Inflation via logarithmic entropy-corrected holographic dark energy model
arXiv:1610.03304 · doi:10.1140/epjc/s10052-016-4556-0
Abstract
We study the inflation via logarithmic entropy-corrected holographic dark energy LECHDE model with future event horizon, particle horizon and Hubble horizon cut-offs, and compare the results with those of obtained in the study of inflation by holographic dark energy HDE model. In comparison, the spectrum of primordial scalar power spectrum in the LECHDE model becomes redder than the spectrum in HDE model. Moreover, the consistency with the observational data in LECHDE model of inflation, constrains the reheating temperature and Hubble parameter by one parameter of holographic dark energy and two new parameters of logarithmic corrections.
11 pages, 10 figures
References in corpus (9)
- Dynamics of dark energy
- Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
- A New Model of Agegraphic Dark Energy
- Quantum Tunneling and Back Reaction
- Holographic tachyon model of dark energy
- Black hole quantum tunnelling and black hole entropy correction
- Entropy-Corrected Holographic Dark Energy
- Inflation with Holographic Dark Energy
- Inflation with High Derivative Couplings