A Background Independent Algebra in Quantum Gravity
Edward Witten

TL;DR
This paper introduces a background-independent algebra of operators in quantum gravity along an observer's worldline, linking it to the Hartle-Hawking state and defining entropy via relative entropy, especially in de Sitter vacua.
Contribution
It proposes a novel algebraic framework for quantum gravity that is background-independent and connects it to entropy definitions using the Hartle-Hawking state.
Findings
Defines a background-independent algebra of operators in quantum gravity.
Relates the Hartle-Hawking state to maximum entropy.
Provides sensible entropy results for de Sitter vacua.
Abstract
We propose an algebra of operators along an observer's worldline as a background-independent algebra in quantum gravity. In that context, it is natural to think of the Hartle-Hawking no boundary state as a universal state of maximum entropy, and to define entropy in terms of the relative entropy with this state. In the case that the only spacetimes considered correspond to de Sitter vacua with different values of the cosmological constant, this definition leads to sensible results.
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 · Black Holes and Theoretical Physics · Cosmology and Gravitation Theories
