The Role of the 96 keV Level in the 19O(β-)19F Process at Stellar Temperatures

Details The Role of the 96 keV Level in the 19O(β-)19F Process at Stellar Temperatures The Role of the 96 keV Level in the 19O(β-)19F Process at Stellar Temperatures

Nov 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005apj...633l..61c&link_type=abstract

The Astrophysical Journal, Volume 633, Issue 1, pp. L61-L64.

Astronomy and Astrophysics

Astronomy

Nuclear Reactions, Nucleosynthesis, Abundances

Scientific paper

From isobaric analog symmetry arguments and nuclear shell model calculations, we evaluate the temperature dependence of the beta-decay rates of the ground state and first excited state at an excitation energy of 96 keV in 19O. It is shown that the decay from the excited level exceeds that of the ground state for T9>1. This feature may be of significance in the r-process and explosive nucleosynthesis.

Affiliated with

Also associated with

No associations

Rating

The Role of the 96 keV Level in the 19O(β-)19F Process at Stellar Temperatures 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 Role of the 96 keV Level in the 19O(β-)19F Process at Stellar Temperatures, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Role of the 96 keV Level in the 19O(β-)19F Process at Stellar Temperatures will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1835263