Coulomb dissociation of N 20,21

M. Röder,Tatsuya Adachi,Yulia Aksyutina,J. Alcantara,H. Alvarez-Pol,N. I. Ashwood,L. Atar,T. Aumann,V. Avdeichikov,M. Barr,S. Beceiro,D. Bemmerer,J. Benlliure,C. A. Bertulani,K. Boretzky,María José García Borge,G. Burgunder,M. Caamaño,C. Caesar,E. Casarejos,W. N. Catford,Joakim Cederkäll,S. Chakraborty, M. Chartier, L. V. Chulkov,D. Cortina-Gil,R. Crespo,Ushasi Datta Pramanik,Paloma Diaz-Fernandez,Iris Dillmann,Z. Elekes,J. Enders, O. Ershova, A. Estrade, F. Farinon, L. M. Fraile,Martin Freer,M. Freudenberger,H. O. U. Fynbo,Daniel Galaviz, H. Geissel,R. Gernhäuser, K. Göbel, P. Golubev,D. Gonzalez Diaz, J. Hagdahl,T. Heftrich,M. Heil,M. Heine,A. Heinz,A. Henriques,M. Holl, G. Ickert,A. Ignatov,B. Jakobsson,H. Johansson,B. Jonson, N. Kalantar-Nayestanaki,R. Kanungo,A. Kelic-Heil,R. Knöbel,T. Kröll,R. Krücken,J. Kurcewicz,Nikolaus Kurz, M. Labiche,C. Langer,Tudi Le Bleis, R. C. Lemmon, O. Lepyoshkina,Simon Lindberg,Jorge Machado,J. Marganiec, Magdalena Mostazo Caro, A. Movsesyan, M. A. Najafi, T. Nilsson,C. Nociforo, V. Panin,S. Paschalis, A. Perea, M. Petri,S. Pietri,R. Plag,A. Prochazka,A. Rahaman, G. Rastrepina,R. Reifarth,G. Ribeiro,M. Valentina Ricciardi,C. Rigollet,K. Riisager,D. Rossi,Jose Sanchez del Rio Saez,D. Savran,Heiko Scheit,Haik Simon,Olivier Sorlin, B. Streicher,J. Taylor,Olof Tengblad,S. Terashima, R. Thies,Yasuhiro Togano, E. Uberseder,J. Van de Walle, P. Velho,V. Volkov,A. Wagner,F. Wamers,H. Weick, M. Weigand,C. Wheldon,G. Wilson,C. Wimmer,J. S. Winfield,Philip Woods,Dmitry Yakorev,M. V. Zhukov, A. Zilges,K. Zuber

PHYSICAL REVIEW C(2016)

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摘要
Neutron-rich light nuclei and their reactions play an important role in the creation of chemical elements. Here, data from a Coulomb dissociation experiment on N-20,N-21 are reported. Relativistic N-20,N-21 ions impinged on a lead target and the Coulomb dissociation cross section was determined in a kinematically complete experiment. Using the detailed balance theorem, the N-19(n,gamma)N-20 and N-20(n,gamma)N-21 excitation functions and thermonuclear reaction rates have been determined. The N-19(n,gamma)N-20 rate is up to a factor of 5 higher at T < 1 GK with respect to previous theoretical calculations, leading to a 10% decrease in the predicted fluorine abundance.
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