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Title: High accuracy {sup 18}O(p,{alpha}){sup 15}N reaction rate in the 8{center_dot}10{sup 6}-5{center_dot}10{sup 9} K temperature range

Journal Article · · AIP Conference Proceedings
DOI:https://doi.org/10.1063/1.3628378· OSTI ID:21612048
; ; ; ; ; ; ; ; ; ; ;  [1]; ; ; ; ; ;  [2];  [3];  [4]
  1. INFN - Laboratori Nazionali del Sud and DMFCI - Universita di Catania, Catania (Italy)
  2. Cyclotron Institute - Texas A and M University, College Station, TX (United States)
  3. CSNSM CNRS/IN2P3, Universite Paris Sud, Orsay France (France)
  4. GIK - Institute of Engineering Sciences and Technology, Topi District (Pakistan)

The {sup 18}O(p,{alpha}){sup 15}N reaction is of great importance in several astrophysical scenarios, as it influences the production of key isotopes such as {sup 19}F, {sup 18}O and {sup 15}N. In this work, a high accuracy {sup 18}O(p,{alpha}){sup 15}N reaction rate is proposed, based on the simultaneous fit of direct measurements and of the results of a new Trojan Horse experiment. In particular, we have focused on the study of the broad 660 keV 1/2{sup +} resonance. Since {Gamma}{approx}100-300 keV, it strongly influences the nearly-zero-energy region of the cross section by means of the low-energy tail of the resonant contribution and dominates the cross section at higher energies. Here we provide a factor of 2 larger reaction rate above T{approx}0.5 10{sup 9} K based over our new improved determination of its resonance parameters.

OSTI ID:
21612048
Journal Information:
AIP Conference Proceedings, Vol. 1377, Issue 1; Conference: FINUSTAR 3 Conference on frontiers in nuclear structure, astrophysics, and reactions, Rhodes (Greece), 23-27 Aug 2010; Other Information: DOI: 10.1063/1.3628378; (c) 2011 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA); ISSN 0094-243X
Country of Publication:
United States
Language:
English