Temporal Casimir Rigidity and Closure of the Effective Metric: Identification of A_τ = 2

Under the frozen, unestablished hypothesis [H-F], Q11 claims $A_\tau=2$ using a normalisation pending revision and Schur rigidity. Under the independent spatial-limit hypothesis [H-L], this supplies the temporal entry of $g^{\mu\nu}=\mathrm{diag}(-2,2,2,2)\propto\eta^{\mu\nu}$, whose three spatial entries come from Q8 and Q10 and are pending revision.

Reading this page. The account below reports Q11's published argument pending correction. Its scalar normalisation depends on Q8; it is not a separate derivation protected by the frozen hypothesis [H-F]. The paper's historical title is retained.

Overview

The Q5b paper left open problem O3: the identification of the temporal coefficient $A_\tau$ entering the effective Lorentzian co-metric. The spatial coefficients $A_H = A_Z = 2$ were asserted by Q8 and Q10. Q11 claims to supply the missing temporal identification, using Q8's normalisation; this claim remains to be revised.

Q11's published argument invokes [H-F] to transfer equivariance to the temporal sector. Even if that transfer holds, Schur fixes a form only up to a scalar. Q11 sets that scalar using Q8, so the value $A_\tau=2$ is not independently established by this argument.

Q11 consequently claims, with the additional metric hypothesis [H-L], \[ g^{\mu\nu} = \mathrm{diag}(-2,\; 2,\; 2,\; 2) \propto \eta^{\mu\nu}, \] giving the conditional Minkowski metric reading. The three spatial entries are the values Q8 and Q10 assert; their derivation is pending revision since Q7 version 2.0 withdrew the identification it rests on. Q11 also imports Q8's scalar normalisation for $A_\tau$; the temporal value is pending revision too.

Revision pending. The claims summarised on this page are those of the deposited Q11, not independently validated coefficient values. Q11's abstract and proof explicitly import Q8's normalisation to fix the temporal scalar. [H-F] does not remove that dependency: both the absolute temporal value and the spatial values require revision. Schur alone leaves a scalar free.

Published argument, pending revision

The derivation chain and Q5b-O3

Q11 sits at the end of a long derivation chain linking the spectral admissibility programme to the emergent geometry:

Q5a → Q5b → Q7 → Q8 → Q9 → Q10 → U1 → W1 → H2 → Q11. The algebraic $A_\tau=2$ claim uses [H-F] and Q8's scalar normalisation; it is pending revision together with the spatial values. The metric reading additionally requires [H-L].

Each step contributes a specific structural argument:

Significance. A temporal coefficient derived independently would advance the programme. Q11's imported normalisation does not currently supply that independent result.

Relation to the Cosmochrony programme

Under [H-L], the identification $g^{\mu\nu} \propto \eta^{\mu\nu}$ asserted by the Q11 chain is a prerequisite for the papers that build the dynamical theory on the emergent geometry. Its temporal and spatial coefficient values are pending revision in the cascade Q7 version 2.0 opens:

Under [H-L], the temporal sign (the $-2$ entry in $g^{\mu\nu}$) encodes the Lorentzian signature and traces back to the opposite orientation of the temporal BFS shells relative to the spatial shells — a consequence of the non-commutative structure of the Heisenberg group.

References

Jérôme Beau. Temporal Casimir Rigidity and Closure of the Effective Metric: Identification of A_τ = 2, 2026. doi:10.5281/zenodo.20098387