Abstract

We analyze the constraints of general coordinate invariance for quantum theories possessing conformal symmetry in four dimensions. The character of these constraints simplifies enormously on the Einstein universe R×S3R \times S^3. The SO(4,2)SO(4,2) global conformal symmetry algebra of this space determines uniquely a finite shift in the Hamiltonian constraint from its classical value. In other words, the global Wheeler-De Witt equation is {\it modified} at the quantum level in a well-defined way in this case. We argue that the higher moments of T00T^{00} should not be imposed on the physical states {\it a priori} either, but only the weaker condition ⟨T˙00⟩=0\langle \dot T^{00} \rangle = 0. We present an explicit example of the quantization and diffeomorphism constraints on R×S3R \times S^3 for a free conformal scalar field.

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