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The cosmological constant problem in codimension-two brane models
Christof WetterichJan-markus Schwindtsubject
High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsFOS: Physical sciencesNon-standard cosmologyCosmological constantMetric expansion of spaceGeneral Relativity and Quantum Cosmologysymbols.namesakeTheoretical physicsClassical mechanicsHigh Energy Physics - Theory (hep-th)De Sitter universeFriedmann–Lemaître–Robertson–Walker metricBrane cosmologysymbolsBraneCosmological constant problemdescription
We discuss the possibility of a dynamical solution to the cosmological constant problem in the contaxt of six-dimensional Einstein-Maxwell theory. A definite answer requires an understanding of the full bulk cosmology in the early universe, in which the bulk has time-dependent size and shape. We comment on the special properties of codimension two as compared to higher codimensions.
year | journal | country | edition | language |
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2005-08-09 | Physics Letters B |