Effects of a Geometrically Realized Early Dark Energy Era on the Spectrum of Primordial Gravitational Waves
V.K. Oikonomou, Eirini C. Lymperiadou

TL;DR
This paper explores how a geometrically generated early dark energy era influences the primordial gravitational wave spectrum, showing potential detectability and dependence on the dark energy parameters and reheating temperatures.
Contribution
It introduces a model where early dark energy generated by $f(R)$ gravity amplifies primordial gravitational waves, with detailed analysis of parameter effects on the spectrum.
Findings
Amplification of gravitational wave spectrum depends on dark energy equation of state.
Largest amplification occurs near $w=-1$ and specific temperature ranges.
Detectable signals are predicted for various reheating temperatures.
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 it to have a constant equation of state parameter , is synergistically generated by an appropriate gravity in the presence of matter and radiation perfect fluids. As we demonstrate, the predicted signal for the energy spectrum of the 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 most latter affecting more crucially the amplification. Specifically the amplification occurs when the equation of state parameter approaches the de Sitter…
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Taxonomy
TopicsCosmology and Gravitation Theories · Pulsars and Gravitational Waves Research · Geophysics and Gravity Measurements
