Indirect methods for astrophysical reaction rates
نویسندگان
چکیده
Capture reactions can be a technical challenge in the energy region of astrophysical interest. Alternative experimental techniques were developed making use of beams available at higher energies. Although they have been widely applied, these indirect methods have long called for theoretical validation. In this work we discuss the use of transfer and breakup reactions as astrophysical tools. We discuss the models used to analyze these reactions and the level of accuracy that can be obtained in the capture cross section. We also consider the various sources of uncertainties that need to be under control.
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