Coulomb dissociation reactions on Mo isotopes for astrophysics applications
Coulomb dissociation reactions on Mo isotopes for astrophysics applications
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天体物理学应用中钼同位素的库仑解离反应
DOI:
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发表时间:
2011
期刊:
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通讯作者:
A. Zilges
中科院分区:
文献类型:
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作者:
O. Ershova;P. Adrich;H. Alvarez;F. Aksouh;T. Aumann;M. Babilon;K. Behr;J. Benlliure;T. Berg;M. Boehmer;K. Boretzky;A. Bruenle;R. Beyer;E. Casarejos;M. Chartier;D. Cortina;A. Chatillon;U. D. Pramanik;Lionel Deveaux;M. Elvers;T. Elze;H. Emling;M. Erhard;B. Fernández;H. Geissel;M. Gorska;M. Heil;M. Hellstroem;G. Ickert;H. Johansson;A. Junghans;F. Käppeler;O. Kiselev;A. Klimkiewicz;J. Kratz;R. Kulessa;N. Kurz;M. Labiche;T. Bleis;R. Lemmon;K. Lindenberg;Y. Litvinov;P. Maierbeck;A. Movsesyan;S. Mueller;T. Nilsson;C. Nociforo;N. Paar;R. Palit;S. Paschalis;W. Prokopowicz;R. Reifarth;D. Rossi;L. Schnorrenberger;H. Simon;S. Klaus;G. Surówka;D. Vretenar;A. Wagner;S. Walter;W. Waluś;H. Weick;N. Winckler;M. Winkler;A. Zilges
Photo-dissociation reactions play an important role in p-process nucleosynthesis, which takes place in supernova explosions. Theoretical calculations of isotopic abundances of the p-nuclei require a vast reaction network linking thousands of isotopes, where most of the reaction rates must be derived from the Hauser-Feshbach statistical model. However, as many rates as possible need to be determined experimentally, in order to provide a reliable reference for the calculations. Measuring reaction rates on Mo isotopes is important to explain the problem of the significant underproduction of Mo and Ru in all existing models of p-process nucleosynthesis. Another aspect of the project is to verify the accuracy of the Coulomb dissociation method by comparing our data with experiments performed with real photons at S-DALINAC (TU Darmstadt) and ELBE (FZD) [1].