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What is Early Dark Energy Cosmologies Explained about?

This document summarizes a new parameterization for describing dark energy cosmologies that allow for a non-negligible contribution of dark energy even at early times. The parameterization directly models the fractional dark energy density Ωd(a) as a function of scale factor a, rather than the equation of state w(a). This approach has advantages in that it makes the early dark energy density a direct parameter and allows various cosmological quantities to be calculated analytically. The proposed parameteriz

Author

Alberto Gon

Language

EN