The synthesis of the light Mo and Ru isotopes: how now, no need for an exotic solution ?

Details The synthesis of the light Mo and Ru isotopes: how now, no need for an exotic solution ? The synthesis of the light Mo and Ru isotopes: how now, no need for an exotic solution ?

2000-05-25

arxiv.org/abs/astro-ph/0005513v1

Astronomy and Astrophysics

Astrophysics

4 pages, 4 figures. LaTex2e with aa.cls. A&A Letters, in press

Scientific paper

The most detailed calculations of the p-process call for its development in the O/Ne layers of Type II supernovae. In spite of their overall success in reproducing the solar system content of p-nuclides, they suggest a significant underproduction of the light Mo and Ru isotopes. On grounds of a model for the explosion of a 25 solar mass star with solar metallicity, we demonstrate that this failure might just be related to the uncertainties left in the rate of the 22Ne(alpha,n)25Mg neutron producing reaction. The latter indeed have a direct impact on the distribution of the s-process seeds for the p-process.

Affiliated with

Also associated with

No associations

Rating

The synthesis of the light Mo and Ru isotopes: how now, no need for an exotic solution ? 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 synthesis of the light Mo and Ru isotopes: how now, no need for an exotic solution ?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The synthesis of the light Mo and Ru isotopes: how now, no need for an exotic solution ? will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-200472