Nonperturbative Quantum Gravity in a Closed Lorentzian Universe
Yasunori Nomura, Tomonori Ugajin

TL;DR
This paper shows that nonperturbative quantum gravity in a closed universe can produce meaningful predictions through partial observability and environment-induced decoherence, without external observers or modifications.
Contribution
It introduces a framework where classical observables and probabilities emerge naturally from quantum gravity via subsystem tracing, avoiding the need for external measurement assumptions.
Findings
Classical outcomes arise from partial access to the universe.
Reduced density matrices encode classical information with suppressed uncertainties.
Quantum gravity in a closed universe can produce robust predictions inherently.
Abstract
We study how meaningful physical predictions can arise in nonperturbative quantum gravity in a closed Lorentzian universe. In such settings, recent developments suggest that the quantum gravitational Hilbert space is one-dimensional and real for each -sector, as induced by spacetime wormholes. This appears to obstruct the conventional quantum-mechanical prescription of assigning probabilities via projection onto a basis of states. While previous approaches have introduced external observers or augmented the theory to resolve this issue, we argue that quantum gravity itself contains all the necessary ingredients to make physical predictions. We demonstrate that the emergence of classical observables and probabilistic outcomes can be understood as a consequence of partial observability: physical observers access only a subsystem of the universe. Tracing out the inaccessible…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsNoncommutative and Quantum Gravity Theories · Cosmology and Gravitation Theories · Black Holes and Theoretical Physics
