Search for a resonance in the 14N(p,γ)15O reaction at Ep=127 keV

Details Search for a resonance in the 14N(p,γ)15O reaction at Ep=127 keV Search for a resonance in the 14N(p,γ)15O reaction at Ep=127 keV

Aug 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002phrvc..66b2801r&link_type=abstract

Physical Review C, vol. 66, Issue 2, id. 022801

Physics

1

Radiative Capture, Hydrostatic Stellar Nucleosynthesis, 6<=A<=19

Scientific paper

The 14N(p,γ)15O reaction regulates the energy produced by the CN cycle in main-sequence stars and in red giants. Recently, preliminary evidence was presented for a new resonance in this reaction, which would significantly increase the reaction rate for temperatures near 108 K. We have attempted to confirm this result and find no indication of a resonance near Elabp=127 keV. Our upper limit on its strength is ωγ<=32 neV (95% C.L.), which is more than 2 orders of magnitude below the previously reported value.

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