Exact and Slow-Roll Solutions for Exponential Power-Law Inflation Connected with Modified Gravity and Observational Constraints
We investigate the ability of the exponential power-law inflation to be a phenomenologically correct model of the early universe. We study General Relativity (GR) scalar cosmology equations in Ivanov–Salopek–Bond (or Hamilton–Jacobi like) representation where the Hubble parameter <i>H</i>...
Main Authors: | , |
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Format: | Article |
Language: | English |
Published: |
MDPI AG
2020-10-01
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Series: | Universe |
Subjects: | |
Online Access: | https://www.mdpi.com/2218-1997/6/11/199 |