Hydrostatic and explosive nucleosynthesis in massive stars using improved nuclear and stellar physics

Details Hydrostatic and explosive nucleosynthesis in massive stars using improved nuclear and stellar physics Hydrostatic and explosive nucleosynthesis in massive stars using improved nuclear and stellar physics

May 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003nupha.718..463r&link_type=abstract

Nuclear Physics A, Volume 718, p. 463-465.

Physics

Nuclear Physics

2

Scientific paper

We have performed the first calculations to follow the evolution of all stable nuclei and their radioactive progenitors in a finely-zoned stellar model computed from the onset of central hydrogen burning through explosion as a Type II supernova. Calculations were done for 15 Msolar, 19 Msolar, 20 Msolar, and 25 Msolar Pop I stars using the most recently available set of experimental and theoretical nuclear data, revised opacity tables, and taking into account mass loss due to stellar winds. Here, we focus on the nuclear inputs.

Affiliated with

Also associated with

No associations

Rating

Hydrostatic and explosive nucleosynthesis in massive stars using improved nuclear and stellar physics 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 Hydrostatic and explosive nucleosynthesis in massive stars using improved nuclear and stellar physics, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Hydrostatic and explosive nucleosynthesis in massive stars using improved nuclear and stellar physics will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1471723