Answers are grounded in this paper and cite their sources.
A bstract We present a background-independent renormalization framework for one-loop primordial spectra. We apply it to two observables: the scalar-induced tensor spectrum sourced by a minimally coupled spectator field, and the scalar spectrum generated by potential self-interactions. In both cases, the UV part of the loops is isolated and, using the universal WKB behavior of the internal modes, the UV poles are extracted analytically and absorbed into local counterterms without having to specify either the background evolution or the full dynamics of the field running in the loop. This yields finite model-independent expressions for the renormalized spectra amenable to numerical analysis.
No takes yet. Share an insight, caveat, or question.
Ballesteros et al. (2026) studied this question.
Synapse has enriched 10 related papers. Consider them for comparative context: