Shadows and photon spheres with spherical accretions in the four-dimensional Gauss–Bonnet black hole

Abstract We investigate the shadows and photon spheres of the four-dimensional Gauss–Bonnet black hole with the static and infalling spherical accretions. We show that, for both cases, there always exist shadows and photon spheres. The radii of the shadows and photon spheres are independent of the p...

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Main Authors: Xiao-Xiong Zeng, Hai-Qing Zhang, Hongbao Zhang
Format: Article
Language:English
Published: SpringerOpen 2020-09-01
Series:European Physical Journal C: Particles and Fields
Online Access:http://link.springer.com/article/10.1140/epjc/s10052-020-08449-y
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spelling doaj-f01fbd485668485ea09c752ad2a4f0b72020-11-25T03:48:37ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522020-09-0180911110.1140/epjc/s10052-020-08449-yShadows and photon spheres with spherical accretions in the four-dimensional Gauss–Bonnet black holeXiao-Xiong Zeng0Hai-Qing Zhang1Hongbao Zhang2State Key Laboratory of Mountain Bridge and Tunnel Engineering, Chongqing Jiaotong UniversityDepartment of Space Science, Center for Gravitational Physics, Beihang UniversityDepartment of Physics, Beijing Normal UniversityAbstract We investigate the shadows and photon spheres of the four-dimensional Gauss–Bonnet black hole with the static and infalling spherical accretions. We show that, for both cases, there always exist shadows and photon spheres. The radii of the shadows and photon spheres are independent of the profiles of accretion for a fixed Gauss–Bonnet constant, implying that the shadow is a signature of the spacetime geometry and it is hardly influenced by accretion. Because of the Doppler effect, the shadows of the infalling accretion are found to be darker than in the static case. We also investigate the effect of the Gauss–Bonnet constant on the shadow and photon spheres, and we find that the larger the Gauss–Bonnet constant is, the smaller the radii of the shadow and photon spheres will be. In particular, the observed specific intensity increases as the Gauss–Bonnet constant grows.http://link.springer.com/article/10.1140/epjc/s10052-020-08449-y
collection DOAJ
language English
format Article
sources DOAJ
author Xiao-Xiong Zeng
Hai-Qing Zhang
Hongbao Zhang
spellingShingle Xiao-Xiong Zeng
Hai-Qing Zhang
Hongbao Zhang
Shadows and photon spheres with spherical accretions in the four-dimensional Gauss–Bonnet black hole
European Physical Journal C: Particles and Fields
author_facet Xiao-Xiong Zeng
Hai-Qing Zhang
Hongbao Zhang
author_sort Xiao-Xiong Zeng
title Shadows and photon spheres with spherical accretions in the four-dimensional Gauss–Bonnet black hole
title_short Shadows and photon spheres with spherical accretions in the four-dimensional Gauss–Bonnet black hole
title_full Shadows and photon spheres with spherical accretions in the four-dimensional Gauss–Bonnet black hole
title_fullStr Shadows and photon spheres with spherical accretions in the four-dimensional Gauss–Bonnet black hole
title_full_unstemmed Shadows and photon spheres with spherical accretions in the four-dimensional Gauss–Bonnet black hole
title_sort shadows and photon spheres with spherical accretions in the four-dimensional gauss–bonnet black hole
publisher SpringerOpen
series European Physical Journal C: Particles and Fields
issn 1434-6044
1434-6052
publishDate 2020-09-01
description Abstract We investigate the shadows and photon spheres of the four-dimensional Gauss–Bonnet black hole with the static and infalling spherical accretions. We show that, for both cases, there always exist shadows and photon spheres. The radii of the shadows and photon spheres are independent of the profiles of accretion for a fixed Gauss–Bonnet constant, implying that the shadow is a signature of the spacetime geometry and it is hardly influenced by accretion. Because of the Doppler effect, the shadows of the infalling accretion are found to be darker than in the static case. We also investigate the effect of the Gauss–Bonnet constant on the shadow and photon spheres, and we find that the larger the Gauss–Bonnet constant is, the smaller the radii of the shadow and photon spheres will be. In particular, the observed specific intensity increases as the Gauss–Bonnet constant grows.
url http://link.springer.com/article/10.1140/epjc/s10052-020-08449-y
work_keys_str_mv AT xiaoxiongzeng shadowsandphotonsphereswithsphericalaccretionsinthefourdimensionalgaussbonnetblackhole
AT haiqingzhang shadowsandphotonsphereswithsphericalaccretionsinthefourdimensionalgaussbonnetblackhole
AT hongbaozhang shadowsandphotonsphereswithsphericalaccretionsinthefourdimensionalgaussbonnetblackhole
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