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

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arxiv hep-th/0310273 v2 pith:UQT5ATES submitted 2003-10-29 hep-th gr-qc

Dumitru Astefanesei , Robert Mann , Eugen Radu This is my paper · ORCID
classification hep-thgr-qc
keywords blackcoordinatesplanarboundaryholeholesreissner-nordstrom-desitter
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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.

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  1. De Sitter space constraints on brane tensions and couplings

    hep-th 2024-11 conditional novelty 6.0 of 10

    The Festina Lente bound on particle masses is generalized to p-branes with world-volume Chern-Simons couplings, giving tension bounds in de Sitter space that string theory D-branes satisfy.

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