Statistics – Computation
Scientific paper
Aug 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1269..439s&link_type=abstract
THE 10TH INTERNATIONAL SYMPOSIUM ON ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: OMEG-2010. AIP Conference Proceedings, Volume 1
Statistics
Computation
X-Ray Sources (Astronomical), Novae, Nucleosynthesis, Radioactive Ion Beams, X-Ray Sources, X-Ray Bursts, Cataclysmic Binaries, Symbiotic Stars, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages, Sources Of Radioactive Nuclei
Scientific paper
To better understand the energy generation and element synthesis occurring in novae and X-ray bursts, we give quantitative definitions to the concepts of ``bottlenecks'' and ``waiting points'' in the thermonuclear reaction flow. We use these criteria to search for bottlenecks and waiting points in post-processing element synthesis explosion simulations. We have incorporated these into the Computational Infrastructure for Nuclear Astrophysics, a suite of nuclear astrophysics codes available online at nucastrodata.org, so that anyone may perform custom searches for bottlenecks and waiting points.
Hix William Raphael
Lingerfelt Eric J.
Nesaraja Caroline D.
Smith Michael S.
Sunayama Tomomi
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