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Waiting Points in Nova and X-ray Burst Nucleosynthesis...

by Tomomi Sunayama, Michael S Smith, Eric J Lingerfelt, Kim Buckner, Caroline D Nesaraja
Publication Type
Conference Paper
Journal Name
AIP Conference Proceedings
Publication Date
Page Numbers
415 to 417
Volume
1016
Conference Name
10th International Symposium on Origin of Matter and Evolution of Galaxies
Conference Location
Sapporo, Japan
Conference Sponsor
Hokkaido University
Conference Date
-

In nova and X-ray burst nucleosynthesis, waiting points are nuclei in the reaction path which interrupt the nuclear flow towards heavier nuclei, typically because of a weak proton capture reaction and a long beta+ lifetime. Waiting points can influence the energy generation and final abundances synthesized in these explosions. We have constructed a systematic, quantitative set of criteria to identify rp-process waiting points, and use them to search for waiting points in post-processing simulations of novae and X-ray bursts. These criteria have been incorporated into the Computational Infrastructure for Nuclear Astrophysics, online at nucastrodata.org, to enable anyone to run customized searches for waiting points.