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THE F-18(P,ALPHA) REACTION AND ITS ASTROPHYSICAL IMPLICATIONS

机译:F-18(P,ALPHA)反应及其天体物理意义

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摘要

F-18 radioactive beams were used to measure the F-18(p,alpha) reaction in the c.m. energy ranges of 265-535 keV and 550-740 keV. In each case, a resonant level was clearly detected, of which the resonant strength and some other properties were deduced. The astrophysical reaction rate was calculated down to the novae peak temperature. Consequences for the hot CNO cycles were drawn. (C) 1997 Elsevier Science B.V. [References: 16]
机译:F-18放射性束用于测量c.m中的F-18(p,α)反应。能量范围为265-535 keV和550-740 keV。在每种情况下,都清楚地检测到共振水平,由此推断出共振强度和其他一些特性。计算天体物理反应速率直至新星峰值温度。得出了热CNO循环的后果。 (C)1997 Elsevier Science B.V. [参考:16]

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