Stellar reaction rate of 14N(p, γ)15O and hydrogen burning in massive stars

Details Stellar reaction rate of 14N(p, γ)15O and hydrogen burning in massive stars Stellar reaction rate of 14N(p, γ)15O and hydrogen burning in massive stars

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987nupha.467..240s&link_type=abstract

Nuclear Physics A, Volume 467, Issue 2, p. 240-260.

Physics

Nuclear Physics

67

Nuclear Reactions

Scientific paper

The capture reaction 14N(p, γ)15O has been investigated in the energy range Ep = 0.2 to 3.6 MeV with the use of windowless gas targets as well as implanted 14N solid targets of high isotopic purity. The measurement of absolute cross sections, γ-ray angular distributions and excitation functions is reported. The data provide information on the capture amplitudes involved in the transitions to all bound states of 15O. The astrophysical S-factor at stellar energies has been determined by means of theoretical fits. The result of S(0) = 3.20 keV . b is in good agreement with the value incorporated in the compilations. Also discussed are the nuclear physics aspects of the data.

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