Quantum Fluctuations and Newton-Cartan Geometry for Non-Relativistic de Sitter space

Fuente: arXiv
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Auteurs principaux: Harksen, Matthias, Hidalgo, Diego, Sybesma, Watse
Format: Preprint
Publié: 2026
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author Harksen, Matthias
Hidalgo, Diego
Sybesma, Watse
author_facet Harksen, Matthias
Hidalgo, Diego
Sybesma, Watse
contents We study a non-relativistic realisation of two-dimensional de Sitter gravity both from its boundary and bulk description with the goal of learning about de Sitter space and paving the way for extending the holographic duality into a non-relativistic direction. On the boundary side, we analyse the Schwarzian-type boundary action associated with non-relativistic de Sitter gravity and evaluate its one-loop partition function in order to compute its quantum fluctuations. Rather than relying on the coadjoint-orbit construction, we derive the path integral measure directly from the action using the Ostrogradsky formalism. We find a temperature-dependent prefactor scaling as $T^2$, of which the power agrees with the counting of the four global symmetry generators present. On the bulk side, we construct the corresponding torsionless Newton-Cartan geometry and show that it satisfies the equations of motion of a non-relativistic JT-like action and uplift the geometry to a three-dimensional Lorentzian geometry.
format Preprint
id arxiv_https___arxiv_org_abs_2604_07449
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Quantum Fluctuations and Newton-Cartan Geometry for Non-Relativistic de Sitter space
Harksen, Matthias
Hidalgo, Diego
Sybesma, Watse
High Energy Physics - Theory
We study a non-relativistic realisation of two-dimensional de Sitter gravity both from its boundary and bulk description with the goal of learning about de Sitter space and paving the way for extending the holographic duality into a non-relativistic direction. On the boundary side, we analyse the Schwarzian-type boundary action associated with non-relativistic de Sitter gravity and evaluate its one-loop partition function in order to compute its quantum fluctuations. Rather than relying on the coadjoint-orbit construction, we derive the path integral measure directly from the action using the Ostrogradsky formalism. We find a temperature-dependent prefactor scaling as $T^2$, of which the power agrees with the counting of the four global symmetry generators present. On the bulk side, we construct the corresponding torsionless Newton-Cartan geometry and show that it satisfies the equations of motion of a non-relativistic JT-like action and uplift the geometry to a three-dimensional Lorentzian geometry.
title Quantum Fluctuations and Newton-Cartan Geometry for Non-Relativistic de Sitter space
topic High Energy Physics - Theory
url https://arxiv.org/abs/2604.07449