Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

Waiting Points in Nova and X-ray Burst Nucleosynthesis

Conference ·
DOI:https://doi.org/10.1063/1.2943610· OSTI ID:938747
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.
Research Organization:
Oak Ridge National Laboratory (ORNL), Oak Ridge, TN (United States)
Sponsoring Organization:
USDOE
DOE Contract Number:
AC05-00OR22725
OSTI ID:
938747
Country of Publication:
United States
Language:
English

Similar Records

Waiting Points in Nova and X-ray burst Nucleosynthesis
Journal Article · Wed May 21 00:00:00 EDT 2008 · AIP Conference Proceedings · OSTI ID:21143496

Bottlenecks and Waiting Points in Nucleosynthesis in X-ray bursts and Novae
Journal Article · Thu Aug 12 00:00:00 EDT 2010 · AIP Conference Proceedings · OSTI ID:21439577

Bottlenecks and Waiting Points in Nucleosynthesis in X-ray bursts and Novae
Conference · Sun Aug 01 00:00:00 EDT 2010 · AIP Conference Proceedings · OSTI ID:1564245