;
BECVAR F.;
BEINRUCKER C.;
BERTHOUMIEUX E.;
BILLOWES J.;
BOSNAR D.;
BROWN S;
BRUGGER M.;
CAAMANO M.;
CALVIANI M.;
CALVIÑO F.;
CANO-OTT D.;
CARDELLA R.;
CASANOVAS A.;
CASTELLUCCIO D. M.;
CERUTTI F.;
CHEN Y. H.;
CHIAVERI E.;
COLONNA N.;
CORTES-GIRALDO M. A.;
CORTÉS G. P.;
COSENTINO Luigi;
DAMONE L.;
DIAKAKI M.;
DIETZ M.;
DOMINGO-PARDO C.;
DRESSLER R.;
DUPONT E.;
DURAN I.;
FERNÁNDEZ-DOMÍNGEZ B.;
FERRARI A.;
FERRO-GONÇALVES I.;
FINOCCHIARO Paolo;
FURMAN V.;
GARCIA A. R.;
GLODARIU T.;
GONCALVES I. F.;
GONZÁLEZ-ROMERO E.;
GOVERDOVSKI A.;
GRIESMAYER E.;
GUERRERO Carlos;
GÖBEL K.;
HARADA H.;
HEFTRICH T.;
HEYSE Jan;
JENKINS D. G.;
JERICHA E.;
KADI Y.;
KAPPELER F.;
KATABUCHI T.;
KAVRIGIN P.;
KETLEROV V.;
KHRYACHKOV Vitali;
KIMURA A.;
KIVEL N.;
KNAPOVA I.;
KOKKORIS M.;
KÄPPELER F.;
LEAL-CIDONCHA E.;
LEEB H.;
LERENDEGUI-MARCO J.;
LO MEO S.;
LONSDALE S.;
LOSITO R.;
MACINA D.;
MARGANIEC J.;
MARTÍNEZ T.;
MASTINU P.;
MASTROMARCO M.;
MATTEUCCI F.;
MAUGERI Emilio;
MENDOZA E.;
MENGONI A.;
MILAZZO P.M.;
MIREA M.;
MONTESANO S.;
MUSUMARRA A.;
NOLTE R.;
OPREA A.;
PATRONIS N.;
PAVLIK A.;
PORRAS I.;
PRAENA J.;
QUESADA J.;
RAJEEV K.;
RAUSCHER T.;
RIEGO-PEREZ A.;
ROUT P;
RUBBIA C.;
RYAN J.;
SABATE-GILARTE M;
SAXENA A.;
SCHILLEBEECKX Peter;
SCHMIDT S.;
SCHUMANN D.;
SEDYSHEV P.;
SMITH A. G.;
STAMATOPOULOS A.;
TAGLIENTE G.;
TAIN J.L.;
TARIFENO-SALDIVIA A.;
TASSAN-GOT L.;
TSINGANIS A.;
VANNINI G.;
VARIALE V.;
VAZ P.;
VENTURA A.;
VLACHOUDIS V.;
VLASTOU R.;
WALLNER A.;
WARREN S.;
WEIGAND M.;
WOLF C.;
WOODS P. J.;
WRIGHT T. J.;
ZUGEC P.;
2020-09-01
AMER PHYSICAL SOC
JRC119827
2469-9985 (online),
https://publications.jrc.ec.europa.eu/repository/handle/JRC119827,
10.1103/PhysRevC.100.045804 (online),
Additional supporting files
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