Double-scaled SYK, Chords and de Sitter Gravity
Herman Verlinde

TL;DR
This paper connects 3D de Sitter gravity with double scaled SYK, showing they share the same energy spectrum and chord rules, and uses this to compute key physical quantities.
Contribution
It identifies the Hamiltonian of 3D de Sitter gravity with a gravitational Wilson-line, matching the double scaled SYK model's spectrum and rules.
Findings
Hamiltonian matches double scaled SYK spectrum
Partition function computed using the SYK correspondence
Scalar two-point function derived in de Sitter gravity
Abstract
We study the partition function of 3D de Sitter gravity defined as the trace over the Hilbert space obtained by quantizing the phase space of non-rotating Schwarzschild-de Sitter spacetime. Motivated by the correspondence with double scaled SYK, we identify the Hamiltonian with the gravitational Wilson-line that measures the conical deficit angle. We express the Hamiltonian in terms of canonical variables and find that it leads to the exact same chord rules and energy spectrum as the double scaled SYK model. We use the obtained match to compute the partition function and scalar two-point function in 3D de Sitter gravity.
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
TopicsHistorical Geography and Cartography
