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Resonance strength measurement at astrophysical energies: The {sup 17}O(p,α){sup 14}N reaction studied via Trojan Horse Method

Journal Article · · AIP Conference Proceedings
DOI:https://doi.org/10.1063/1.4932280· OSTI ID:22492475
;  [1];  [1]; ;  [2];  [3];  [4]; ;  [5]; ;  [6]
  1. INFN, Laboratori Nazionali del Sud, Catania (Italy)
  2. Dipartimento di Fisica e Astronomia, Università degli studi di Catania, Catania (Italy)
  3. Cyclotron Institute, Texas A&M University, College Station, Texas 77843 (United States)
  4. GIK Institute of Engineering Sciences and Technology, Topi, Districti Swabi, Khyber Pakhtunkhwa (Pakistan)
  5. Department of Physics, Joint Institute for Nuclear Astrophysics, University of Notre Dame, Notre Dame 46556, Indiana (United States)
  6. Nuclear Physics Institute of ASCR, Rez (Czech Republic)

In recent years, the Trojan Horse Method (THM) has been used to investigate the low-energy cross sections of proton-induced reactions on {sup 17}O nuclei, overcoming extrapolation procedures and enhancement effects due to electron screening. We will report on the indirect study of the {sup 17}O(p,α){sup 14}N reaction via the THM by applying the approach developed for extracting the resonance strength of narrow resonance in the ultralow energy region. Two measurements will be described and the experimental THM cross sections will be shown for both experiments.

OSTI ID:
22492475
Journal Information:
AIP Conference Proceedings, Journal Name: AIP Conference Proceedings Journal Issue: 1 Vol. 1681; ISSN APCPCS; ISSN 0094-243X
Country of Publication:
United States
Language:
English

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