Abstract
We show that coupling the standard model to a Lorentz symmetry-violating sector may coexist with viable phenomenology provided that the interaction between the two is mediated by higher-dimensional operators. In particular, if the new sector acquires anisotropic-scaling behavior above a ``Ho\ifmmode \check{r}\else \v{r}\fi{}ava-Lifshitz'' energy scale $\Lambda${}HL and couples to the standard model through interactions suppressed by Mpl, the transmission of the Lorentz violation into the standard model is protected by the ratio $\Lambda${}HL2/Mpl2. A wide-scale separation $\Lambda${}HL$\ll${}Mpl can then make Lorentz-violating terms in the standard model sector within experimental bounds without fine-tuning. We first illustrate our point with a toy example of Lifshitz-type neutral fermion coupled to photon via the magnetic moment operator, and then implement similar proposal for the Ho\ifmmode \check{r}\else \v{r}\fi{}ava-Lifshitz gravity coupled to conventional Lorentz-symmetric matter fields. We find that most radiatively induced Lorentz violation can be controlled by a large-scale separation, but the existence of instantaneously propagating non-Lifshitz modes in gravity can cause a certain class of diagrams to remain quadratically divergent above $\Lambda${}HL. Such problematic quadratic divergence however can be removed by extending the action with terms of higher Lifshitz-dimension, resulting in a completely consistent setup that can cope with the stringent tests of Lorentz invariance.

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