1 Limiting curvature can also be implemented to avoid future singularities (see, e.g., [3]).2 Even if one works in a gauge where ∂ i φ = 0, one assumes that ∂µφ remains a timelike vector in cuscuton gravity. Non-dynamical scalar fields with spacelike rather than timelike gradient vectors can also lead to interesting scalar-tensor theories of modified gravity [33]. 3 In a k-essence theory or generally without kinetic braiding [39], this quantity is the Hubble parameter. Thus, the issue arises when H = 0, which corresponds to the bouncing point when the universe transitions from contraction to expansion. 4 In fact, cuscuton gravity is often implemented within Horndeski theory, i.e., it is a special subclass. The simplest models of cuscuton gravity are of the k-essence type.