Shadow and Weak Deflection Angle of a Black Hole in Nonlocal Gravity

Black hole shadow and gravitational lensing play important roles in testing gravitational theories in the strong field regime. As the first-order modifications from quantum gravity, the nonlocality can be manifested by black hole shadow and gravitational lensing. For example, the nonlocal parameter...

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Main Authors: Qi-Ming Fu, Shao-Wen Wei, Li Zhao, Yu-Xiao Liu, Xin Zhang
Format: Article
Language:English
Published: MDPI AG 2022-06-01
Series:Universe
Subjects:
Online Access:https://www.mdpi.com/2218-1997/8/7/341
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author Qi-Ming Fu
Shao-Wen Wei
Li Zhao
Yu-Xiao Liu
Xin Zhang
author_facet Qi-Ming Fu
Shao-Wen Wei
Li Zhao
Yu-Xiao Liu
Xin Zhang
author_sort Qi-Ming Fu
collection DOAJ
description Black hole shadow and gravitational lensing play important roles in testing gravitational theories in the strong field regime. As the first-order modifications from quantum gravity, the nonlocality can be manifested by black hole shadow and gravitational lensing. For example, the nonlocal parameter introduced by nonlocality will affect the shape and size of the black hole shadow, and also affect the deflection angle of light rays. In this paper, we mainly investigate the effects of the nonlocality on the black hole shadow and the gravitational lensing for two types of rotating black holes in nonlocal gravity. It is found that the size of the black hole shadow decreases with the nonlocal parameter since the nonlocality weakens the gravitational constant, and the shape of the shadow becomes more deformed with the increase in the nonlocal parameter. However, if the rotation parameter is small, the shape of the shadow is almost a circle even though the nonlocal parameter approaches its maximum. The energy emission rate in both models is also studied. The results show that there is a peak for each curve and the peak decreases and shifts to the low frequency with the increase in the nonlocal parameter. In addition, we also explore the shadow of both types of black holes surrounded by a nonmagnetized pressureless plasma which satisfies the separability condition. It is found that the plasma has a frequency-dependent dispersive effect on the size and shape of the black hole shadow. For the gravitational lensing, we find that the nonlocal parameter of model A makes a positive contribution to the deflection angle, which can be compared with the contribution of the rotation parameter, while the nonlocal parameter of model B makes a negative contribution which can be ignored. These results may be helpful for probing nonlocal gravity in future observations.
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spelling doaj.art-1eb7b37c9b3f4d6e9f85e95b3aae52112023-12-03T12:21:38ZengMDPI AGUniverse2218-19972022-06-018734110.3390/universe8070341Shadow and Weak Deflection Angle of a Black Hole in Nonlocal GravityQi-Ming Fu0Shao-Wen Wei1Li Zhao2Yu-Xiao Liu3Xin Zhang4Department of Physics, College of Sciences, Northeastern University, Shenyang 110819, ChinaInstitute of Theoretical Physics and Research Center of Gravitation, Lanzhou University, Lanzhou 730000, ChinaInstitute of Theoretical Physics and Research Center of Gravitation, Lanzhou University, Lanzhou 730000, ChinaInstitute of Theoretical Physics and Research Center of Gravitation, Lanzhou University, Lanzhou 730000, ChinaDepartment of Physics, College of Sciences, Northeastern University, Shenyang 110819, ChinaBlack hole shadow and gravitational lensing play important roles in testing gravitational theories in the strong field regime. As the first-order modifications from quantum gravity, the nonlocality can be manifested by black hole shadow and gravitational lensing. For example, the nonlocal parameter introduced by nonlocality will affect the shape and size of the black hole shadow, and also affect the deflection angle of light rays. In this paper, we mainly investigate the effects of the nonlocality on the black hole shadow and the gravitational lensing for two types of rotating black holes in nonlocal gravity. It is found that the size of the black hole shadow decreases with the nonlocal parameter since the nonlocality weakens the gravitational constant, and the shape of the shadow becomes more deformed with the increase in the nonlocal parameter. However, if the rotation parameter is small, the shape of the shadow is almost a circle even though the nonlocal parameter approaches its maximum. The energy emission rate in both models is also studied. The results show that there is a peak for each curve and the peak decreases and shifts to the low frequency with the increase in the nonlocal parameter. In addition, we also explore the shadow of both types of black holes surrounded by a nonmagnetized pressureless plasma which satisfies the separability condition. It is found that the plasma has a frequency-dependent dispersive effect on the size and shape of the black hole shadow. For the gravitational lensing, we find that the nonlocal parameter of model A makes a positive contribution to the deflection angle, which can be compared with the contribution of the rotation parameter, while the nonlocal parameter of model B makes a negative contribution which can be ignored. These results may be helpful for probing nonlocal gravity in future observations.https://www.mdpi.com/2218-1997/8/7/341black hole shadowgravitational lensingweak deflection anglenonlocal gravity
spellingShingle Qi-Ming Fu
Shao-Wen Wei
Li Zhao
Yu-Xiao Liu
Xin Zhang
Shadow and Weak Deflection Angle of a Black Hole in Nonlocal Gravity
Universe
black hole shadow
gravitational lensing
weak deflection angle
nonlocal gravity
title Shadow and Weak Deflection Angle of a Black Hole in Nonlocal Gravity
title_full Shadow and Weak Deflection Angle of a Black Hole in Nonlocal Gravity
title_fullStr Shadow and Weak Deflection Angle of a Black Hole in Nonlocal Gravity
title_full_unstemmed Shadow and Weak Deflection Angle of a Black Hole in Nonlocal Gravity
title_short Shadow and Weak Deflection Angle of a Black Hole in Nonlocal Gravity
title_sort shadow and weak deflection angle of a black hole in nonlocal gravity
topic black hole shadow
gravitational lensing
weak deflection angle
nonlocal gravity
url https://www.mdpi.com/2218-1997/8/7/341
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AT shaowenwei shadowandweakdeflectionangleofablackholeinnonlocalgravity
AT lizhao shadowandweakdeflectionangleofablackholeinnonlocalgravity
AT yuxiaoliu shadowandweakdeflectionangleofablackholeinnonlocalgravity
AT xinzhang shadowandweakdeflectionangleofablackholeinnonlocalgravity