Inflation from Supersymmetric Quantum Cosmology

Abstract

We derive a special scalar field potential using the anisotropic Bianchi type I cosmological model from canonical quantum cosmology under determined conditions in the evolution to anisotropic variables ${\beta }_{\pm }$. In the process, we obtain a family of potentials that has been introduced by hand in the literature to explain cosmological data. Considering supersymmetric quantum cosmology, this family is scanned, fixing the exponential potential as more viable in the inflation scenario $\mathrm{V}(\varphi )={\mathrm{V}}_0{\mathrm{e}}^{-\sqrt{3}\varphi }$.

14 pages, latex2e, To appear in Phys. Rev. D

References in corpus (5)

• Dynamics of dark energy
• What does inflation really predict?
• On the nature of dark matter
• Scalar potentials out of canonical quantum cosmology
• Towards SDp-brane Quantization

Cited by in corpus (5)

• Hamilton's approach in cosmological inflation with an exponential potential and its observational constraints
• Classical and quantum exact solutions for a FRW in chiral like cosmology
• Variable cosmological term $\Lambda (t)$
• Quintom potentials from quantum cosmology using the FRW cosmological model
• Quintom phase-space: beyond the exponential potential