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• W1628568551 abstract "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]." @default.
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• W1628568551 date "2011-07-06" @default.
• W1628568551 modified "2023-10-17" @default.
• W1628568551 title "Coulomb dissociation reactions on Mo isotopes for astrophysics applications" @default.
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• W1628568551 doi "https://doi.org/10.22323/1.100.0232" @default.
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