Fig. 5.

Top: rate of change in 4He abundance due to the triple-α (red) and 12C(α, γ)16O (blue) reactions at a density of 1.2 × 106 g cm−3 and X(12C) = 0.1 dependent on temperature; bottom: crossing temperature TX above which the depletion due to α-captures exceeds that due to triple-α dependent on initial carbon abundance at a density of 1.2 × 106 g cm−3. The reaction rates are taken from the JINA Reaclib Database (Cyburt et al. 2010) based on Xu et al. (2013) for the α-capture and Fynbo et al. (2005) for the triple-α reaction.
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