Codimension two branes in Einstein-Gauss-Bonnet gravity
Creators
- 1. Department of Physics, Nankai University, Tianjin, 300071 (China)
- 2. CCAST (World Laboratory), P.O. Box 8730, Beijing 100080 (China)
- 3. Department of Physics, University of Arizona, Tucson, Arizona 85721 (United States)
Description
Codimension two branes play an interesting role in attacking the cosmological constant problem. Recently, in order to handle some problems in codimension two branes in Einstein gravity, Bostock et al. proposed using six-dimensional Einstein-Gauss-Bonnet (EGB) gravity instead of six-dimensional Einstein gravity. In this paper, we present the solutions of codimension two branes in six-dimensional EGB gravity. We show that Einstein's equations take a factorizable form for a factorized metric tensor ansatz even in the presence of the higher-derivative Gauss-Bonnet term. Especially, a new feature of the solution is that the deficit angle depends on the brane geometry. We discuss the implication of the solution to the cosmological constant problem. We also comment on a possible problem of inflation model building on codimension two branes
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.71.024023;
- arXiv
- arXiv:hep-th/0406170v4;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 71
- Journal Issue
- 2
- Journal Page Range
- p. 024023-024023.7
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 37021033
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
- Descriptors DEI
- COSMOLOGICAL CONSTANT; COSMOLOGY; EINSTEIN FIELD EQUATIONS; GEOMETRY; GRAVITATION; INFLATIONARY UNIVERSE; MANY-DIMENSIONAL CALCULATIONS; MATHEMATICAL SOLUTIONS; MEMBRANES; SPACE-TIME; TENSORS
- Descriptors DEC
- COSMOLOGICAL MODELS; EQUATIONS; FIELD EQUATIONS; MATHEMATICAL MODELS; MATHEMATICS
Optional Information
- Notes
- (c) 2005 The American Physical Society