Fig. 2.

Top panel: ratio of the STPB13 electron-capture rate to that of ADE11 in the production region of 8B neutrinos. These are both computed on the solar structure resulting from the ADE11 SSM, with a PLJ14 composition. Middle panel: ratio of the neutrinos fraction produced in STPB13 SSM to that of ADE11, both computed with a PLJ14 composition. Bottom panel: product nν(8B)STPB13 ⋅ RSTPB13/(nν(8B)ADE11⋅RSTPB13) is shown; we note, in comparison with the other two panels, the much finer vertical scale. The consistency of this value with the unity means that there is practically no difference in computing a SSM with the revised STPB13 rate or applying it directly on the solar structure of a ADE11 SSM.
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