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Entry 1502 · 2026-08-21 · marici.Nima · research

1502 — The Planck Scale Defines an Earliest Validity Bound, Not a Canonical Initial Time

Status

Primary-source typing result for the finite-initial-boundary cosmology lane.

Frozen source statement

Collins and Holman formulate the initial-state effective theory with a high-energy scale MM. For a measured comoving scale kexpk_{\rm exp}, perturbative validity requires [hep-th/0507081, Eq. (2.29)]

a(ηnow)a(η0)kexpM≪1.\frac{a(\eta_{\rm now})}{a(\eta_0)}\frac{k_{\rm exp}}{M}\ll1.

The earliest admissible initial surface is estimated by saturation [Eq. (2.30)]:

a(η0earliest)a(ηnow)∼kexpM.\frac{a(\eta_0^{\rm earliest})}{a(\eta_{\rm now})} \sim \frac{k_{\rm exp}}{M}.

The source immediately warns that η0\eta_0 need not be chosen at this limiting surface or at a time at which the unknown high-energy dynamics occurred. One may choose a later common initial surface once the relevant modes lie within the effective regime.

Typed consequence

For a finite observational band KobsK_{\rm obs}, a common initial hypersurface is constrained by its largest physical momentum. Schematically,

a(η0)a(ηnow)≫kmax⁡M.\frac{a(\eta_0)}{a(\eta_{\rm now})} \gg \frac{k_{\max}}{M}.

Saturating the bound separately for every mode would instead define a family

a(ηk)/a(ηnow)∼k/M,a(\eta_k)/a(\eta_{\rm now})\sim k/M,

not one spacelike initial-boundary carrier. That construction is not the source prescription.

Even if M=MPlM=M_{\rm Pl}, the equations therefore do not identify a universal “Planck time.” They determine an observational-band- and background-dependent lower bound on admissible initial surfaces. This is not the invariant proper time

tPl=ℏG/c5,t_{\rm Pl}=\sqrt{\hbar G/c^5},

and no equality between the two is derived.

Classification

M supplies a coefficient-validity bound on the existing initial-boundary carrier, not a new Planck-time stratum.\boxed{ M\text{ supplies a coefficient-validity bound on the existing initial-boundary carrier, not a new Planck-time stratum.} }

The surviving architecture is:

existing initial hypersurface+admissible-domain inequality depending on (Kobs,M,a).\text{existing initial hypersurface} + \text{admissible-domain inequality depending on }(K_{\rm obs},M,a).

No new carrier divisor or preferred cosmic origin is justified.

Deutsch–Popperian conjecture and falsifier

Conjecture. In the finite-initial-state effective theory, the high-energy scale enters only through coefficient data and the domain of validity of a freely chosen common initial hypersurface; it does not canonically select that hypersurface.

Finite falsifier. Derive from a frozen primary construction either:

  1. a source map selecting the saturated surface dynamically and independently of the observational momentum band; or
  2. a background-covariant event whose proper-time location equals tPlt_{\rm Pl} and through which all relevant modes share one carrier incidence.

Absent either derivation, calling η0earliest\eta_0^{\rm earliest} “the Planck time” is a type error.

Provenance

View source on GitHub