Direct measurement of the O-16(alpha,gamma)Ne-20 reaction at E-c.m.=2.43 MeV and 1.69 MeV
PHYSICAL REVIEW C(2012)
摘要
In stars, O-16 represents the endpoint of the helium burning sequence due to the low rate of O-16(alpha,gamma)Ne-20. We present a new direct measurement of the total cross section of O-16(alpha,gamma)Ne-20 at E-c.m. = 1.69MeV employing the DRAGON recoil separator. In addition, the branching ratios and strength of the E-c.m. = 2.426 MeV 3(-) resonance were determined.
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