New results for 8B(p,γ)9C, 11C(p,γ)12N, 13C(p,γ)14N and 14N(p,γ)15O at stellar energies

Details New results for 8B(p,γ)9C, 11C(p,γ)12N, 13C(p,γ)14N and 14N(p,γ)15O at stellar energies New results for 8B(p,γ)9C, 11C(p,γ)12N, 13C(p,γ)14N and 14N(p,γ)15O at stellar energies

May 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003nupha.718..147t&link_type=abstract

Nuclear Physics A, Volume 718, p. 147-150.

Physics

Nuclear Physics

2

Scientific paper

Four (p,γ) capture reaction rates have been determined at stellar energies through measurements of asymptotic normalization coefficients (ANCs). A brief introduction to ANCs is given followed by new results for the 8B(p,γ)9C, 11C(p,γ)12N, 13C(p,γ)14N and 14N(p,γ)15O reactions.

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