Stellar Neutron Captures on Unstable Isotopes

Details Stellar Neutron Captures on Unstable Isotopes Stellar Neutron Captures on Unstable Isotopes

Jun 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003cgrs.conf..282k&link_type=abstract

CAPTURE GAMMA-RAY SPECTROSCOPY AND RELATED TOPICS. Proceedings of the Eleventh International Symposium. Held 2-6 September 2002

Astronomy and Astrophysics

Astrophysics

Scientific paper

The status of cross section measurements on unstable isotopes in the astrophysically relevant energy range between 0.3 to 300 keV is compared with the information requested from stellar evolution and explosive nucleosynthesis. Recently, this problem has attracted considerable experimental efforts as illustrated by some examples. New and promising perspectives for the near future are provided by the high fluxes available at spallation neutron sources which will allow for measurements on hitherto inaccessible cases. These data are very important for testing the current astrophysical scenarios of neutron capture nucleosynthesis.

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