
parameter-free, and it carries a CSS stabilizer code on its edges [9]. The matter content of the
same lattice, baryons as trapped defects, has been developed elsewhere [8]. Here we establish two
things and connect them.
First (Section 2), we compute the linearized Regge action on the D
4
star directly and show,
numerically and to machine precision, that the resulting operator has the defining properties of lin-
earized general relativity: it is two-derivative, its kernel is the group of linearized diffeomorphisms,
and a static energy source yields the Newtonian potential. This is the statement that the discrete
elastic geometry of D
4
reproduces linearized Einstein gravity.
Second (Sections 3–4), we reinterpret this sector as quantum error correction and add the
missing dynamics. We give the dictionary between code and geometry, and we introduce a decoding
flow, gradient descent on the squared syndrome residual, whose equilibrium we prove to be the
linearized Einstein equation of the first part. The flow is an auxiliary relaxation used to characterize
that fixed point, not a proposal for physical graviton propagation.
Scope. All results are at linear order in the metric perturbation. At this order the D
4
Regge
operator is exactly Fierz–Pauli. The cubic (three-graviton) vertex departs from Einstein–Hilbert
by an irreducible lattice anisotropy; that is a separate result, and we state it in Section 5 as a
limitation rather than treating it here.
Relation to prior work. Emergent linearized Einstein equations have been obtained before
from quantum-information structures, and it is important to state precisely what is and is not
new here. Cao, Carroll, and Michalakis [5] reconstruct a spatial geometry from the entanglement
structure of an abstract Hilbert-space state and find that perturbations obey a spatial analog of
Einstein’s equation; Cao and Carroll [6] extend this to a four-dimensional spacetime and argue,
through a modified version of Jacobson’s entanglement equilibrium, that the weak-field Einstein
equation emerges, explicitly without a boundary and with quantum error correction specifying the
emergence map. The finite-geometric model of L´evay and Holweck [4] likewise realizes spacetime
as an error-correcting code. Our construction differs from these in three specific respects. First, it
is anchored to a fixed, parameter-free physical lattice (D
4
/FCC), on which the linearized operator
is not merely argued to be Einstein-like but is computed and shown, in exact arithmetic, to equal
the Fierz–Pauli operator (Section 2.4). Second, it uses no entropy, entanglement equilibrium, or
Ryu–Takayanagi relation: the objective is a bare syndrome residual, a positive syndrome-residual
quantity, and the reference vacuum is a stabilizer codespace rather than a thermal or maximally
symmetric state. Third, it supplies an explicit decoding construction (a gradient flow on the
syndrome residual whose fixed point is the linearized Einstein equation), giving an operational
characterization of the field equation as the equilibrium of an error-correcting decoder rather than
deriving it only as an equilibrium condition; the flow itself is auxiliary, and we do not claim it as
physical graviton propagation. We note in passing a relevant limitation theorem: stabilizer codes
cannot support a nontrivial area operator for a bipartition [7], which is consistent with the present
work, since we do not construct an area operator or a holographic (boundary) correspondence; the
code here is a bulk lattice code and the geometry is carried by edge lengths, not by entanglement
areas.
2