The construction, made concrete

Bits → qubits — the finite-λ ladder

The finite-information λ thesis says λ is a finite index over a finite set of record-histories, carrying the exact Born weights, with holography bounding the index. The cleanest way to see what that means is to build it at the smallest scales — one bit, two bits, three qubits — each machine-checked in Lean. This page is the ladder.

Read these as toys, not new physics. Every model below lives in a single fixed basis and is deliberately simple — its job is to make the construction, the metaselector, and the holographic boundary concrete and checkable. Because Born stays exact and λ stays inert, all of it is operationally Everett. “Entanglement” here means single-basis correlation (not a Bell/contextuality witness), and “Born emerges” assumes the iid variance (it packages Chebyshev, it does not derive Born). Everything is verified in the Lean development (TinyUniverse, TwoBitUniverse, ThreeQubitUniverse).

One bit — a single qubit

The smallest universe is a single qubit. Φ\Phi has two basis records; λ{0,1}\lambda \in \{0,1\} names which one is actual. Three things are machine-checked:

Two bits — two qubits

Now λ=(λA,λB)\lambda=(\lambda_A,\lambda_B) over four records. The new thing is correlation:

Honest caveat on “entanglement.” bell_correlated is a single-basis fact: the separable mixture 120000+121111\tfrac12\lvert00\rangle\langle00\rvert+\tfrac12\lvert11\rangle\langle11\rvert has the identical computational-basis distribution. So this is classical correlation in one basis, not an entanglement witness — a genuine witness needs multiple incompatible measurement contexts (CHSH/Mermin), which these toys do not have.

One bit in a two-qubit world — coarse-graining

What if the actuality budget is smaller than the record structure — one bit in a four-record world? Then λ cannot name a record; it names a binary coarse-graining (a yes/no question), and that coarse law is a one-bit universe (coarseBorn, coarse_is_oneBit). Spending the bit on a local outcome gives one party’s marginal (coarse_fstBit_eq_marginalA). And here correlation bites: on the Bell state the parity bit is definite (bell_parity_zero/_one) while a local bit is uniform (bell_local_uniform) — which binary question you actualize interacts with Φ’s correlations.

Three qubits — the resolution hierarchy and the entropy ceiling

Eight records. A kk-bit λ resolves a 2k2^k-block coarse-graining with exact partial-Born weights (blockBorn); at three bits it is the full per-record law (blockBorn_full_eq_triBorn). The budget is a resolution dial: 1 bit → 2 blocks, 2 bits → 4 blocks, 3 bits → 8 records.

The lesson is the entropy ceiling. The GHZ state c(000+111)c(\lvert000\rangle+\lvert111\rangle) lives in 8 records but only 000000 and 111111 carry weight (ghz_supported_on_diagonal): its computational-basis Born entropy is 1 bit, not logdim=3\log\dim = 3. So no budget reveals more than one bit — a two-bit reading never even separates A from B (ghz_2bit_collapse). In short, H(R)H(R) can sit far below logdim\log\dim — record information is the support entropy of the Born distribution, not the Hilbert dimension.

What this is and isn’t (honest scope). This is a standard Shannon / data-processing fact — a sparse Born distribution has H(R)<logdimH(R)<\log\dim — and it is basis-fixed: GHZ’s “1 bit” is the computational-outcome entropy (in the GHZ’s own basis it is 0; in the XX basis it is \sim2 bits), and the incoherent mixture 12000000+12111111\tfrac12\lvert000\rangle\langle000\rvert+\tfrac12\lvert111\rangle\langle111\rvert gives the identical table. So this is not a coherence/entanglement effect, and it is not evidence for holography: it illustrates the trivial H(R)logdimH(R)\le\log\dim, not the holographic H(R)SH(R)\le S (which rests on the finite-capacity postulate — and note, per P4-MICRO, that what is postulated is finiteness; the area form S=A/4P2S=A/4\ell_P^2 is itself derived via the Sakharov bridge, and even the value of GG is now derivable — as the relation G=1/(NΛs2)G=1/(N\Lambda_s^2) from a posited record-granularity scale Λs\Lambda_s (InducedNewtonConstant), the numerical value still needing the species accounting; and with that induced GG the granularity capacity maps onto the holographic dictionary — the boundary Cardy microstate count == QIQT-H’s bulk capacity exponent (A/4)NΛs2(A/4)N\Lambda_s^2, a machine-checked correspondence (HolographicBridge), not a boundary CFT — see below). This whole ladder is a sanity-check / pedagogy tool, not evidence: every number here is what any Everettian computes from the same Born distribution.

The metaselector — what fixes the framework

The ladder fixes a basis by hand and shows what λ selects among. The separate question — which record framework {Pα}\{P_\alpha\} is the right one (the metaselector) — is answered, machine-checked, as a no-go trilogy plus a positive selector: neither capacity (capacity_underdetermines_realm), nor symmetry (the unitary group is transitive on frameworks, so any invariant score is constant), nor the state Φ alone (it generates only the trivial framework) selects it — but einselection does (Zurek’s commutativity criterion: a record commuting with the monitored observable AA commutes with the interaction ABA\otimes B, so it is decoherence-free). The framework is the spectral algebra of the interaction Hamiltonian. See the theorem index.

Where the horizon creates the boundary

This is where holography enters the ladder. The Bekenstein–Bousso bound, attached to a causal diamond, caps how many distinguishable record-histories a region can hold — the finite stage on which λ is an index. Concretely, the holographic entropy SS of the diamond bounds the record information, and λ’s information is exactly that:

H(λ)  =  I(λ;R)    H(R)    Shorizon    A4P2.H(\lambda) \;=\; I(\lambda; R) \;\le\; H(R) \;\le\; S_{\text{horizon}} \;\sim\; \frac{A}{4\ell_P^2}.

So the horizon area is the boundary condition on λ’s finiteness: it bounds the cardinality of the index (how many actual records can coexist, eS\le e^{S}), per causal diamond — not Φ’s superpositions (that was the retired “capacity forbids records” error), and not the probability law (the retired “grid”). The quantity the bound caps is H(R)H(R), not logdim\log\dim — a sparse Born distribution can have H(R)logdimH(R)\ll\log\dim (the entropy ceiling above), so a region can carry a high-dimensional Φ while its actual record content stays within the horizon budget. Two honest qualifications: the H(R)SH(R)\le S step is the postulate (the only place holography enters — the enumeration neither tests nor supports it; it shows only the trivial H(R)logdimH(R)\le\log\dim), and H(λ)=I(λ;R)H(\lambda)=I(\lambda;R) holds because λ is the record (a deterministic function of RR).

Honest status of the boundary. The horizon bound here is a postulate — a one-sided capacity boundary condition supplied by the bounding area of a causal diamond, not derived. Two strengths are kept distinct: the entropy form H(R)SH(R)\le S (Bousso, on the decohered record) and the strictly stronger cardinality form logRS\log\lvert R\rvert\le S. (This is the Bousso capacity boundary condition — distinct from the von Neumann area floor SvN(ρR)QRS_{\rm vN}(\rho_R)\le Q_R, which is a derived P4-MICRO theorem given finiteness; see the theory.) The contract that threads it is machine-checked and category-error-proof (RecordContract, Born-from-projectors ‖P_r Φ‖²); the area value itself is physics input.

In one line

The ladder makes the finite-information λ construction concrete: λ is a finite index over records (exact Born), einselection fixes the framework, and the horizon bounds the index’s cardinality — the place where “Quantized Information” and “Holographic” meet the selector. It is single-basis pedagogy, machine-checked, and — because Born stays exact and λ is inert — operationally Everett.