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Quantum cosmology in 2+1 and 3+1 dimensions
Authors:Tom Banks  W Fischler  Leonard Susskind
Institution:Stanford Linear Accelerator Center, Stanford University, Stanford, California 94305, USA;Department of Physics, University of Texas, Austin, Texas 78712, USA;Department of Physics, Stanford University, Stanford, California 94305, USA
Abstract:We study the Wheeler-DeWitt equations for the wave function of the universe in 2+1 and 3+1 dimensions. Perturbation methods are developed and the first few orders areexplicitly calculated for the case of an inflating universe. We find that early quantum fluctuation can produce large-scale inhomogenities in the global structure of the universe at later times.
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