Extended Data Table 4 Similar to Extended Data Table 3 but uses the actual central temperature trajectory of a 40 M⊙ population III star model2 and using a mixing model to emulate convection

From: Measurement of 19F(p, γ)20Ne reaction suggests CNO breakout in first stars

  1. The trajectory was run until a core hydrogen mass fraction of 0.01. The mixing model assumes that the trajectory represents a fraction of τmix = 0.0595 of the total reservoir such that burning reduced the H mass fraction in the trajectory to 0.01, consistent with the stellar model. The reference rate for just using the original REACLIB rates for all binary reactions is log(40Ca) = −12.02.
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