The background as a quantum observable: Einstein's hole argument in a quasiclassical context
I. Schmelzer

TL;DR
This paper demonstrates that in a quasiclassical context, a background-free covariant theory cannot define outcomes of gravitational decoherence experiments, implying the necessity of a shared background for consistent results.
Contribution
It introduces a thought experiment linking gravitational decoherence to the background dependence of covariant theories, highlighting the need for a shared background in such frameworks.
Findings
Covariant theories cannot specify outcomes of gravitational decoherence experiments.
Experiments can reconstruct a common background shared by superposed gravitational fields.
Background dependence is essential for defining measurement outcomes in gravitational contexts.
Abstract
I consider a thought experiment measuring the decoherence for quasiclassical superpositions of gravitational field. A version of the hole argument allows to prove that a covariant (background-free) theory is completely unable to define the outcome of this experiment and is therefore not viable. Instead, the results of experiments of this type allow to reconstruct a common background shared by all superposed gravitational fields.
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
TopicsCosmology and Gravitation Theories · Noncommutative and Quantum Gravity Theories · Quantum Mechanics and Applications
