Cosmological significance of one-loop effective gravity
D. Espriu, T. Multamaki, E. C. Vagenas

TL;DR
This paper investigates quantum corrections to Einstein's gravity in a cosmological context, revealing that non-local quantum effects can significantly influence early universe inflation dynamics.
Contribution
It demonstrates the potential importance of non-local quantum gravity effects during the inflationary phase of the early universe.
Findings
Non-local terms become significant during inflation.
Quantum corrections can cause deviations from standard inflation.
Early universe dynamics are affected by quantum gravity effects.
Abstract
We study the one-loop effective action for gravity in a cosmological setup to determine possible cosmological effects of quantum corrections to Einstein theory. By considering the effect of the universal non-local terms in a toy model, we show that they can play an important role in the very early universe. We find that during inflation, the non-local terms are significant, leading to deviations from the standard inflationary expansion.
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