Inflation from Supersymmetric Quantum Cosmology - General Relativity and Quantum CosmologyReport as inadecuate




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Abstract: We derive a special scalar field potential using the anisotropic Bianchi typeI cosmological model from canonical quantum cosmology under determinedconditions in the evolution to anisotropic variables $\beta \pm$. In theprocess, we obtain a family of potentials that has been introduced by hand inthe literature to explain cosmological data. Considering supersymmetric quantumcosmology, this family is scanned, fixing the exponential potential as moreviable in the inflation scenario $ m V \phi = V 0 \,e^{-\sqrt{3}\phi}$.



Author: J. Socorro, Marco D'Oleire

Source: https://arxiv.org/







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