Entanglement and Generalized Berry Geometrical Phases in Quantum Gravity
Diego J. Cirilo-Lombardo (Keldysh Institute of the Russian Academy of, Sciences, CONICET-UBA-INFINA), Norma G. Sanchez (CNRS, The Chalonge -, Hector de Vega International School of Astrophysics)

TL;DR
This paper introduces a new formalism based on the Minimum Group Representation Principle to analyze quantum spacetime, revealing novel entanglement and geometrical phases in cosmological and black hole contexts, with implications for quantum gravity dualities.
Contribution
It develops a formalism using the Metaplectic group to describe quantum spacetime, uncovering new entanglement structures and Berry phases relevant to cosmology and black holes.
Findings
Berry phases in inflationary cosmology linked to observable indices
Pure entangled states characterized in the Metaplectic group framework
Entanglement between different spacetime regions and quantum gravity duality
Abstract
A new formalism is introduced describe the physical and geometric content of quantum spacetime. It is based in the Minimum Group Representation Principle. New results for entanglement and geometrical/topological phases are found and implemented in cosmological and black hole space-times. Our main results here are: (i) The Berry phases for inflation, for the cosmological perturbations, and its expression in terms of observables, as the spectral scalar and tensor indices, an , and their ratio . The Berry phase for de Sitter inflation is imaginary, its sign describing the exponential acceleration. (ii) The pure entangled states in the minimum group (metaplectic) representation for quantum de Sitter space-time and black holes are found. (iii) For entanglement, the relation between the Schmidt type representation and the physical states of the group is found:…
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.
