1986
DOI: 10.1086/163928
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A new estimate of the Ne-19(p, gamma) Na-20 and O-15(alpha, gamma) Ne-19 reaction rates at stellar energies

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Cited by 107 publications
(86 citation statements)
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“…The coincidence efficiencies are roughly 50%, 60%, and 70%, respectively. Our internal energy calibrations allow identifications of these states which are consistent with known levels in who studied the 19 F(d, n) 20 Ne reaction at several bombarding energies. In Ref.…”
supporting
confidence: 75%
“…The coincidence efficiencies are roughly 50%, 60%, and 70%, respectively. Our internal energy calibrations allow identifications of these states which are consistent with known levels in who studied the 19 F(d, n) 20 Ne reaction at several bombarding energies. In Ref.…”
supporting
confidence: 75%
“…The result on the lifetime of the 4.03-MeV state was also confirmed in an independent measurement at TRIUMF [21]. The remaining quantity to be determined is the α-decay branching ratios B α = Γ α /Γ that have mostly been estimated from the α strengths of the mirror states in 19 F with large systematic model dependent uncertainties inherent to the DWBA analysis of α-transfer reactions on 15 N [10,14,22]. Several attempts have been made in the past to measure the relative α-decay widths directly [13,17,18,23].…”
mentioning
confidence: 68%
“…This suggested that the previous lower limit estimate was too low. Cooper et al on the other hand performed an analytical stability study suggesting that the widely used rate of Langanke et al [10] might be too high [8]. An experimental study of 15 O(α, γ) 19 Ne is clearly necessary.…”
mentioning
confidence: 99%
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“…The 15 O(α,γ) 19 Ne reaction is known to play a crucial role in the advanced stages of astrophysical hydrogen burning [13]. In the 15 O(α,γ) 19 Ne reaction, the most crucial resonance is known to arise through the J π = 3/2 + resonant level at 504 keV with respect to the α + 15 O threshold (E x = 4.03 MeV).…”
Section: Introductionmentioning
confidence: 99%