Plain Definition
What is simulation theory in physics?
Simulation theory is the idea that physical reality is generated by a deeper information process. OPH makes that idea precise as a zero-dial closure theory (zero quantitative inputs at the theory layer; working borrows counted in the scorecard): finite observer patches compare overlap-visible records, repair mismatch, and stabilize into the public physics we measure. The observer-facing fixed point counts as simulation only with the OPH certificate: endogenous update, records, repair, branch elimination, and clock closure.
The OPH version replaces the video-game metaphor with a physics claim about holographic screens, observer-local algebras, synchronization, records, repair, and certified fixed-point structure.
The local equation P_* = phi + sqrt(pi)/A_T(P_*) has a certified root for an incomplete map.
The official equation is N = log M0(U_N). Global finite readback is the correctable capacity M0(q) = alpha(Gq); selector-free closure is
Fr,0(D*) = {D*}, with N_CRC = log D*. On the exact reversible branch this reduces to
M0(q) = |Xreach(q)|. Separate horizon and electroweak/Higgs receipts connect that capacity to Lambda and the weak hierarchy.