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WheelerDeWittEquation
The Wheeler-DeWitt equation plays a central role in the attempt to unify quantum mechanics with general relativity. It's part of a framework known as canonical quantum gravity and arises in the quantization of the Hamiltonian constraint in general relativity.
The classical Hamiltonian constraint is a central part of the Einstein-Hamilton equations, reflecting the invariance of general relativity under reparametrizations of time. When attempting to quantize gravity, this constraint leads to a rather unusual feature: the absence of time in the fundamental description.
The Wheeler-DeWitt equation can be more precisely written as:
Here,
This absence of time makes the interpretation of the Wheeler-DeWitt equation challenging. It raises deep questions about what it means for a system to evolve or for an observation to occur at a specific time.
Some approaches to solving or interpreting the Wheeler-DeWitt equation involve introducing a notion of time through additional structures or conditions, such as the introduction of a "clock" field within the system or the use of semiclassical approximations where classical time re-emerges. These attempts are misguided and doomed to fail because our universe lives in a specific surface that expanded from one of the roots of the conformally transformed Hardy Z function
where the scale is taken to be