A search for the fine-structure constant evolution from fast radio bursts and type Ia supernovae data

Abstract

The search for a space-time variation of the fundamental constants has been explored over the years to test our physical theories. In this paper, we use the dispersion measure ($DM$) of fast radio bursts (FRB) combined with type Ia supernovae (SNe) data to investigate a possible redshift evolution of the fine-structure constant ($\alpha$), considering the runaway dilaton scenario, which predicts $\frac{\Delta \alpha }{\alpha }=-\gamma \ln (1+z)$, where $\gamma$ is a constant proportional to the current value of the coupling between the dilaton field and hadronic matter. We derive all the relevant expressions for the $DM$ dependence concerning the fine-structure constant and constrain the parameter $\gamma$ from measurements of 17 well-localized FRBs and 1048 SNe data from the Pantheon compilation. We also use Monte Carlo simulations to forecast the constraining power of larger samples of FRB measurements for data sets with $N=500$ and $N=1000$ points. We found that the uncertainty on $\gamma$ can be improved by one order of magnitude and that limits on $\frac{\Delta \alpha }{\alpha }$ beyond $\sigma \sim 10^{-2}$ will depend crucially on better control of statistical and systematic uncertainties of upcoming FRB data.

19 pages, 4 figures, 3 tables

References in corpus (78)

• emcee: The MCMC Hammer
• Cosmic Star Formation History
• The ATNF Pulsar Catalogue
• The Complete Light-curve Sample of Spectroscopically Confirmed Type Ia Supernovae from Pan-STARRS1 and Cosmological Constraints from The Combined Pantheon Sample
• Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM
• A bright millisecond radio burst of extragalactic origin
• Search for New Physics with Atoms and Molecules
• The fundamental constants and their variation: observational status and theoretical motivations
• A New Electron Density Model for Estimation of Pulsar and FRB Distances
• A Population of Fast Radio Bursts at Cosmological Distances
• The direct localization of a fast radio burst and its host
• Varying constants, Gravitation and Cosmology
• A census of baryons in the Universe from localized fast radio bursts
• One percent determination of the primordial deuterium abundance
• FRBCAT: The Fast Radio Burst Catalogue
• A Living Theory Catalogue for Fast Radio Bursts
• Reconstruction of dark energy and expansion dynamics using Gaussian processes
• A repeating fast radio burst source localised to a nearby spiral galaxy
• A single fast radio burst localized to a massive galaxy at cosmological distance
• Violations of the equivalence principle in a dilaton-runaway scenario
• Runaway dilaton and equivalence principle violations
• Detection of Extended He II Reionization in the Temperature Evolution of the Intergalactic Medium
• A fast radio burst localised to a massive galaxy
• The low density and magnetization of a massive galaxy halo exposed by a fast radio burst
• Australian Square Kilometre Array Pathfinder: I. System Description
• A real-time fast radio burst: polarization detection and multiwavelength follow-up
• New varying speed of light theories
• Cosmological implications of Fast Radio Burst / Gamma-Ray Burst Associations
• Host Galaxy Properties and Offset Distributions of Fast Radio Bursts: Implications for their Progenitors
• A nearby repeating fast radio burst in the direction of M81
• Characterizing the FRB host galaxy population and its connection to transients in the local and extragalactic Universe
• Changing alpha With Time: Implications For Fifth-Force-Type Experiments And Quintessence
• The host galaxies and progenitors of Fast Radio Bursts localized with the Australian Square Kilometre Array Pathfinder
• The status of varying constants: a review of the physics, searches and implications
• Bounds on the possible evolution of the Gravitational Constant from Cosmological Type-Ia Supernovae
• Updated fundamental constant constraints from Planck 2018 data and possible relations to the Hubble tension
• Fast Radio Burst/Gamma-Ray Burst Cosmography
• A measurement of Hubble's Constant using Fast Radio Bursts
• Probing the Intergalactic Medium with Fast Radio Bursts
• An 8\% Determination of the Hubble Constant from localized Fast Radio Bursts
• Future Cosmological Constraints from Fast Radio Bursts
• A Local Universe Host for the Repeating Fast Radio Burst FRB 20181030A
• A Distant Fast Radio Burst Associated to its Host Galaxy with the Very Large Array
• Extragalactic dispersion measures of fast radio bursts
• Quintessence Cosmology and Varying $\alpha$
• High-precision limit on variation in the fine-structure constant from a single quasar absorption system
• Breaking of the equivalence principle in the electromagnetic sector and its cosmological signatures
• Blinkverse: A Database of Fast Radio Bursts
• A luminous fast radio burst that probes the Universe at redshift 1
• The Large Dispersion and Scattering of FRB 20190520B are Dominated by the Host Galaxy
• Cosmology-independent estimate of the fraction of baryon mass in the IGM from fast radio burst observations
• Model-independent constraints on the cosmic opacity
• Late-time cosmology of scalar-tensor theories with universal multiplicative coupling between the scalar field and the matter Lagrangian
• Exacerbating the cosmological constant problem with interacting dark energy
• Evolution of the fine-structure constant in runaway dilaton models
• Cosmology with Gravitational Wave/Fast Radio Burst Associations
• Statistical modelling of the cosmological dispersion measure
• Varying fundamental constants principal component analysis: additional hints about the Hubble tension
• Fundamental cosmology in the E-ELT era: The status and future role of tests of fundamental coupling stability
• Primordial nucleosynthesis with varying fundamental constants: Solutions to the Lithium problem and the Deuterium discrepancy
• Constraint on the time variation of the fine-structure constant with the SDSS-III/BOSS DR12 quasar sample
• Fast Radio Burst Dispersion Measure Distribution as a Probe of Helium Reionization
• Variation in the fine-structure constant, distance-duality relation and the next generation of high-resolution spectrograph
• Galaxy clusters and a possible variation of the fine structure constant
• Constraints on a possible variation of the fine structure constant from galaxy cluster data
• Big Bang Nucleosynthesis constraints on varying electron mass solution to the Hubble tension
• Probing spatial variation of the fine-structure constant using the CMB
• Variations in fundamental constants at the cosmic dawn
• Cosmological model-independent constraints on the baryon fraction in the IGM from fast radio bursts and supernovae data
• Primordial nucleosynthesis with varying fundamental constants: Degeneracies with cosmological parameters
• Consistent Constraints on the Equivalence Principle from localised Fast Radio Bursts
• Variation of the fine structure constant in the light of recent helium abundance measurement
• Limits on evolution of the fine-structure constant in runaway dilaton models from Sunyaev-Zeldovich Observations
• Probing the anisotropic distribution of baryon matter in the Universe using fast radio bursts
• Forecasting constraints on the baryon mass fraction in the IGM from fast radio bursts and type Ia supernovae
• Galaxy dispersion measured by Fast Radio Bursts as a probe of baryonic feedback models
• Cosmological constraints on $\Lambda (\alpha )$CDM models with time-varying fine structure constant
• Variation of fundamental constants and white dwarfs

Cited by in corpus (3)

• The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
• Fast Radio Bursts as probes of the late-time universe: a new insight on the Hubble tension
• Refining fundamental constants with white dwarfs: machine learning informed constraints on fine-structure constant and proton-to-electron mass ratio