One-loop corrections to a scalar field during inflation
David Seery

TL;DR
This paper calculates the main quantum correction to the power spectrum of a light scalar field during single-field slow-roll inflation, providing insights into quantum effects in early universe cosmology.
Contribution
It presents the first detailed calculation of one-loop quantum corrections to a scalar field's power spectrum during inflation.
Findings
Quantum corrections modify the scalar power spectrum.
Results are relevant for understanding primordial fluctuations.
Provides a framework for future quantum cosmology studies.
Abstract
The leading quantum correction to the power spectrum of a gravitationally-coupled light scalar field is calculated, assuming that it is generated during a phase of single-field, slow-roll inflation.
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