Timelike-bounded dS 4 holography from a solvable sector of the T 2 deformation

Abstract Recent research has leveraged the tractability of T T ¯ $$ T\overline{T} $$ style deformations to formulate timelike-bounded patches of three-dimensional bulk spacetimes including dS 3. This proceeds by breaking the problem into two parts: a solvable theory that captures the most entropic e...

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Main Authors: Eva Silverstein, Gonzalo Torroba
Format: Article
Language:English
Published: SpringerOpen 2025-03-01
Series:Journal of High Energy Physics
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Online Access:https://doi.org/10.1007/JHEP03(2025)156
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author Eva Silverstein
Gonzalo Torroba
author_facet Eva Silverstein
Gonzalo Torroba
author_sort Eva Silverstein
collection DOAJ
description Abstract Recent research has leveraged the tractability of T T ¯ $$ T\overline{T} $$ style deformations to formulate timelike-bounded patches of three-dimensional bulk spacetimes including dS 3. This proceeds by breaking the problem into two parts: a solvable theory that captures the most entropic energy bands, and a tuning algorithm to treat additional effects and fine structure. We point out that the method extends readily to higher dimensions, and in particular does not require factorization of the full T 2 operator (the higher dimensional analogue of T T ¯ $$ T\overline{T} $$ defined in [1]). Focusing on dS 4, we first define a solvable theory at finite N via a restricted T 2 deformation of the CFT 3 on S 2 × ℝ, in which T is replaced by the form it would take in symmetric homogeneous states, containing only diagonal energy density E/V and pressure (-dE/dV) components. This explicitly defines a finite-N solvable sector of dS 4/deformed-CFT3, capturing the radial geometry and count of the entropically dominant energy band, reproducing the Gibbons-Hawking entropy as a state count. To accurately capture local bulk excitations of dS 4 including gravitons, we build a deformation algorithm in direct analogy to the case of dS 3 with bulk matter recently proposed in [2]. This starts with an infinitesimal stint of the solvable deformation as a regulator. The full microscopic theory is built by adding renormalized versions of T 2 and other operators at each step, defined by matching to bulk local calculations when they apply, including an uplift from AdS 4/CFT 3 to dS 4 (as is available in hyperbolic compactifications of M theory). The details of the bulk-local algorithm depend on the choice of boundary conditions; we summarize the status of these in GR and beyond, illustrating our method for the case of the cylindrical Dirichlet condition which can be UV completed by our finite quantum theory.
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spelling doaj-art-45565f2a244f4201b19d7b49d261dac92025-08-20T03:06:48ZengSpringerOpenJournal of High Energy Physics1029-84792025-03-012025312710.1007/JHEP03(2025)156Timelike-bounded dS 4 holography from a solvable sector of the T 2 deformationEva Silverstein0Gonzalo Torroba1Stanford Institute for Theoretical PhysicsCentro Atómico Bariloche, CONICET, and Instituto BalseiroAbstract Recent research has leveraged the tractability of T T ¯ $$ T\overline{T} $$ style deformations to formulate timelike-bounded patches of three-dimensional bulk spacetimes including dS 3. This proceeds by breaking the problem into two parts: a solvable theory that captures the most entropic energy bands, and a tuning algorithm to treat additional effects and fine structure. We point out that the method extends readily to higher dimensions, and in particular does not require factorization of the full T 2 operator (the higher dimensional analogue of T T ¯ $$ T\overline{T} $$ defined in [1]). Focusing on dS 4, we first define a solvable theory at finite N via a restricted T 2 deformation of the CFT 3 on S 2 × ℝ, in which T is replaced by the form it would take in symmetric homogeneous states, containing only diagonal energy density E/V and pressure (-dE/dV) components. This explicitly defines a finite-N solvable sector of dS 4/deformed-CFT3, capturing the radial geometry and count of the entropically dominant energy band, reproducing the Gibbons-Hawking entropy as a state count. To accurately capture local bulk excitations of dS 4 including gravitons, we build a deformation algorithm in direct analogy to the case of dS 3 with bulk matter recently proposed in [2]. This starts with an infinitesimal stint of the solvable deformation as a regulator. The full microscopic theory is built by adding renormalized versions of T 2 and other operators at each step, defined by matching to bulk local calculations when they apply, including an uplift from AdS 4/CFT 3 to dS 4 (as is available in hyperbolic compactifications of M theory). The details of the bulk-local algorithm depend on the choice of boundary conditions; we summarize the status of these in GR and beyond, illustrating our method for the case of the cylindrical Dirichlet condition which can be UV completed by our finite quantum theory.https://doi.org/10.1007/JHEP03(2025)156AdS-CFT Correspondencede Sitter space
spellingShingle Eva Silverstein
Gonzalo Torroba
Timelike-bounded dS 4 holography from a solvable sector of the T 2 deformation
Journal of High Energy Physics
AdS-CFT Correspondence
de Sitter space
title Timelike-bounded dS 4 holography from a solvable sector of the T 2 deformation
title_full Timelike-bounded dS 4 holography from a solvable sector of the T 2 deformation
title_fullStr Timelike-bounded dS 4 holography from a solvable sector of the T 2 deformation
title_full_unstemmed Timelike-bounded dS 4 holography from a solvable sector of the T 2 deformation
title_short Timelike-bounded dS 4 holography from a solvable sector of the T 2 deformation
title_sort timelike bounded ds 4 holography from a solvable sector of the t 2 deformation
topic AdS-CFT Correspondence
de Sitter space
url https://doi.org/10.1007/JHEP03(2025)156
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AT gonzalotorroba timelikeboundedds4holographyfromasolvablesectorofthet2deformation