Constraint on the minimally extended varying speed of light using time dilations in type Ia supernovae

Abstract

The Friedmann-Lemaître-Robertson-Walker model establishes the correlation between redshifts and distances. It has a metric expansion of space. As a result, the wavelength of photons propagating through the expanding space is stretched, creating the cosmological redshift, $z$. It also relates the frequency of light detected by a local observer to that emitted from a distant source. In standard cosmology (\textit{i.e.}, a constant speed light model), this relation is given by a factor $1/(1+z)$. However, this ratio is modified in the minimally extended varying speed of light model (meVSL, $c=c_0{a}^{b/4}$) as $1/(1+z{)}^{1-b/4}$. This time dilation effect is detected as the observed rate of the time variation in the intensity of emitted radiation. The spectra of type Ia supernovae (SNe Ia) provide a reliable way to measure the apparent aging rate of distant objects. We use data on 13 high-redshift ($0.28\le z\le 0.62$) SNe Ia to obtain $b=0.198\pm 0.415$ at the $1$-$\sigma$ confidence interval. The current data is too sparse to give meaningful constrain on the meVSL and cannot distinguish the meVSL model from the standard model.

arXiv commentversion 2 to match the version accepted by MNRAS. 5 pages, 1 figure, 2 tables

References in corpus (16)

• The Pantheon+ Analysis: Cosmological Constraints
• The Pantheon+ Analysis: The Full Dataset and Light-Curve Release
• Testing General Relativity in Cosmology
• Timescale Stretch Parameterization of Type Ia Supernova B-band Light Curves
• Time Dilation in the Light Curve of the Distant Type Ia Supernovae SN 1995K
• Time Dilation from Spectral Feature Age Measurements of Type Ia Supernovae
• Time Dilation in Type Ia Supernova Spectra at High Redshift
• Optical Variability of Quasars with 20-Year Photometric Light Curves
• Can a changing $\alpha$ explain the Supernovae results?
• A Definitive Measurement of Time Dilation in the Spectral Evolution of the Moderate-Redshift Type Ia Supernova 1997ex
• The minimally extended Varying Speed of Light (meVSL)
• Redshift drift in varying speed of light cosmology
• Cosmology with relativistically varying physical constants
• Constraining minimally extended varying speed of light by cosmological chronometers
• A viable varying speed of light model in the RW metric
• Observational constraints on varying fundamental constants in a minimal CPC model

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• A mechanism to generate varying speed of light via Higgs-dilaton coupling: Theory and cosmological applications
• New analysis of SNeIa Pantheon Catalog: Variable speed of light as an alternative to dark energy
• A Unified Interpretation of Supernova, GRB, and QSO Time Dilation Signals in a Generalized Cosmological Time Framework
• Brans-Dicke-like field for co-varying $G$ and $c$: observational constraints
• Perturbation Theory in the Minimally Extended Varying Speed of Light (meVSL) Model
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