Constraint on the minimally extended varying speed of light using time dilations in type Ia supernovae
arXiv:2302.09735 · doi:10.1093/mnras/stad2084
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, . 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 . However, this ratio is modified in the minimally extended varying speed of light model (meVSL, ) as . 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 () SNe Ia to obtain at the - 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.
version 2 to match the version accepted by MNRAS. 5 pages, 1 figure, 2 tables
References in corpus (4)
Cited by in corpus (11)
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