Exploring the 18F(p,γ)19Ne gateway to the formation of heavy elements in hot stars

Details Exploring the 18F(p,γ)19Ne gateway to the formation of heavy elements in hot stars Exploring the 18F(p,γ)19Ne gateway to the formation of heavy elements in hot stars

Feb 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997phrvc..55..566r&link_type=abstract

Physical Review C (Nuclear Physics), Volume 55, Issue 2, February 1997, pp.R566-R569

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Nucleosynthesis In Novae, Supernovae, And Other Explosive Environments, Radiative Capture, Reactions Induced By Unstable Nuclei, 6<=A<=19

Scientific paper

An upper limit to the production of 19Ne through the 18F(p,γ) reaction at the recently discovered s-wave resonance has been determined. The limit implies that in a hot stellar environment (T9>0.5) this reaction is not a significant gateway from the hot CNO cycle towards the production of heavier elements in stars.

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