In de Sitter static patch holography, coupling bulk quantum fields to an observer’s dynamical clock yields a type II von Neumann algebra of gauge-invariant observables. However, the unique tracial state on this algebra fails to reproduce semiclassical bulk correlation functions. We resolve this issue by introducing a family of heavy-clock states, representing an observer reference frame with heavy inertia. We prove that in the heavy-clock limit, -point correlation functions of gauge-invariant dressed observables reproduce the bulk quantum field correlation functions on de Sitter spacetime. Furthermore, we investigate a generalized observer Hamiltonian that incorporates both forward-running () and backward-running () clocks. The resulting von Neumann algebra of gauge-invariant observables remains a type~II factor and is isomorphic to , where is the algebra of complex matrices transforming between the two clock orientations. Time-reversal symmetry is implemented in this setting as an anti-unitary operator that exchanges the two clock orientations, yielding a type~II von Neumann algebra of gauge-invariant, time-reversal-invariant observables. We generalize the heavy-clock state construction to both and , showing that -point correlation functions calculated in heavy-clock states match the corresponding semiclassical bulk correlation functions. Finally, by coupling Einstein gravity to the Brown–Kuchař dust field, we derive the observer Hamiltonian from a perturbative reduction along the observer’s worldline in the limit. This provides a field-theoretic foundation for the observer model developed in this work.

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