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Copy-Horizon Cosmology from Quantum Information Copy Time: An Operational Infrared Cutoff for Holographic Dark Energy with Testable Signatures

Submitted:

06 January 2026

Posted:

09 January 2026

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Abstract
We present a strict, non-circular formulation of a “copy-horizon” infrared (IR) scale Lcopy(t) defined operationally from a quantum-information copy time τcopy(L, t) by the single criterion τcopy(Lcopy(t), t) = H−1(t). The definition requires only mild locality/monotonicity assumptions and does not postulate an a priori cosmological IR cutoff (such as the future event horizon). We then combine this operational IR scale with the Cohen–Kaplan–Nelson (CKN) gravitational collapse bound to obtain the L−2 energy-density scaling as a consistency constraint, and we formulate “saturation” as a falsifiable mechanism with a severe inequality cQ(z) ≤ 1. We derive the minimal background consequence wQ(t) = −1 + (2/3)(L̇copy/(HLcopy)) and show how a hydrodynamic realization of τcopy yields rigid consistency relations linking expansion, growth, and transient time-of-flight observables.
Keywords: 
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Scope and Non-Circularity

This paper isolates a single operational input—the copy time  τ c o p y L , t —and derives its minimal cosmological consequences without introducing an independent cosmological infrared cutoff by fiat. In particular, we do not define L c o p y as the future event horizon. The event-horizon cutoff is used only as a comparator in a dedicated discussion paragraph.

Operational Definition of τ c o p y

Let A and B be spatially separated regions of a quantum many-body system. At t = 0 a local perturbation is applied in A (e.g. by a unitary U A ), yielding two global states ρ 0 t and ρ 1 t at time t with reduced states ρ 0 , B t and ρ 1 , B t on B . Given a measurement class M B accessible to the receiver, define the optimal distinguishability advantage
Δ M B t ; L s u p M M B T r M ( ρ 1 , B t ρ 0 , B t ) .
For unrestricted M B this reduces to the Helstrom distinguishability associated with the trace distance . Fix 0 < ε < 1 . The copy time is
τ c o p y L , t i n f τ 0 : Δ M B τ ; L , t ε .
The functional form of τ c o p y is determined by microscopic dynamics and the choice of M B ; it is not part of the definition. For a complete phenomenology, concrete realizations must be provided (see Sec. 8).

Brick 1: Defining L c o p y t with no Model Parameters

We work in a spatially flat FLRW background with Hubble rate H t = a ˙ / a . We define the copy-horizon scale L c o p y t as the largest physical separation for which the copy certificate is achievable within one Hubble time:
τ c o p y L c o p y t , t = H 1 t .
Assuming L τ c o p y 0 and mild regularity, Eq. [eq:brick1] defines L c o p y t uniquely (locally in time). Differentiating yields the implicit evolution equation
L τ c o p y L c o p y , t L ˙ c o p y + t τ c o p y L c o p y , t = H ˙ H 2 .
This step is non-circular: L c o p y is determined by an operational time criterion, not by an assumed w z .
Illustrative realizations of τ c o p y L (ballistic and diffusive) and the definition τ c o p y L c o p y = H 1 . The intersection determines L c o p y t without assuming a cosmological cutoff.

Brick 2: L 2 Scaling from Gravitational Consistency

The CKN bound constrains any effective description in a region of size L : the energy E ρ L 3 must not exceed the mass of a black hole of the same size, M B H L M P 2 L . Hence
ρ L 3 M P 2 L ρ M P 2 L 2 .
Equation [eq:CKN] is not a dark-energy model; it is a consistency constraint. The same L 2 scaling underlies the holographic dark energy (HDE) literature, but here it is anchored to the operational scale L = L c o p y t rather than an a priori cosmological horizon choice .

Saturation as Mechanism and a Severe Inequality

We define the copy-horizon component Q by evaluating the CKN-consistent scaling at L = L c o p y t and allow for a (dimensionless) saturation parameter c Q :
ρ Q t = 3 c Q 2 M P 2 L c o p y t 2 .
A severe, falsifiable interpretation is
0 < c Q z 1 for   all   tested   z ,
where c Q > 1 would signal a violation of the gravitational consistency bound at the operational IR scale. In the Supplement we provide an explicit attractor toy-model in which saturation emerges as a stable fixed point.
Logical flow of the strict QICT program: operational τ c o p y   definition of L c o p y   CKN bound saturation mechanism and testable consistency conditions.

Brick 3: Fixing c Q from Ω Q , 0

Define ρ c t = 3 M P 2 H t 2 and Ω Q t = ρ Q / ρ c . At t = t 0 (today), ρ Q , 0 = 3 M P 2 H 0 2 Ω Q , 0 . Equating with Eq. [eq:rhoQ] gives
c Q 2 = Ω Q , 0 ( H 0 L c o p y t 0 ) 2 ,
so once L c o p y t 0 is obtained from Eq. [eq:brick1], the amplitude is fixed with no multi-parameter cosmological fit.

Minimal Cosmological Consequence: w Q from Conservation

Assuming no background energy exchange between Q and matter, ρ Q obeys
ρ ˙ Q + 3 H 1 + w Q ρ Q = 0 .
Since ρ Q L c o p y 2 , we have ρ ˙ Q / ρ Q = 2 L ˙ c o p y / L c o p y , hence
w Q t = 1 + 2 3 L ˙ c o p y t H t L c o p y t .
Thus w Q is a consequence once L c o p y t is determined from τ c o p y .

Concrete Realizations of τ c o p y and Rigid Consistency Relations

Ballistic (Causal) Lower Bound

Locality implies a light-cone constraint (Lieb–Robinson or relativity) : no measurement on B can have Δ > 0 before t < L / v L R . Therefore
τ c o p y L , t L / v L R t .

Diffusive Hydrodynamic Theorem (Constructive)

Assume a conserved density n x , t coupled to the perturbation and a hydrodynamic regime t n = D t 2 n with slowly varying D t . For an observable N B = B n x d 3 x in the measurement class, the mean response at distance L is controlled by the diffusive Green’s function. Using a severe SNR/Helstrom bound (e.g. via Cauchy–Schwarz and Pinsker-type inequalities) , one obtains asymptotically
τ c o p y L , t = L 2 4 D t 1 + O l o g L ,
up to subleading logarithmic terms that depend on thresholding and region geometry.

A Hard “Triangle” Test

If the diffusive closure [eq:diffusive] applies on the cosmological effective description, Eq. [eq:brick1] yields
L c o p y t = 2 D t H t .
Consequently, [eq:wQ] becomes a rigid relation between w Q and the log-derivatives of D and H . The strict program is then to confront a single inferred L c o p y z (and c Q z ) against multiple datasets: expansion H z (BAO/SNe/CMB), growth f σ 8 z and lensing, and an independent transient observable (e.g. energy-dependent time-of-flight dispersion δ t E , z if present). The joint compatibility is summarized schematically in Figure 3.
A hard observational test: the same L c o p y z and c Q z 1 must be compatible with expansion, growth/lensing, and an independent transient observable (if predicted) within the same microphysical closure.
Figure 1. Logical flow of the strict QICT construction: operational copy-time $\rightarrow$ copy-horizon scale $\rightarrow$ gravitational consistency bound $\rightarrow$ saturation hypothesis.
Figure 1. Logical flow of the strict QICT construction: operational copy-time $\rightarrow$ copy-horizon scale $\rightarrow$ gravitational consistency bound $\rightarrow$ saturation hypothesis.
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Figure 2. Examples of copy-time scalings (ballistic and diffusive) and the operational definition $\tau_{\mathrm{copy}}(L_{\mathrm{copy}})=H^{-1}$.
Figure 2. Examples of copy-time scalings (ballistic and diffusive) and the operational definition $\tau_{\mathrm{copy}}(L_{\mathrm{copy}})=H^{-1}$.
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Figure 3. Cross-observable consistency concept linking expansion $H(z)$, equation of state $w_Q(z)$, and an independent transient timing observable.
Figure 3. Cross-observable consistency concept linking expansion $H(z)$, equation of state $w_Q(z)$, and an independent transient timing observable.
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Minimal Real-Data Sanity Check (Cosmic Chronometers)

To demonstrate that the strict framework can be confronted with actual expansion-rate measurements without introducing many phenomenological degrees of freedom, we present a deliberately rigid closure example: (i) the diffusive scaling [eq:diffusive] with constant effective diffusivity D z = D 0 , (ii) maximal saturation c Q = 1 motivated by the max-capacity attractor picture in the Supplement, and (iii) spatial flatness with radiation neglected for z 2 .
In this limit, the background expansion becomes parameter-free once H 0 , Ω m 0 are fixed. Writing E z = H z / H 0 and Ω Q 0 = 1 Ω m 0 , the Friedmann equation reduces to a cubic relation
E z 3 E z Ω m 0 1 + z 3 Ω Q 0 = 0 .
We plot the corresponding prediction (normalized to the Planck 2018 baseline values ) against a 32-point cosmic-chronometer compilation in Figure 4. This is not advertised as a definitive global fit, but as a minimal, falsifiable closure demonstration that can be systematically upgraded (time-dependent D z , inclusion of radiation/curvature, joint BAO/SNe/CMB likelihoods).
Minimal real-data sanity check: cosmic-chronometer H z points compared to the rigid constant- D diffusive closure with maximal saturation c Q = 1 (no fitted parameters in this illustration; the normalization uses Planck 2018 values ).
Figure 4. Minimal quantitative illustration using a public cosmic-chronometer $H(z)$ compilation: data versus an illustrative QICT closure curve (not a full likelihood analysis).
Figure 4. Minimal quantitative illustration using a public cosmic-chronometer $H(z)$ compilation: data versus an illustrative QICT closure curve (not a full likelihood analysis).
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Figure 5. Derived $c_Q(z)$ from the minimal $H(z)$ illustration, displaying the strict consistency bound $c_Q(z)\le 1$ over the tested redshift range.
Figure 5. Derived $c_Q(z)$ from the minimal $H(z)$ illustration, displaying the strict consistency bound $c_Q(z)\le 1$ over the tested redshift range.
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Figure 6. Illustrative (mock) evolution of the QICT equation-of-state $w_Q(z)$ implied by the copy-horizon closure.
Figure 6. Illustrative (mock) evolution of the QICT equation-of-state $w_Q(z)$ implied by the copy-horizon closure.
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Figure 7. Illustrative (mock) evolution of the saturation parameter $c_Q(z)$ showing the falsifiable bound $c_Q(z)\le 1$ under an attractor mechanism.
Figure 7. Illustrative (mock) evolution of the saturation parameter $c_Q(z)$ showing the falsifiable bound $c_Q(z)\le 1$ under an attractor mechanism.
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Relation to Standard HDE Cutoffs (Comparator Only)

Standard holographic dark energy often adopts a future event-horizon cutoff L H D E R h . In contrast, the present work defines L c o p y operationally by Eq. [eq:brick1]. The event-horizon choice may be treated as a comparator model, or potentially recovered as a special case under additional assumptions on the functional dependence of τ c o p y L , t ; we do not assume such an identification in the main derivation.

Conclusions

The strict QICT copy-horizon program is characterized by (i) an operational definition of τ c o p y and L c o p y , (ii) a gravitational consistency bound implying L 2 scaling, and (iii) falsifiable saturation conditions such as c Q z 1 and multi-observable consistency relations. The accompanying Supplement and derivation package provide additional proofs, sector separation statements, and reproducible scripts.

References

  1. C. W. Helstrom, Quantum Detection and Estimation Theory (Academic Press, 1976). [CrossRef]
  2. S. Holevo, Probabilistic and Statistical Aspects of Quantum Theory (North-Holland, 1982). [CrossRef]
  3. M. A. Nielsen and I. L. Chuang, Quantum Computation and Quantum Information (Cambridge University Press, 2010).
  4. E. H. Lieb and D. W. Robinson, “The finite group velocity of quantum spin systems,” Commun. Math. Phys. 28, 251–257 (1972). [CrossRef]
  5. Cohen, D. Kaplan, and A. Nelson, “Effective field theory, black holes, and the cosmological constant,” Phys. Rev. Lett. 82, 4971 (1999). [CrossRef]
  6. M. Li, “A model of holographic dark energy,” Phys. Lett. B 603, 1–5 (2004).
  7. N. Aghanim et al. (Planck Collaboration), “Planck 2018 results. VI. Cosmological parameters,” Astron. Astrophys. 641, A6 (2020). [CrossRef]
  8. M. Moresco, R. Jimenez, L. Verde, A. Cimatti, and L. Pozzetti, “Setting the Stage for Cosmic Chronometers. II. Impact of Stellar Population Synthesis Models Systematics and Full Covariance Matrix,” Astrophys. J. 898, 82 (2020); arXiv:2003.07362. [CrossRef]
  9. Mehrabi, Cosmic_chronometer_data (GitHub repository), file HzTable_MM_BC32.txt (accessed 2026-01-06).
  10. Csiszár and J. Körner, Information Theory: Coding Theorems for Discrete Memoryless Systems (Akadémiai Kiadó, 1981). (See Pinsker-type inequalities.).
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