Critical points of D-dimensional extended gravities

Journal Article · Tue Mar 15 00:00:00 EDT 2011 · Physical Review. D, Particles Fields

DOI:https://doi.org/10.1103/PHYSREVD.83.061502· OSTI ID:21537481

Deser, S; Haishan, Liu; Lue, H; Pope, C N; Sisman, Tahsin Cagri; Tekin, Bayram ^[1]

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1. Physics Department, Brandeis University, Waltham, Massachusetts 02454 (United States) and Lauritsen Laboratory, California Institute of Technology, Pasadena, California 91125 (United States)

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{sup 2} model with a unique vacuum, whose {Lambda} is determined.

• OSTI ID: 21537481
• Journal Information: Physical Review. D, Particles Fields, Vol. 83, Issue 6; Other Information: DOI: 10.1103/PhysRevD.83.061502; (c) 2011 American Institute of Physics; ISSN 0556-2821
• Country of Publication: United States
• Language: English

Related Subjects

72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
ANTI DE SITTER SPACE
BLACK HOLES
COSMOLOGICAL MODELS
CRITICALITY
EXCITATION
GENERAL RELATIVITY THEORY
GRAVITATION
GRAVITONS
MANY-DIMENSIONAL CALCULATIONS
ELEMENTARY PARTICLES
ENERGY-LEVEL TRANSITIONS
FIELD THEORIES
GRAVITATIONAL RADIATION
MASSLESS PARTICLES
MATHEMATICAL MODELS
MATHEMATICAL SPACE
POSTULATED PARTICLES
RADIATIONS
RELATIVITY THEORY
SPACE