Holographic image features of an AdS black hole in Einstein-power-Yang-Mills gravity

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Hauptverfasser: Hu, Xin-Yun, He, Ke-Jian, Zeng, Xiao-Xiong
Format: Preprint
Veröffentlicht: 2024
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author Hu, Xin-Yun
He, Ke-Jian
Zeng, Xiao-Xiong
author_facet Hu, Xin-Yun
He, Ke-Jian
Zeng, Xiao-Xiong
contents By utilizing the AdS/CFT correspondence, we investigate the holographic image of an AdS black hole in Einstein-power-Yang-Mills gravity. The AdS boundary hosts a Gaussian oscillation source, which induces a lensed response on the opposite side of the boundary during propagation through bulk spacetime. The optical system assists observers at the north pole to continuously capture holographic images that show an axisymmetric bright ring known as the Einstein ring. As the observation position shifted, the bright ring gradually transformed into a luminous arc and eventually transitioned into a light point. Simultaneously, we examine the impact of variations in relevant physical quantity on the ring, and present the corresponding brightness curve. The results indicate that as the temperature $T$ and nonlinear Yang Mills charge parameter $q$ increase, the ring radius also increases, while an increase in the chemical potential $u$ leads to a decrease. However, the peak brightness curve of the ring invariably decreases as the values of $T$, $u$, and $q$ increase, albeit to varying degrees. Upon comparing the outcomes of geometric optics, it can be observed that the position of the ring in holography images is consistent with that of the photon ring.
format Preprint
id arxiv_https___arxiv_org_abs_2406_03083
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Holographic image features of an AdS black hole in Einstein-power-Yang-Mills gravity
Hu, Xin-Yun
He, Ke-Jian
Zeng, Xiao-Xiong
High Energy Physics - Theory
General Relativity and Quantum Cosmology
By utilizing the AdS/CFT correspondence, we investigate the holographic image of an AdS black hole in Einstein-power-Yang-Mills gravity. The AdS boundary hosts a Gaussian oscillation source, which induces a lensed response on the opposite side of the boundary during propagation through bulk spacetime. The optical system assists observers at the north pole to continuously capture holographic images that show an axisymmetric bright ring known as the Einstein ring. As the observation position shifted, the bright ring gradually transformed into a luminous arc and eventually transitioned into a light point. Simultaneously, we examine the impact of variations in relevant physical quantity on the ring, and present the corresponding brightness curve. The results indicate that as the temperature $T$ and nonlinear Yang Mills charge parameter $q$ increase, the ring radius also increases, while an increase in the chemical potential $u$ leads to a decrease. However, the peak brightness curve of the ring invariably decreases as the values of $T$, $u$, and $q$ increase, albeit to varying degrees. Upon comparing the outcomes of geometric optics, it can be observed that the position of the ring in holography images is consistent with that of the photon ring.
title Holographic image features of an AdS black hole in Einstein-power-Yang-Mills gravity
topic High Energy Physics - Theory
General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2406.03083