content_image/365871.jpg content_image/365879.jpg
<img src='content_image/365871.jpg'>

The largest possible contributions to the B$_{d,s}$ mixing amplitudes come from the MFV con- tributions to the ( δ d i $_{3}$)$_{LL}$ ’s. Therefore, the effect is not enhanced for large tan β . 

We conclude that, for anarchical gravity-mediated contributions to the A -terms, the effects on FCNC processes are negligibly small. In contrast, any improvements in the neutron EDM measurements may either further strengthen the constraints on this framework or discover its effects. 

## C. Yukawa-like A -terms 

Here we explore the implications of A -terms of Yukawa-like texture as in the models with a FN symmetry discussed in Section IV A, specifically, Eq. (4.7), and 

<img src='content_image/365879.jpg'>

As concerns the δ q LL,RR parameters, the effect of such A -terms can be described as O ( r ) changes in the RGE coefficients c$_{u}$, c$_{d}$, c$_{uR}$, c$_{dR}$ defined in Eq. (A2); see Eqs. (A6) and (A7). This leads, in turn, to at most O (1) changes in the X$_{q}$$_{A}$ matrices. Therefore, the estimates for the ( δ q $_{ij}$)$_{LL,RR}$ parameters in this scenario vary by at most O (1) from the estimates obtained in Section V A for Z$_{A}$$_{q}$ = 0 at the high scale. 

As concerns the δ q LR parameters, the parametric suppression of ˜ A q ij can be extracted from 

