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The constraints in Eq. (5.14) imply that, for reasonable values of the RG-factor r$_{3}$ = O (1 − 10), most of the δ q LL parameters are dominated by MFV effects: 

where i ̸ = 3, whereas 

with 

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can be either MFV or gravity dominated. The δ q RR parameters in full anarchy are still non-MFV dominated, with the RR-mixing being subject to some subtleties discussed below. Order of magnitude estimates for the various δ q ij are given in Table VII. 

The situation regarding the RR flavor mixing is driven by three factors: the extremely strong constraint on r/r$_{3}$ , the fact that the latter stems from LR-mixing, which is only suppressed by √ r/r$_{3}$ , and the absence of significant MFV terms in the RR-mixing as opposed to the LL one. 

