2003
DOI: 10.1103/physrevd.67.064005
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Elliptic de Sitter space:dS/Z2

Abstract: We propose that for every event in de Sitter space, there is a CPT-conjugate event at its antipode. Such an "elliptic" Z 2 -identification of de Sitter space provides a concrete realization of observer complementarity: every observer has complete information. It is possible to define the analog of an S-matrix for quantum gravity in elliptic de Sitter space that is measurable by all observers. In a holographic description, S-matrix elements may be represented by correlation functions of a dual (conformal field)… Show more

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Cited by 90 publications
(170 citation statements)
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“…However, owing to the validity of the S-Matrix only in the region of space-time that is near the horizon, this identification is presumably valid only in this region. Global identifications of the two exteriors have been considered in the past [60][61][62]. The physics of the scattering, with this identification is now clear.…”
Section: Discussionmentioning
confidence: 99%
“…However, owing to the validity of the S-Matrix only in the region of space-time that is near the horizon, this identification is presumably valid only in this region. Global identifications of the two exteriors have been considered in the past [60][61][62]. The physics of the scattering, with this identification is now clear.…”
Section: Discussionmentioning
confidence: 99%
“…Unlike the black hole membrane paradigm, for which only those observers who remain outside the black hole see a membrane, here every observer has its own stretched horizon. The physical interpretation of the membrane in such a scenario probably involves some form of observer complementarity [28].…”
Section: B De Sitter Spacementioning
confidence: 99%
“…These gravity waves travel on null trajectories with respect to the background metric. Now, if a gravity wave intersects the timelike boundary, its amplitude and derivatives leave a corresponding perturbation on the boundary matter, via (6) and (7), and then (24) and (28).…”
Section: Relation To Cauchy Problemmentioning
confidence: 99%
“…Yet their dual versions, bulk-Bob and bulk-Alice, have a nonzero amplitude to interact in the shared future region. While this may perhaps be possible if we consider a Z 2 identification [42], with excitations also respecting the same identification, it seems hard to understand for the usual eternal BTZ black hole. Conceptual puzzles related to this issue have been raised in [18][19][20] and other puzzles with this picture have been raised in [16].…”
Section: Implications For the Massive Btz Black Holementioning
confidence: 99%