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Quantum Fields on Time-Periodic AdS$_3/\mathbb{Z}$

Walker Melton, Andrew Strominger, Tianli Wang

TL;DR

This work constructs quantum field theory on the time-periodic spacetime $AdS_3/\mathbb{Z}$, a model with closed timelike curves, using geometric quantization to overcome obstacles to canonical quantization. The authors identify two invariant symplectic forms corresponding to PT-even and PT-odd principal series representations of $SO(2,2)$, and show that for $m^2<-1$ the theory admits a unitary norm on the unitary principal series. They connect bulk periodic scalar modes to conformal primaries and establish explicit two-point functions on the Lorentzian boundary torus, providing a concrete bulk-to-boundary dictionary. In the context of celestial holography, they relate Klein space reductions to wedge CFT$_2$s, fix normalization constants by consistency with 4D-2D correlators, and show that the 4D S-matrix is dual to a maximally entangled state between the two wedge CFT$_2$s, from which translation invariance emerges. These results illuminate how a CFT$_2$-symmetric, entangled boundary picture can encode bulk physics in a spacetime with CTCs and offer a precise celestial bulk-to-boundary dictionary via wedge holography.

Abstract

We consider a free complex massive scalar on the quotient spacetime AdS$_3/\mathbb{Z}$, which has the isometry group SO(2,2) rather than its universal cover. This problem is of interest as a special example of QFT on a spacetime with closed timelike curves (CTCs), as a new context in which to study generalizations of AdS/CFT and for its role in celestial holography. A basis of time-periodic solutions to the Klein-Gordon wave equation is found in terms of hypergeometric functions. They fall into a PT even and a PT odd principal series representation, rather than the more familiar highest-weight representations of the cover of SO(2,2). For masses below the Breitenlohner-Freedman (BF) bound, the modes fall on the unitary principal series. The presence of CTCs precludes the usual canonical quantization, but geometric quantization, which begins with a symplectic form on the phase space of classical solutions, is applicable. Operators, commutators, an \sot invariant vacuum and a Fock space are constructed and transform like those of a CFT$_2$. The Fock space norm is positive below the BF bound. In celestial holography, AdS$_3/\mathbb{Z}$ arises as leaves of a hyperbolic foliation of Klein space. Our analysis determines new entries in the symmetry-constrained celestial bulk-to-boundary dictionary. In particular the Klein space $\mathcal{S}$-matrix is dual to a maximally entangled state in the tensor product of two copies of the 'wedge CFT$_2$' associated to the timelike and spacelike wedges of Klein space. Translation invariance is not present in the wedge CFT$_2$ itself but emerges as a property of this maximally entangled state.

Quantum Fields on Time-Periodic AdS$_3/\mathbb{Z}$

TL;DR

This work constructs quantum field theory on the time-periodic spacetime , a model with closed timelike curves, using geometric quantization to overcome obstacles to canonical quantization. The authors identify two invariant symplectic forms corresponding to PT-even and PT-odd principal series representations of , and show that for the theory admits a unitary norm on the unitary principal series. They connect bulk periodic scalar modes to conformal primaries and establish explicit two-point functions on the Lorentzian boundary torus, providing a concrete bulk-to-boundary dictionary. In the context of celestial holography, they relate Klein space reductions to wedge CFTs, fix normalization constants by consistency with 4D-2D correlators, and show that the 4D S-matrix is dual to a maximally entangled state between the two wedge CFTs, from which translation invariance emerges. These results illuminate how a CFT-symmetric, entangled boundary picture can encode bulk physics in a spacetime with CTCs and offer a precise celestial bulk-to-boundary dictionary via wedge holography.

Abstract

We consider a free complex massive scalar on the quotient spacetime AdS, which has the isometry group SO(2,2) rather than its universal cover. This problem is of interest as a special example of QFT on a spacetime with closed timelike curves (CTCs), as a new context in which to study generalizations of AdS/CFT and for its role in celestial holography. A basis of time-periodic solutions to the Klein-Gordon wave equation is found in terms of hypergeometric functions. They fall into a PT even and a PT odd principal series representation, rather than the more familiar highest-weight representations of the cover of SO(2,2). For masses below the Breitenlohner-Freedman (BF) bound, the modes fall on the unitary principal series. The presence of CTCs precludes the usual canonical quantization, but geometric quantization, which begins with a symplectic form on the phase space of classical solutions, is applicable. Operators, commutators, an \sot invariant vacuum and a Fock space are constructed and transform like those of a CFT. The Fock space norm is positive below the BF bound. In celestial holography, AdS arises as leaves of a hyperbolic foliation of Klein space. Our analysis determines new entries in the symmetry-constrained celestial bulk-to-boundary dictionary. In particular the Klein space -matrix is dual to a maximally entangled state in the tensor product of two copies of the 'wedge CFT' associated to the timelike and spacelike wedges of Klein space. Translation invariance is not present in the wedge CFT itself but emerges as a property of this maximally entangled state.
Paper Structure (19 sections, 82 equations, 2 figures)

This paper contains 19 sections, 82 equations, 2 figures.

Figures (2)

  • Figure 1: Geometry of ${\rm AdS}_3/{\mathbb{Z}}$
  • Figure 2: A toric Penrose diagram of Klein space. The red lines are ${\rm AdS}_3/{\mathbb{Z}}$ leaves of the foliation of the $-$ wedge with $X^2 < 0$, while the blue lines are those of the $+$ wedge with $X^2 > 0$.