# Shadows and deflection angle of charged and slowly rotating black holes   in Einstein-{\AE}ther theory

**Authors:** Tao Zhu, Qiang Wu, Mubasher Jamil, Kimet Jusufi

arXiv: 1906.05673 · 2019-09-04

## TL;DR

This paper investigates how the Einstein-{	ext{"A}}}ther field influences the shadow size and light deflection of charged, slowly rotating black holes, providing observational constraints and analyzing the effects of specific aether parameters.

## Contribution

It introduces a detailed analysis of black hole shadows and light deflection in Einstein-{	ext{"A}}}ther theory for two specific parameter combinations, linking theoretical predictions with observational data.

## Key findings

- Shadow size increases with c_{13} for both black hole types.
- Shadow size decreases with c_{14} for the second type black hole.
- Deflection angle and time delay are slightly affected by aether parameters.

## Abstract

In this paper, we study the shadow cast by two types of charged and slowly rotating black holes in Eisntein-aether theory of gravity. This two types of black holes are corresponding to two specific combinations of the coupling constants of the aether field, i.e., $c_{14} = 0$ but $c_{123}\neq 0$ for the first type and $c_{123} = 0$ for the second type, respectively. For both types of black holes, in addition to the mass and charge of the black holes, we show that the presence of the aether field can also affect the size of the shadow. For the first type black hole, it is shown that the shadow size increases with the parameter $c_{13}$, while for the second type black hole, the shadow size still increases with c13 but decreases with the parameter $c_{14}$. With these properties of these aether parameters, we also discuss the observational constraints on these parameters by using the data of the first black hole image by the Event Horizon Telescope. In addition, we also explore the effect of the aether field on the the deflection angle of light and the time delay by using the Gauss-Bonnet theorem. It is shown that, for a specific combination $c_{123} = 0$, the deflection angle/time delay is slightly affected by the aether parameter $c_{13}$ at the leading order.

## Full text

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## Figures

20 figures with captions in the complete paper: https://tomesphere.com/paper/1906.05673/full.md

## References

74 references — full list in the complete paper: https://tomesphere.com/paper/1906.05673/full.md

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Source: https://tomesphere.com/paper/1906.05673