Holographic warm inflation

The increasing interest in studying the role of holographic dark energy evolution very early Universe motivates us to study it for scenario warm inflation. Because this scenario, energy, which now drives inflation, has an interaction with radiation. case interacting also received late time cosmology. infrared cutoff is taken as Hubble length, and all corrections are assumed be exhibited by parameter $c$, appears energy. By comparing predictions model observational data, free constants could determined. Then, using these values constants, density inflation estimated. Next, we consider validity fundamental assumptions e.g., $T/H>1$, necessary held during obtained constant. Gathering outcomes, counted a suitable candidate