The canonical multi-event r- and s-process models, and their interrelations

Details The canonical multi-event r- and s-process models, and their interrelations The canonical multi-event r- and s-process models, and their interrelations

Feb 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997nupha.621..401g&link_type=abstract

Nuclear Physics A, v. 621, p. 401-404.

Physics

Nuclear Physics

Scientific paper

When considering an optimized superposition of astrophysical events characterized by a restricted set of plausible conditions, it is shown that the solar system r-process abundances can be reproduced quite well. The non-establishment of the (n,γ)-(γ,n) equilibrium along some isotopic chain is shown to be able to account for previously reported discrepancies with solar system observations. Additional uncertainties on the solar system r-abundances are discussed in the framework of a non-exponential s-process model. A new multi-event s-process model is constructed and compared with the exponential model predictions. Error bars on solar system r-abundances are derived by allowing deviations to the usually adopted exponential superposition of neutron exposures.

Affiliated with

Also associated with

No associations

Rating

The canonical multi-event r- and s-process models, and their interrelations does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The canonical multi-event r- and s-process models, and their interrelations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The canonical multi-event r- and s-process models, and their interrelations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1606905