Can chaos be observed in quantum gravity?
Bianca Dittrich, Philipp A. Hoehn, Tim A. Koslowski, Mike I. Nelson

TL;DR
This paper explores how chaos in classical general relativity impacts the quantization of gravity, proposing a refined topology approach to define observables and achieve a viable quantum theory.
Contribution
It introduces a novel perspective on chaos in quantum gravity, suggesting topology refinement to obtain continuous observables and a consistent quantum framework.
Findings
Standard topology prevents semiclassical limits in the toy model.
Refined topology allows for complete quantum Dirac observables.
Implications for realistic quantum gravity theories and the concept of quantization.
Abstract
Full general relativity is almost certainly 'chaotic'. We argue that this entails a notion of nonintegrability: a generic general relativistic model, at least when coupled to cosmologically interesting matter, likely possesses neither differentiable Dirac observables nor a reduced phase space. It follows that the standard notion of observable has to be extended to include non-differentiable or even discontinuous generalized observables. These cannot carry Poisson-algebraic structures and do not admit a standard quantization; one thus faces a quantum representation problem of gravitational observables. This has deep consequences for a quantum theory of gravity, which we investigate in a simple model for a system with Hamiltonian constraint that fails to be completely integrable. We show that basing the quantization on standard topology precludes a semiclassical limit and can even…
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