Astrophysical S(E)-factor of the ^15N(p,α)^12C reaction at sub-Coulomb energies via the Trojan-horse method

Details Astrophysical S(E)-factor of the ^15N(p,α)^12C reaction at sub-Coulomb energies via the Trojan-horse method Astrophysical S(E)-factor of the ^15N(p,α)^12C reaction at sub-Coulomb energies via the Trojan-horse method

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aps..dnp.3a073s&link_type=abstract

American Physical Society, Division of Nuclear Physics Annual Meeting, October 25-28, 2006, abstract #3A.073

Physics

Nuclear Physics

Scientific paper

The low-energy bare-nucleus cross section for ^15N(p,α)^12C is extended by means of the Trojan-horse method applied to the ^2H(^15N,α^12C)n reaction at Ebeam=60 MeV. The astrophysical S-factor is compared to the direct data in the same energy region. A fair agreement is found at low energies between 80 keV and 250 keV, while the low-energy behavior of the S-factor suggests a smaller rate than reported in literature. There is a larger discrepancy between the direct data and Trojan-horse data at high energy. Further study is needed to clarify the source of this error.

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