New limits for the 19Ne(p,γ)20Na astrophysical reaction rate from direct measurements using radioactive beams

Details New limits for the 19Ne(p,γ)20Na astrophysical reaction rate from direct measurements using radioactive beams New limits for the 19Ne(p,γ)20Na astrophysical reaction rate from direct measurements using radioactive beams

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996phlb..381..402m&link_type=abstract

Physics Letters B, v. 381, p. 402-406.

Physics

9

Scientific paper

In explosive stellar hydrogen burning, the hot CNO cycles and the rp-process are mainly linked by the reaction sequence15 O(α,γ)19Ne(p,γ)20Na. Using intense 19Ne radioactive beams, both the 19Ne(p,γ) and the 19Ne(d,n) reaction have been studied. Upper and lower limits for the 19Ne(p,γ) reaction rate have been deduced, allowing to conclude that the 15O(α,γ) reaction is most likely the bottleneck reaction.

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