The Capture Reactions 15N(α, γ)19F and 20Ne(α, γ)24Mg at Astrophysically Relevant Energies

Details The Capture Reactions 15N(α, γ)19F and 20Ne(α, γ)24Mg at Astrophysically Relevant Energies The Capture Reactions 15N(α, γ)19F and 20Ne(α, γ)24Mg at Astrophysically Relevant Energies

Feb 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997nupha.621..145w&link_type=abstract

Nuclear Physics A, v. 621, p. 145-148.

Physics

Nuclear Physics

4

Scientific paper

The capture reactions 15N(α, γ)19F and 20Ne(α, γ)24Mg have been studied using a windowless gas target system and a 100% relative efficiency germanium detector with an active BGO shielding. For the 15N(α, γ)19F reaction 14 resonances have been analyzed in the range 650 keV < Eα,lab < 2650 keV, branching ratios and resonance strengths have been deduced. For the 20Ne(α, γ)24Mg reaction up to now 10 resonances have been investigated in the range 1640 keV < Eα,lab < 2650 keV. Due to the effective background reduction resonance strengths of weak resonances could be deduced. In near future the study will be extended to lower energies.

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