Faster-than-light signalling is free of causal paradoxes only in theories with a preferred foliation of spacetime, a single global time that orders all signals. We ask whether R-layer Mode Theory (RLMT) supplies such a foliation. (1) None of the definitions of "layer" in earlier RLMT documents is a time function on four-dimensional spacetime; we therefore promote the Lindblad parameter of the Ω-layer to a spacetime field.(2) Under the assumptions of the parent paper the three mode populations obey a three-state master equation. With detailed balance, as in the parent paper, every clock built from the Ω-layer state stops as the layer relaxes, and no preferred foliation survives today. With a cycle affinity A ≠ 0, a nonequilibrium steady state carries a constant current J around the cycle 1→2→3→1 with entropy production σ = JA, and the cycle count is a clock that never stops. Three is the minimal number of modes for which this is possible.(3) In the Cartesian basis of the spin-1 representation the cycle is exactly the 120° rotation about the (1,1,1) axis, so A is the handedness of the Ω-layer circulation.(4) The primordial power spectrum cannot constrain A: for A = 3 the change in P(k) is at most 0.7% and is absorbed by the mode couplings to better than 10⁻⁴.(5) Promoting the cycle count to a field gives, by shift symmetry alone, a ghost condensate, the late-time attractor of the expansion. The branch fits in 1 eV ≲ M ≲ 100 GeV but RLMT does not predict M; its excitations are subluminal within the effective theory for α ≤ 1/4, and it inherits the generalized-second-law tension common to preferred-frame theories. The answer to the title question is: not in the parent form, and only in a nonequilibrium extension whose low-energy limit is a known, constrained theory without a usable faster-than-light channel. Numerical scripts are included.
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Tsuyoshi Tohi (2026) studied this question.
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