Inflation scenario from canonical quantum cosmology

Using the canonical quantization for the flat FRW cosmological model with scalar field and scalar potential V(Ø), we obtain a differential equation for this potential. Also we present the quantum solution for this model, and under the WKB approximation to get the semiclassical formulation, we give a family of potentials. Finally, the classical evolution of the system is given in the inflation scenary.

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Bibliographic Details
Main Authors: Guzmán,W, Sabido,M, Socorro,J, Ureña-López,L. Arturo
Format: Digital revista
Language:English
Published: Sociedad Mexicana de Física 2007
Online Access:http://www.scielo.org.mx/scielo.php?script=sci_arttext&pid=S0035-001X2007001000012
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