Asymptotic Safety of Four-Dimensional Quantum Gravity
Determine whether quantum gravity in four spacetime dimensions is asymptotically safe by establishing that the renormalization group flow of all gravitational couplings approaches a finite-dimensional ultraviolet critical surface, thereby ensuring predictivity at arbitrarily high energies.
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It remains controversial whether gravity in 4 spacetime dimensions is actually asymptotically safe (our main calculational tools are restricted to the low-energy and weak-curvature regime), but if it were then standard QFT techniques could suffice to describe gravity in the strongly quantum domain (and thereby provide the simplest approach to making sensible predictions for it at high energies).
The question of whether a different treatment of the off-shell pole in the metric propagator can give rise to a Horndeski trajectory with positive $\Lambda$ in the IR is left to future work.
The question of whether Horndeski gravity can be ruled out as the EFT approximation to asymptotically safe scalar-tensor theories becomes even more nontrivial in larger truncations, and this work highlights the importance of further investigation of this issue.