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...
Main Authors: | , , |
---|---|
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 |
id |
doaj-f01fbd485668485ea09c752ad2a4f0b7 |
---|---|
record_format |
Article |
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 |
_version_ |
1724497984506298368 |