A radiation-like era before inflation
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We show that the semiclassical approximation to the Wheeler-DeWitt equation for the minisuperspace of a minimally coupled scalar field in the spatially flat de Sitter Universe prompts the existence of an initial power-law evolution driven by non-adiabatic terms from the gravitational wavefunction which act like radiation. This simple model hence describes the onset of inflation from a previous radiation-like expansion during which the cosmological constant is already present but subleading.
LaTeX, 8 pages, no figures; final version to be published in JCAP
LaTeX, 8 pages, no figures; final version to be published in JCAP