Cited by 7Cosmology and Gravitation TheoriesNoncommutative and Quantum Gravity TheoriesAdvanced Mathematical Theories and Applications

Incompatibility of fine-structure constant variations at recombination with local observations

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Vacher, Léo, Schöneberg, Nils·2024·Physical Review D

Abstract

Some attempts of easing the critical Hubble tension present in modern cosmology have resorted to using variations of fundamental constants, such as the fine-structure constant, at the time of recombination. In this article we demonstrate that there are critical hurdles to construct such viable models using scalar fields, due to the striking precision of local constraints on the fine-structure constant stability. These hurdles demonstrate that in single-field models one has to extremely fine-tune the shape of the potential and/or the initial conditions. Indeed, for single-field models in a potential that is not fine-tuned we can put a generic bound at recombination of $\mathrm{\ensuremath{\Delta}}\ensuremath{\alpha}/\ensuremath{\alpha}<5\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}4}$ (95% CL).

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Crossref · 10.1103/physrevd.109.103520

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  • In single-field models, one has to extremely fine-tune the shape of the potential and/or the initial conditions.

    “In particular they demonstrates that in single-field models one has to extremely fine-tune the shape of the potential and/or the initial conditions.”

    From Fundamental constants: from measurement to the universe, a window on gravitation and cosmology (2025) · cites this paper as Vacher and Schoeneberg 2024

  • On the example of B(φ)F^2 models, Vacher and Schoeneberg (2024) demonstrated that this is a critical hurdle to construct a viable model of varying constant that would resolve the Hubble tension since the field would have to relax rapidly enough to avoid local constraints.

    “On the example of BðuÞF 2 models discussed in Sect.7.4 Vacher and Scho ¨neberg (2024) demonstrated that this is a critical hurdle to construct a viable model of varying constant that would resolve the Hubble tension since the field would have to relax rapidly enough to avoid the local constraints.”

    From Fundamental constants: from measurement to the universe, a window on gravitation and cosmology (2025) · cites this paper as Vacher and Schoeneberg 2024

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Research works printed but not linked: 9

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Cited by

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Authors
Vacher, L., & Schöneberg, N.
Affiliations
  • Scuola Internazionale Superiore di Studi Avanzati (IT)
  • Universitat de Barcelona (ES)
Venue
Physical Review D
Published
2024-05-13
Volume
109
Issue
10
ISSN
  • 2470-0010 (ISSN-L)
  • 2470-0029
OpenAlex
W4392489763
Cited by
7
References
62
Citations by year
2025: 4 · 2024: 3
FWCI
1.32
Type
journal article
Language
en
Open access
Locations
  • Physical review. D/Physical review. D. (publishedVersion)
  • arXiv (Cornell University) (submittedVersion)
  • DIGITAL.CSIC (Spanish National Research Council (CSIC)) (submittedVersion)
  • arXiv (Cornell University)
Funders
  • Agenzia Spaziale Italiana (2020-9-HH.0, 2016-24-H.1-2018)
  • Fundação para a Ciência e a Tecnologia (2022.04048.PTDC)
  • Aix-Marseille Université
  • Ministerio de Ciencia e Innovación (PID 2022-141125NB-I00)
  • Agencia Estatal de Investigación
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
  • Physical Sciences › Physics and Astronomy › Statistical and Nonlinear Physics › Noncommutative and Quantum Gravity Theories
  • Physical Sciences › Physics and Astronomy › Statistical and Nonlinear Physics › Advanced Mathematical Theories and Applications
Keywords
fine-structure constant variation, Hubble tension, recombination epoch, scalar field models, variation of fundamental constants, single-field inflation, initial conditions, cosmological constant problem

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