Abstract

We model the back-reaction of a static observer in four-dimensional de Sitter spacetime by means of a singular ℤq quotient. The set of fixed points of the ℤq action consists of a pair of codimension two minimal surfaces given by 2-spheres in the Euclidean geometry. The introduction of an orbifold parameter q > 1 permits the construction of an effective action for the bulk gravity theory with support on each of these minimal surfaces. The effective action corresponds to that of Liouville field theory on a 2-sphere with a finite vacuum expectation value of the Liouville field. The intrinsic Liouville theory description yields a thermal Cardy entropy that we reintrepret as a modular free energy at temperature T = q−1, whereupon the Gibbons-Hawking entropy arises as the corresponding modular entropy. We further observe that in the limit q → ∞ the four-dimensional geometry reduces to that of global dS3 spacetime, where the two original minimal surfaces can be mapped to the future and past infinities of dS3 by means of a double Wick rotation. In this limit, the Liouville theories on the minimal surfaces become boundary theories at zero temperature whose total central charge equals that computed using the dS3/CFT2 correspondence.

Highlights

  • The set of fixed points of the Zq action consists of a pair of codimension two minimal surfaces given by 2-spheres in the Euclidean geometry

  • The intrinsic Liouville theory description yields a thermal Cardy entropy that we reintrepret as a modular free energy at temperature T = q−1, whereupon the Gibbons-Hawking entropy arises as the corresponding modular entropy

  • When such back-reaction is taken into account, we shall refer to the static observer as a massive observer, and we shall think of the q → 1 limit as its massless probe limit in which one recovers the original, non-singular dS4 geometry

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Summary

Static observers in dS4

De Sitter spacetime (dS4) can be viewed as a four-dimensional timelike hypersurface embedded in five-dimensional Minkowski space M1,4. Taking the embedding coordinates to be Xμ ∈ M1,4, μ = 0, . 4, and considering the Minkowski metric ds2M1,4 = −(dX0)2 +. The hyperboloid (2.2) has the topology of R × S3 with manifest O(4, 1) symmetries

Massless probe observers
Massive observers and antipodal defects
Liouville theory description of a massive observer
Effective two-dimensional action
On-shell correspondence with Liouville theory
Central charge and Cardy formula
Modular free energy and Gibbons-Hawking entropy
The large q limit and dS3 holography
Conclusions
A Liouville theory
Full Text
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