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arXiv · 2305.11118

Shadows of black holes at cosmological distances in the co-varying physical couplings framework

R. R. Cuzinatto·C. A. M. de Melo·Juliano C. S. Neves
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Abstract

The co-varying physical couplings (CPC) framework states that physical parameters like the speed of light in vacuum $c$, the Newtonian constant $G$, and the cosmological constant $\Lambda$ could indeed vary with the spacetime coordinates $x^{\mu}$. Here, we assume a temporal variation, that is, $c(t),G(t)$ and $\Lambda(t)$. We show that the McVittie spacetime, a black hole in an expanding universe, is a solution of the CPC framework providing naturally an important parameter of the model. Then, we calculate the shadow angular radius of this black hole at cosmological distances. A black hole shadow in the CPC context could be either larger or smaller than the same shadow in the standard cosmology. It depends on how the set $\{ c,G,\Lambda \}$ varies with time or with the cosmic expansion.

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R. R. Cuzinatto, C. A. M. de Melo, Juliano C. S. Neves. 2023-05-18. Shadows of black holes at cosmological distances in the co-varying physical couplings framework. https://doi.org/10.1093/mnras%2Fstad2954

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