A New 13N(p,{gamma})14O Reaction Rate And Its Influence In Novae Nucleosynthesis
Journal Article
·
· AIP Conference Proceedings
- Physics Division, Argonne National Laboratory, Argonne, Illinois 60439 (United States)
- Cyclotron Institute, Texas A and M University, College Station, Texas 77843 (United States)
- Institute of Nuclear Physics, Czech Academy of Sciences, Prague (Czech Republic)
- Institute of Physics and Nuclear Engineering H. Hulubei, Bucharest (Romania)
- Department of Physics, National University, Tashkent (Uzbekistan)
The direct capture contribution for 13N(p,{gamma})14O has been determined more precisely with the peripheral transfer reaction, 14N(13N,14O)13C at the energy of 11.8 MeV/nucleon using the ANC technique. The updated 13N(p,{gamma})14O reaction rate is about 2.5 times larger than the standard REACLIB rate in the temperature range 0.1 < T9 < 0.3. The transition condition from the cold to hot CNO cycles has been determined with this updated rate. The influences incurred by this update have been investigated with two one-zone nova models.
- OSTI ID:
- 20630861
- Journal Information:
- AIP Conference Proceedings, Vol. 764, Issue 1; Conference: Conference on nuclei at the limits, Argonne, IL (United States), 26-30 Jul 2004; Other Information: DOI: 10.1063/1.1905331; (c) 2005 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA); ISSN 0094-243X
- Country of Publication:
- United States
- Language:
- English
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