Physics
Scientific paper
Sep 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986zphya.325..309w&link_type=abstract
Zeitschrift für Physik A Atomic Nuclei, Volume 325, Issue 3, pp.309-315
Physics
15
25.40, 97.10
Scientific paper
We have updated and recalculated the21Na( p, γ)22Mg and22Na( p, γ)23Mg reaction rates for temperatures 107 109 K relevant for explosive hydrogen burning in stellar environment. We find the21Na( p, γ)22Mg rate lower than recently suggested. Considering various uncertainties in spin and parity assignments of the low energy22Na+ p resonances we present upper and lower limits for the22Na( p, γ)23Mg reaction rate which, however, allows for a meaningful discussion of the consequences of the new rates on the Ne - Na cycle under various stellar conditions.
Langanke Karlheinz
Wiescher Michael
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