R-Process Signatures:. Observations Versus Model Predictions

Details R-Process Signatures:. Observations Versus Model Predictions R-Process Signatures:. Observations Versus Model Predictions

Jun 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003cgrs.conf..328k&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

We compare r-process model predictions with recent astronomical observations from the solar system, ultra-metal-poor (UMP) halo stars and meteoritic r-process signatures, i.e. containing elemental as well as isotopic abundances. We deduce (1) astrophysical conditions (nn-ranges for weak and main r-process components) under which such r-patterns can be obtained, and (2) criteria to determine Th/U chronometric ages.

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