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In this work, we theoretically assume that a compact object (CO) can have a dark surface so that the CO is simplified to have no emissions and reflections.
1904
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S. Vagnozzi and L. Visinelli, “Hunting for extra dimensions in the shadow of M87*,” Phys. Rev. D
1905
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1906
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1906
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1912
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S. L. Shapiro, S. A. Teukolsky, and B. Holes, “Black holes, white dwarfs, and neutron stars: The physics of compact objects,” Physics Today
1983
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B. Mashhoon, F. Hehl, and D. Theiss, “On the influence of the proper rotation of central bodies on the motions of planets and moons according to einstein’s theory of gravitation,” General Relativity and Gravitation
1984
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2001
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2004
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2004
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B. Kleihaus, J. Kunz, and M. List, “Rotating boson stars and Q-balls,” Phys. Rev. D
2005
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2005
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2006
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2007
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2008
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2009
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M. Zhang and J. Jiang, “Shadows of accelerating black holes,” Phys. Rev. D
2010
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2011
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2011
Cited alongside, same era.
Z. Hu, Z. Zhong, P.-C. Li, M. Guo, and B. Chen, “QED effect on a black hole shadow,” Phys. Rev. D
2012
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S.-W. Wei and Y.-X. Liu, “Observing the shadow of Einstein-Maxwell-Dilaton-Axion black hole,” JCAP
2013
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2014
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2021
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2021
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Event Horizon Telescope
2022
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2022
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Event Horizon Telescope
2022
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2015
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2016
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2016
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2016
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2017
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2018
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2018
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2018
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2022
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Event Horizon Telescope
2022
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Event Horizon Telescope
2022
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2022
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2022
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2022
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2022
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2022
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2022
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2022
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2022
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2022
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2022
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X.-R. Zhu, Y.-X. Chen, P.-H. Mou, and K.-J. He, “The shadow and observation appearance of black hole surrounded by the dust field in Rastall theory,” Chin. Phys. B
2023
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