Brans-Dicke-like field for co-varying and : observational constraints
arXiv:2509.09211 · doi:10.1093/mnras/stag391
Abstract
Ref. [Symmetry 15 (2023) 709] introduced a Brans-Dicke-like framework wherein the scalar field is composed of both and which, for this reason, co-vary according to . In this paper, we use observational data to constrain the supposed co-varying and , under the hypothesis of the validity of the standard Lemaitre formula . The datasets include SN Ia, BAO and the value of extracted from CMB data. A proxy function is demanded for the varying since the framework does not provide a closed set of equations for computing the functional form of either or uniquely. Accordingly, we choose three separate parameterizations for inspired both by desirable properties of the varying speed of light (VSL) and by successful phenomenological models from the literature -- including the one by Gupta (CCC framework in e.g. Ref. [Mon. Not. R. Astron. Soc., 498 (2020) 4481-4491]. When combined with DESI, Pantheon+ data strongly favor a variable speed of light with more than confidence level for all parameterizations considered in this paper, whereas Union2.1 suggests no variation of the speed of light. As we shall demonstrate, this apparent discrepancy is due to a strong correlation that emerges between and VSL.
arXiv comment25 pages, 8 figures, 2 tables
References in corpus (51)
- f(R) Theories Of Gravity
- In the Realm of the Hubble tension a Review of Solutions
- The Hubble Space Telescope Cluster Supernova Survey: V. Improving the Dark Energy Constraints Above z>1 and Building an Early-Type-Hosted Supernova Sample
- The Pantheon+ Analysis: Cosmological Constraints
- DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations
- Measuring the Baryon Acoustic Oscillation scale using the SDSS and 2dFGRS
- Cosmological implications of baryon acoustic oscillation (BAO) measurements
- Varying constants, Gravitation and Cosmology
- The Hubble Hunter's Guide
- Measurements of the Hubble Constant: Tensions in Perspective
- Beyond CDM: Problems, solutions, and the road ahead
- New physics in light of the tension: an alternative view
- A time varying speed of light as a solution to cosmological puzzles
- Curvature tension: evidence for a closed universe
- Cosmologies with Varying Light-Speed
- emcee v3: A Python ensemble sampling toolkit for affine-invariant MCMC
- GetDist: a Python package for analysing Monte Carlo samples
- Why reducing the cosmic sound horizon alone can not fully resolve the Hubble tension
- `c' is the speed of light, isn't it?
- Varying- Theories and Solutions to the Cosmological Problems
- Early modified gravity in light of the tension and LSS data
- Scalar-tensor theories of gravity, neutrino physics, and the tension
- JWST early Universe observations and ΛCDM cosmology
- Recombination-independent determination of the sound horizon and the Hubble constant from BAO
- BAO+BBN revisited -- Growing the Hubble tension with a 0.7km/s/Mpc constraint
- The minimally extended Varying Speed of Light (meVSL)
- Cosmology with relativistically varying physical constants
- Introduction to modified gravity
- Effect of evolutionary physical constants on type-1a supernova luminosity
- A search for the variation of speed of light using galaxy cluster gas mass fraction measurements
- Covariant c-flation: a variational approach
- Galaxy clusters and a possible variation of the fine structure constant
- Testing CCC+TL Cosmology with Observed BAO Features
- Dynamical analysis of the covarying coupling constants in scalar-tensor gravity
- Constraining minimally extended varying speed of light by cosmological chronometers
- Varying Coupling Constants and Their Interdependence
- Testing a varying- model for dark energy within Co-varying Physical Couplings framework
- Constraint on the minimally extended varying speed of light using time dilations in type Ia supernovae
- Observational constraints on varying fundamental constants in a minimal CPC model
- Sound-Horizon-Agnostic Inference of the Hubble Constant and Neutrino Mass from BAO, CMB Lensing, and Galaxy Weak Lensing and Clustering
- Shadows of black holes at cosmological distances in the co-varying physical couplings framework
- Constraining Coupling Constants' Variation with Supernovae, Quasars, and GRBs
- Non-parametric reconstruction of the fine structure constant with galaxy clusters
- Cosmography of the minimally extended Varying Speed of Light Model
- 3+1 formalism of the minimally extended varying speed of light model
- Dilaton-induced variations in Planck constant and speed of light: An alternative to Dark Energy
- An investigation of a varying G through Strong Lensing and SNe Ia observations
- New analysis of SNeIa Pantheon Catalog: Variable speed of light as an alternative to dark energy
- A mechanism to generate varying speed of light via Higgs-dilaton coupling: Theory and cosmological applications
- Constraining Co-Varying Coupling Constants from Globular Cluster Age
- Perturbation Theory in the Minimally Extended Varying Speed of Light (meVSL) Model