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    Vacuum polarization effects during the reheating epoch

    A. B. Arbuzov1,2 and A. A. Nikitenko1

    Phys. Rev. D 113, 025008 – Published 20 January, 2026

    DOI: https://doi.org/10.1103/wdz1-gytd

    Abstract

    Quantum effects in the era of reheating of the Universe after inflation are considered. A semiclassical approach to gravity theory is applied within Starobinsky’s inflationary model with backreaction. Some subtleties associated with accounting for quantum effects in the one-loop approximation are clarified. An estimate of the contribution of vacuum polarization in the stress-energy tensor of matter fields to the cosmological particle creation due to the scalaron decay is presented.

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