Skip to content
DraconiticResearch
Search Sources API
206,690 studies31 sourcesUpdated 28 min ago
PreprintCC BY 4.0arXiv

Background-independent one-loop renormalization of tensor and scalar primordial spectra

Abstract

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.

Versions

Related

  1. 2% determination of N eff from primordial element abundance, cosmic microwave background, and baryon acoustic oscillation measurements
    Samuel Goldstein, J. Colin Hill
    Physical review. D/Physical review. D.Peer-reviewedLicence not statedFull text22 citedCosmologyOpenAlex
  2. Thermalization of the Primordial Stochastic Gravitational-Wave Background
    Hongguang Zhang, Zhengyang Qiu, Sirui Wang +1
    arXivPreprintCC BY 4.0Full textCosmologyHigh-energy & particle physicsarXiv
  3. A consistent, physical, and analytical model for cosmic microwave background observables of reionisation. I. Derivation, constraining power, and detectability of the auto spectra
    Adélie Gorce
    Astronomy & AstrophysicsPeer-reviewedPublisher termsCosmologyCrossref
  4. Distinguishing cosmology, astrophysics and systematics: the Bayesian search for a primordial gravitational-wave background in next-generation observatories
    Teagan A. Clarke, Sylvia Biscoveanu, Carl-Johan Haster
    arXivPreprintarXiv licenceFull textHigh-energy astrophysicsGravitation & general relativityarXiv
  5. Primordial tensor mode from the neutrino sector
    Shohei Saga, Shuichiro Yokoyama
    arXivPreprintarXiv licenceFull textCosmologyarXiv
BibTeX
@misc{ballesteros2026backgroundindependent,
  title = {{Background-independent one-loop renormalization of tensor and scalar primordial spectra}},
  author = {Guillermo Ballesteros and Jesús Gambín Egea and Flavio Riccardi},
  howpublished = {arXiv},
  year = {2026},
  month = nov,
  doi = {10.48550/arxiv.2607.06042},
  eprint = {2607.06042},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2607.06042},
  note = {CC BY 4.0},
}
RIS
TY  - UNPB
TI  - Background-independent one-loop renormalization of tensor and scalar primordial spectra
AU  - Guillermo Ballesteros
AU  - Jesús Gambín Egea
AU  - Flavio Riccardi
PY  - 2026
DA  - 2026/11/09
PB  - arXiv
DO  - 10.48550/arxiv.2607.06042
UR  - https://arxiv.org/abs/2607.06042
AB  - 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.
ER  -