Statistics – Computation
Scientific paper
Aug 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1269...77s&link_type=abstract
THE 10TH INTERNATIONAL SYMPOSIUM ON ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: OMEG-2010. AIP Conference Proceedings, Volume 1
Statistics
Computation
Radioactive Ion Beams, X-Ray Effects, Supernovae, Nuclear Resonance Reactions, Gamma-Ray Effects, Sources Of Radioactive Nuclei, X-Ray Sources, X-Ray Bursts, Supernovae, Resonance Reactions, Gamma-Ray
Scientific paper
At ORNL, we are using unique radioactive beams to measure scattering, transfer, and capture reactions to help understand exploding stars such as novae, supernovae, and X-ray bursts. Recent results have been obtained with beams of 26Al, 17F, and 130,132Sn, utilizing gas targets, silicon strip detectors, and recoil separators. More exciting work is planned at the future FRIB facility. We are also using synergistic nuclear data evaluations and the Computational Infrastructure for Nuclear Astrophysics to investigate the astrophysical impact of our measurements.
No associations
LandOfFree
ORNL Radioactive Beams for Stellar Explosion Studies 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 ORNL Radioactive Beams for Stellar Explosion Studies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and ORNL Radioactive Beams for Stellar Explosion Studies will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1862476