In the Heisenberg picture, states are fixed and an observable evolves as
For a time-independent Schrödinger-picture observable,
For an operator in the Heisenberg picture, differentiating the evolution operators gives in units . With no explicit operator time dependence, the second term vanishes. Applying this commutator identity to the canonical momentum and real scalar field gives their operator field equations.

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  1. Unitary time evolution
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