Reissner-Nordstrom-de Sitter black hole, planar coordinates and dS/CFT

A. Chamblin; A. Strominger; A. Strominger; A.J.M. Medved; A.M. Awad; A.M. Ghezelbash; A.M. Ghezelbash; A.M. Ghezelbash; C. Contopoulos; C.M. Hull; C.M. Hull; D. Kabat; D. Kastor; D.R. Brill; D.R. Brill; D.R. Brill; D.Z. Freedman; Dumitru Astefanesei; E. Halyo; E. Verlinde; E. Witten; E. Witten; Eugen Radu; F. Leblond; F. Leblond; G.W. Gibbons; I.S. Booth; J.B. Hartle; J.D. Brown; J.D. Brown; J.D.E. Creighton; J.M. Maldacena; K.R. Kristjansson; L. Dyson; M.H. Dehghani; M.H. Dehghani; M.R. Setare; O. Aharony; R. Bousso; R. Bousso; R. Bousso; R. Clarkson; R. Emparan; R.B. Mann; R.B. Mann; R.B. Mann; R.C. Myers; R.G. Cai; Robert Mann; S.W. Hawking; T. Banks; T. Maki; T. Shiromizu; U.H. Danielsson; V. Balasubramanian; V. Balasubramanian; V. Balasubramanian; V. Balasubramanian

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Reissner-Nordstrom-de Sitter black hole, planar coordinates and dS/CFT

Abstract

We discuss the Reissner-Nordstrom-de Sitter black holes in the context of dS/CFT correspondence by using static and planar coordinates. The boundary stress tensor and the mass of the solutions are computed. Also, we investigate how the RG flow is changed for different foliations. The Kastor-Traschen multi-black hole solution is considered as well as AdS counterparts of these configurations. In particular, we find that in planar coordinates the black holes appear like punctures in the dual boundary theory.Comment: 30 pages, 3 eps figures, JHEP style v2: new references added, misprints correcte

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