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Critical points of D-dimensional extended gravities
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Date
2011-03-17
Author
Deser, S.
Liu, Haishan
Lue, H.
Pope, C. N.
Sisman, Tahsin Cagri
Tekin, Bayram
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Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License
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We study the parameter space of D-dimensional cosmological Einstein gravity together with quadratic curvature terms. In D < 4 there are in general two distinct (anti)-de Sitter vacua. We show that, for an appropriate choice of the parameters, there exists a critical point for one of the vacua, with only massless tensor, but neither massive tensor nor scalar, gravitons. At criticality, the linearized excitations have formally vanishing energy (as do black hole solutions). A further restriction of the parameters gives a one-parameter cosmological Einstein plus Weyl(2) model with a unique vacuum, whose Lambda is determined.
Subject Keywords
Massive Gauge
,
Theories
URI
https://hdl.handle.net/11511/41446
Journal
PHYSICAL REVIEW D
DOI
https://doi.org/10.1103/physrevd.83.061502
Collections
Department of Physics, Article
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S. Deser, H. Liu, H. Lue, C. N. Pope, T. C. Sisman, and B. Tekin, “Critical points of D-dimensional extended gravities,”
PHYSICAL REVIEW D
, pp. 0–0, 2011, Accessed: 00, 2020. [Online]. Available: https://hdl.handle.net/11511/41446.