“…Moreover, at NLL one also has to consider the effect of higher-dimensional operators (HDO) associated to the NGB nature of the Higgs, which modify the running of the brother top Yukawa. Notably, the effect of RG evolution, compared to the UV threshold contributions generated at m à , is logarithmically enhanced and, as already noticed in the literature [13,14,20,24], almost saturates the observed value of the Higgs quartic (or equivalently the Higgs mass, once the correct EW vacuum has been achieved). Moreover, while the IR contribution is calculable solely in terms of low-energy degrees of freedom and associated observables; thus, being rather model independent (up to details discussed in Appendix C), the UV contributions depend on the spectrum of composite states.…”