Experimental Needs in Nuclear Astrophysics

Details Experimental Needs in Nuclear Astrophysics Experimental Needs in Nuclear Astrophysics

Oct 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aps..dnp.5wc02w&link_type=abstract

American Physical Society, Division of Nuclear Physics Meeting, October 5-8, 1997, abstract #5WC.02

Physics

Nuclear Physics

Scientific paper

Stable and radioactive beam experiments are important to understand and interpret nucleosynthesis processes in static and explosive stellar scenarios. The study of static stellar nucleosynthesis processes requires the use of high intensity low energy accelerators and the development of new sophisticated detector systems to measure sub-nanobarn reaction cross sections at the stellar energy range. On the other hand, the study of explosive nucleosynthesis requires the development of high intensity radioactive beams to measure reaction cross sections and decay properties on short-lived radioactive species. I will discuss several examples to elucidate various experimental quests in nuclear astrophysics and the experimental approaches on todays available stable and radioactive beam facilities.

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