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On the local term in the anomaly-induced action of Weyl quantum gravity
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abstract
The finite local conformally non-invariant $R^2$-term emerges in the one-loop effective action of the model of quantum gravity based on the Weyl-squared classical action. This term is related to the $\Box R$ contribution to the conformal anomaly, which in a wide class of regularization schemes is determined by the second Schwinger-DeWitt (or Gilkey-Seeley) coefficient of the heat kernel expansion for inverse propagators of the theory. The calculation of this term requires evaluating the contributions of the fourth-order derivative minimal and of the second-order nonminimal operators in the tensor and vector sectors of the theory, corresponding to metric, ghost and gauge-fixing operators. To ensure the correctness of existing formulas, we derived (and confirmed) the result using a special technique of calculations, based on the heat-kernel representation of the Euclidean Green's function and the method of universal functional traces.
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Bounce solutions with quantum vacuum effects of massive fields and subsequent Starobinsky inflation
Quantum trace anomaly effects can produce a nonsingular cosmological bounce, and adding an R-squared term yields a trans-Planckian bounce followed by Starobinsky inflation.
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