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| Main Authors: | , , , , |
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| Format: | Preprint |
| Published: |
2024
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| Subjects: | |
| Online Access: | https://arxiv.org/abs/2403.12840 |
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| _version_ | 1866909142478749696 |
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| author | You, Lei Wang, Rui-bo Ma, Shi-Jie Deng, Jian-Bo Hu, Xian-Ru |
| author_facet | You, Lei Wang, Rui-bo Ma, Shi-Jie Deng, Jian-Bo Hu, Xian-Ru |
| contents | The optical properties of Euler-Heisenberg (EH) black hole (BH) surrounded by Cold Dark Matter (CDM) halo are investigated. By changing BH's parameters, we found that the radius of horizon r_{h} and radius of photon sphere r_{ph} will transparently increase as CDM halo parameters R and ρincrease. To show the influence of CDM halo on the BH's optical characteristics, we took two sets of R and ρwith prominent differences and plot the first four orders of images for thin accretion disk with different angle of inclination θof observer. The images with light intensity distributions using Novikov-Thorne (N-T) model are also derived, as well as the effective potential, photon orbits. Especially, analysis of intersection behaviors between photon trajectories with different impact parameters and circular time-like orbits in accretion disk will help better understand the image of thin accretion disk. Our results showed that CDM halo will make BH become more larger and dimmer distinctly. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2403_12840 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Optical properties of Euler-Heisenberg black hole in the Cold Dark Matter Halo You, Lei Wang, Rui-bo Ma, Shi-Jie Deng, Jian-Bo Hu, Xian-Ru General Relativity and Quantum Cosmology The optical properties of Euler-Heisenberg (EH) black hole (BH) surrounded by Cold Dark Matter (CDM) halo are investigated. By changing BH's parameters, we found that the radius of horizon r_{h} and radius of photon sphere r_{ph} will transparently increase as CDM halo parameters R and ρincrease. To show the influence of CDM halo on the BH's optical characteristics, we took two sets of R and ρwith prominent differences and plot the first four orders of images for thin accretion disk with different angle of inclination θof observer. The images with light intensity distributions using Novikov-Thorne (N-T) model are also derived, as well as the effective potential, photon orbits. Especially, analysis of intersection behaviors between photon trajectories with different impact parameters and circular time-like orbits in accretion disk will help better understand the image of thin accretion disk. Our results showed that CDM halo will make BH become more larger and dimmer distinctly. |
| title | Optical properties of Euler-Heisenberg black hole in the Cold Dark Matter Halo |
| topic | General Relativity and Quantum Cosmology |
| url | https://arxiv.org/abs/2403.12840 |