Measurement of the radiative neutron capture cross section of 206Pb and its astrophysical implications
- DOMINGO-PARDO, C.
- ABBONDANNO, U.
- AERTS, G.
- ALVAREZ, H.
- ALVAREZ-VELARDE, F.
- ANDRIAMONJE, S.
- ANDRZEJEWSKI, J.
- ASSIMAKOPOULOS, P.
- AUDOUIN, L.
- BADUREK, G.
- BAUMANN, P.
- BECVAR, F.
- BERTHOUMIEUX, E.
- BISTERZO, S.
- CALVINO, F.
- CALVIANI, M.
- CANO-OTT, D.
- CAPOTE, R.
- CARRAPICO, C.
- CENNINI, P.
- CHEPEL, V.
- CHIAVERI, E.
- COLONNA, N.
- CORTES, G.
- COUTURE, A.
- COX, J.
- DAHLFORS, M.
- DAVID, S.
- DILLMAN, I.
- DOLFINI, R.
- DRIDI, W.
- DURAN, I.
- ELEFTHERIADIS, C.
- EMBID-SEGURA, M.
- FERRANT, L.
- FERRARI, Anthony
- FERREIRA-MARQUES, R.
- FITZPATRICK, L.
- FRAIS-KOELBL, H.
- FUJII, K.
- 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.
- KAPPELER, F.
- KADI, Y.
- KARADIMOS, D.
- KARAMANIS, D.
- 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.
- MARRONE, S.
- MASSIMI, C.
- MASTINU, P.
- MENGONI, A.
- MILAZZO, P.M.
- MOREAU, C.
- MOSCONI, M.
- NEVES, F.
- OBERHUMMER, H.
- OSHIMA, M.
- O'BRIEN, S.
- PANCIN, J.
- PAPACHRISTODOULOU, C.
- PAPADOPOULOS, C.
- PARADELA, C.
- PATRONIS, N.
- PAVLIK, A.
- PAVLOPOULOS, P.
- PERROT, L.
- PLAG, R.
- PLOMPEN, A.
- PLUKIS, A.
- POCH, A.
- 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
The (n, gamma) cross section of 206Pb has been measured at the CERN n_TOF facility with high resolution in the energy range from 1 eV to 600 keV by using two optimized C6D6 detectors. In the investigated energy interval about 130 resonances could be observed, from which 61 had enough statistics to be reliably analyzed via the R-matrix analysis code SAMMY. Experimental uncertainties were minimized, in particular with respect to (i) angular distribution effects of the prompt capture gamma-rays, and to (ii) the TOF-dependent background due to sample-scattered neutrons. Other background components were addressed by background measurements with an enriched 208Pb sample. The effect of the lower energy cutoff in the pulse height spectra of the C6D...
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