The r-Process and Nuclear Structure near the Dripline

Details The r-Process and Nuclear Structure near the Dripline The r-Process and Nuclear Structure near the Dripline

May 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aps..apr.b2001k&link_type=abstract

American Physical Society, April Meeting, 2004, May 1-4, 2004, Denver, Colorado April 2004, MEETING ID: APR04, abstract #B2.001

Astronomy and Astrophysics

Astrophysics

Scientific paper

The possible astrophysical environments and the two-source nature of the rapid neutron-capture process are not yet fully understood. Observables, like the solar-system isotopic abundance distribution or the elemental abundances in ultra-metal-poor halo stars, witness the interplay between nuclear-structure aspects near the neutron dripline and the appropriate astrophysical settings, and can give guidance to and constraints on stellar conditions and the associated nucleosynthesis of the heavy elements up to the Th, U cosmochronometers.

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