Effects of a Geometrically Realized Early Dark Energy Era on the Spectrum of Primordial Gravitational Waves

Abstract

In this work, we investigate the effects of a geometrically generated early dark energy era on the energy spectrum of the primordial gravitational waves. The early dark energy era, which we choose to have a constant equation of state parameter w, is synergistically generated by an appropriate f(R) gravity in the presence of matter and radiation perfect fluids. As we demonstrate, the predicted signal for the energy spectrum of the f(R) primordial gravitational waves is amplified and can be detectable, for various reheating temperatures, especially for large reheating temperatures. The signal amplitude depends on the duration of the early dark energy era and on the value of the dark energy equation of state parameter, with the latter affecting more crucially the amplification. Specifically, the amplification occurs when the equation of state parameter approaches the de Sitter value w=−1. Regarding the duration of the early dark energy era, we find that the largest amplification occurs when the early dark energy era commences at temperature T=0.85 eV until T=7.8 eV. Moreover, we study a similar scenario in which amplification occurs, where the early dark energy era commences at T=0.29 eV and lasts until the temperature is increased by ΔT∼1.7 eV. The discovery of primordial gravitational waves will reveal if several symmetries in the Universe exist or not so this work is important toward revealing the primordial gravitational waves.