학술논문

Determination of the neutron-capture rate of C-17 for r-process nucleosynthesis
Document Type
Author
Heine, M.Typel, S.Wu, M. R.Adachi, T.Aksyutina, Y.Alcantara, J.Altstadt, S.Alvarez-Pol, H.Ashwood, N.Atar, L.Aumann, T.Avdeichikov, V.Barr, M.Beceiro-Novo, S.Bemmerer, D.Benlliure, J.Bertulani, C. A.Boretzky, K.Borge, M. J. G.Burgunder, G.Caamano, M.Caesar, C.Casarejos, E.Catford, W.Cederkall, J.Chakraborty, S.Chartier, M.Chulkov, L. V.Cortina-Gil, D.Crespo, R.Pramanik, U. D.Diaz Fernandez, Paloma, 1983; Dillmann, I.Elekes, Z.Enders, J.Ershova, O.Estrade, A.Farinon, F.Fraile, L. M.Freer, M.Freudenberger, M.Fynbo, H. O. U.Galaviz, D.Geissel, H.Gernhauser, R.Gobel, K.Golubev, P.Diaz, D. G.Hagdahl, Julius, 1985; Heftrich, T.Heil, M.Heinz, Andreas Martin, 1967; Henriques, A.Holl, M.Ickert, G.Ignatov, A.Jakobsson, B.Johansson, Håkan T, 1977; Jonson, Björn, 1941; Kalantar-Nayestanaki, N.Kanungo, R.Kelic-Heil, A.Knobel, R.Kroll, T.Krucken, R.Kurcewicz, J.Kurz, N.Labiche, M.Langer, C.Le Bleis, T.Lemmon, R.Lepyoshkina, O.Lindberg, Simon, 1987; Machado, J.Marganiec, J.Martinez-Pinedo, G.Maroussov, V.Mostazo, M.Movsesyan, A.Najafi, A.Neff, T.Nilsson, Thomas, 1965; Nociforo, C.Panin, V.Paschalis, S.Perea, A.Petri, M.Pietri, S.Plag, R.Prochazka, A.Rahaman, A.Rastrepina, G.Reifarth, R.Ribeiro, G.Ricciardi, M. V.Rigollet, C.Riisager, K.Roder, M.Rossi, D.del Rio, J. S.Savran, D.Scheit, H.Simon, H.Sorlin, O.Stoica, V.Streicher, B.Taylor, J. T.Tengblad, O.Terashima, S.Thies, Ronja, 1987; Togano, Y.Uberseder, E.Van de Walle, J.Velho, P.Volkov, V.Wagner, A.Wamers, F.Weick, H.Weigand, M.Wheldon, C.Wilson, G.Wimmer, C.Winfield, J. S.Woods, P.Yakorev, D.Zhukov, Mikhail, 1943; Zilges, A.Zuber, K.
Source
Physical Review C. 95(1)
Subject
Rich
Dissociation
Metal-Poor
Relativistic Heavy-Ions
Elements
Nuclear-Physics
Light
Ejecta
Cosmochronology
Detector
Language
English
ISSN
24699985
24699993
Abstract
With the (RB)-B-3-LAND setup at GSI we have measured exclusive relative-energy spectra of the Coulomb dissociation of C-18 at a projectile energy around 425A MeV on a lead target, which are needed to determine the radiative neutron-capture cross sections of C-17 into the ground state of C-18. Those data have been used to constrain theoretical calculations for transitions populating excited states in C-18. This allowed to derive the astrophysical cross section sigma(n gamma)*. accounting for the thermal population of C-17 target states in astrophysical scenarios. The experimentally verified capture rate is significantly lower than those of previously obtained Hauser-Feshbach estimations at temperatures T-9