Nucleosynthesis in Massive Stars and Supernovae

Details Nucleosynthesis in Massive Stars and Supernovae Nucleosynthesis in Massive Stars and Supernovae

Feb 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997nupha.621..445w&link_type=abstract

Nuclear Physics A, v. 621, p. 445-452.

Physics

Nuclear Physics

14

Scientific paper

We briefly summarize some recent work on nucleosynthesis in massive stars and supernovae. Here we explore: 1) the effect of including additional sources of nucleosynthesis besides massive stars into the mixture - especially classical novae and several varieties of Type Ia supernovae; 2) the sensitivity of the results to choices of theoretical nuclear reaction rates in the mass range 28 <= A <= 70; 3) nucleosynthesis above the iron group using a much larger reaction network; and 4) the sensitivity of these results to recent revisions in experimental reaction rates for isotopes A <= 28. For the recently revised rates, 17O is no longer a massive star product.

Affiliated with

Also associated with

No associations

Rating

Nucleosynthesis in Massive Stars and Supernovae 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 Nucleosynthesis in Massive Stars and Supernovae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Nucleosynthesis in Massive Stars and Supernovae will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1606921