4.6 Article

The minimally extended Varying Speed of Light (meVSL)

Journal

Publisher

IOP Publishing Ltd
DOI: 10.1088/1475-7516/2021/08/054

Keywords

cosmology of theories beyond the SM; dark energy theory; gravitational waves / theory; Sunyaev-Zeldovich effect

Funding

  1. Basic Science Research Program through the National Research Foundation of Korea (NRF) - Ministry of Science, ICT and Future Planning [NRF-2017R1A2B4011168]

Ask authors/readers for more resources

The minimally extended VSL (meVSL) model proposed in the paper may have important implications in cosmology, offering new solutions to various problems of the standard ΛCDM model.
Even though there have been various models of the time-varying speed of light (VSL), they remain out of the mainstream because of their possible violation of physics laws built into fundamental physics. In order to be the VSL as a viable theory, it should inherit the success of special relativity including Maxwell equations and thermodynamics at least. For this purpose, we adopt the assumption that the speed of light, (c) over tilde, i.e., (c) over tilde [a], varies for the scale factor, a. The background FLRW universe can be defined by the constant cosmic time hypersurface using physical quantities such as temperature, density, (c) over tilde, etc. It is because they evolve in cosmic time and the homogeneity of the Universe demands that they must equal at the equal cosmic time. The variation of (c) over tilde accompanies the joint variations of all related physical constants in order to satisfy the Lorentz invariance, thermodynamics, Bianchi identity, etc. We dub this VSL model as a minimally extended VSL (meVSL). We derive cosmological observables of meVSL and obtain the constraints on the variation of (c) over tilde by using current cosmological observations. Interestingly, both the cosmological redshift z and all geometrical distances except the luminosity distance of meVSL are the same as those of general relativity. However, the Hubble parameter of meVSL is rescaled as H(z) = (1+z)(-b/4) H-(GR)(z), where H-(GR)(z) denotes the Hubble parameter obtained from general relativity. Thus, it might be used as an alternative solution for the tension of the Hubble parameter measurements. In this manuscript, we provide the main effects of the meVSL model on various cosmological observations including BBN, CMB, SZE, BAO, SNe, GWs, H, SL, and Delta alpha. Compared to previous VSL models, meVSL might provide alternative solutions for various late time problems of the standard Lambda CDM model. This is the main motivation for proposing the meVSL model.

Authors

I am an author on this paper
Click your name to claim this paper and add it to your profile.

Reviews

Primary Rating

4.6
Not enough ratings

Secondary Ratings

Novelty
-
Significance
-
Scientific rigor
-
Rate this paper

Recommended

No Data Available
No Data Available