A microscopic model of de Sitter spacetime with an observer
Damiano Tietto, Herman Verlinde
TL;DR
The paper presents a microscopic quantum-mechanical model of de Sitter holography with an observer, deriving a total entropy formula for a 3D Schwarzschild–de Sitter patch plus the observer and matching it to the DSSYK spectral density. By introducing an observer, the authors obtain a maximal entropy $S_{ m max}(ψ)=S_{ m GH}(ψ)+β_{ m dS}E(ψ)$ and show that the DSSYK entropy satisfies $S_{ m SYK}(ψ)=S_0+S_{ m max}(ψ)$ with $λ=8π G_N$, effectively linking the deficit-angle parameter to the DSSYK thermodynamics. This yields a de Sitter interpretation of the DSSYK spectral density and explains the appearance of two inverse temperatures, connected via $β_{ m GH}=(2π/ψ)β_{ m max}$, aligning physical and fake temperatures within the dual picture. The result strengthens the gravity–SYK correspondence in low dimensions and motivates further exploration of 2D gravity reductions as natural duals.
Abstract
We introduce a simple microscopic quantum mechanical model of low-dimensional de Sitter holography with an observer. Using semiclassical gravity and elementary thermodynamic considerations, we derive a formula for the total entropy of a 3D Schwarzschild-de Sitter universe with an observer. We then match this entropy formula with the exactly known spectral density of the double scaled SYK model. Our result gives a de Sitter interpretation of the appearance of two notions of temperature in DSSYK.
