Abstract
This paper elaborates on an intrinsically quantum approach to gravity, which begins with a general framework for quantum mechanics and then seeks to identify additional mathematical structure on Hilbert space that is responsible for gravity and other phenomena. A key principle in this approach is that of correspondence: this structure should reproduce spacetime, general relativity, and quantum field theory in a limit of weak gravitational fields. A central question is that of “Einstein separability,” and asks how to define mutually independent subsystems, e.g. through localization. Familiar definitions involving tensor products or operator subalgebras do not clearly accomplish this in gravity, as is seen in the correspondence limit. Instead, gravitational behavior, particularly gauge invariance, suggests a network of Hilbert subspaces related via inclusion maps, contrasting with other approaches based on tensor-factorized Hilbert spaces. Any such localization structure is also expected to place strong constraints on evolution, which are also supplemented by the constraint of unitarity.
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Notes
Note, however, that one regularization of a gravitational line is to smear it over a cone extending to infinity, and moreover that in classical GR one can show that even at higher-orders gravitational fields can be localized to conical regions as one approaches infinity [32]. This provides evidence that such gravitational dressings can be consistent at higher orders in \(\kappa \).
See, e.g., [21], and references therin.
Here we make contact with a generalization of the Corvino-Schoen gluing theorem [35, 36] to the case with sources [34]. This theorem states that given initial vacuum initial data, one may find new initial data that agrees with the original data in a compact region, but matches a boosted Kerr solution outside large enough radius.
For gauge invariance, these operators should also be dressed; e.g. analogues to \(\Phi (x)\) may be used.
For the ultra-boosted case, this condition must be appropriately modified.
Note that, unlike entropic bounds, this bound involves energy localized in a region.
A possibly related structure has been described in [39].
Note also that the neighborhoods \(U_\epsilon \) labeling the Hilbert subspaces are not necessarily fundamental at the nonperturbative level, and may need to be replaced by labels not directly associated to neighborhoods.
Of course there is an inherent problem in this approach for closed universes, as the Hamiltonian vanises.
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Acknowledgements
This material is based upon work supported in part by the U.S. Department of Energy, Office of Science, under Award Number DE-SC0011702. I thank J. Hartle for useful conversations and comments on a draft of this paper.
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Giddings, S.B. Quantum-First Gravity. Found Phys 49, 177–190 (2019). https://doi.org/10.1007/s10701-019-00239-1
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DOI: https://doi.org/10.1007/s10701-019-00239-1