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Holographic Einstein rings of a Gauss-Bonnet AdS black hole

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arxiv 2302.03692 v2 pith:526M3CT3 submitted 2023-02-07 gr-qc hep-th

classification gr-qchep-th
keywords holographicblackimagesgauss-bonnetholeringabsolutealways
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abstract

Based on the AdS/CFT correspondence, we studied the holographic Einstein images of a Gauss-Bonnet AdS black hole in the bulk from a given response function on AdS boundary. For the absolute amplitude of total response function, it shows that there always exists the interference pattern as the scalar wave passed through the black hole. And, the absolute amplitude depends closely on the properties of Gaussian source and spacetime geometry. More importantly, we also find that the holographic images always appears as a ring with the concentric stripe surrounded when the observer located at the north pole. At other positions, this ring will change into a luminosity-deformed ring, or two light points. In addition, the effects of Gauss-Bonnet parameter $\alpha$, wave source and optical system on the holographic images have been carefully addressed throughout of paper. Finally, we conclude that the holographic images in different types of black holes with some different features may shed some deep insight on the existence of a gravity dual for a given material.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Image of the time-dependent black hole

    gr-qc 2025-07 conditional novelty 4.0 of 10

    For a Vaidya black hole with linearly growing mass, the accretion disk image's bright spot shifts radially outward with the conformal time coordinate, while the observed flux in the conformal frame remains time-independent.

  2. Testing Extended Theories of Gravity via Black Hole Photon Rings

    gr-qc 2025-05 conditional novelty 3.0 of 10

    For Konoplya-Zhidenko deformed Schwarzschild black holes, epsilon controls photon sphere, shadow, and photon ring size while a2 and b2 are observationally degenerate, and EHT data constrain epsilon to about -0.09 to 0...

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