Probing a regular non-minimal Einstein-Yang-Mills black hole with gravitational lensings

We investigate weak and strong deflection gravitational lensings of the regular black hole predicted by a non-minimal Einstein–Yang–Mills theory. We find that its weak deflection lensing is the same as a Reissner–Nordström black hole's. Observables in the strong deflection lensing, including th...

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Main Authors: Feng-Yuan Liu, Yi-Fan Mai, Wen-Yu Wu, Yi Xie
Format: Article
Language:English
Published: Elsevier 2019-08-01
Series:Physics Letters B
Online Access:http://www.sciencedirect.com/science/article/pii/S0370269319304356
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spelling doaj-0b41d69999b149d18d262d66d23600222020-11-25T00:45:57ZengElsevierPhysics Letters B0370-26932019-08-01795475481Probing a regular non-minimal Einstein-Yang-Mills black hole with gravitational lensingsFeng-Yuan Liu0Yi-Fan Mai1Wen-Yu Wu2Yi Xie3School of Astronomy and Space Science, Nanjing University, Nanjing 210023, China; Key Laboratory of Modern Astronomy and Astrophysics, Nanjing University, Ministry of Education, Nanjing 210023, ChinaSchool of Astronomy and Space Science, Nanjing University, Nanjing 210023, China; Key Laboratory of Modern Astronomy and Astrophysics, Nanjing University, Ministry of Education, Nanjing 210023, ChinaSchool of Astronomy and Space Science, Nanjing University, Nanjing 210023, China; Key Laboratory of Modern Astronomy and Astrophysics, Nanjing University, Ministry of Education, Nanjing 210023, ChinaSchool of Astronomy and Space Science, Nanjing University, Nanjing 210023, China; Key Laboratory of Modern Astronomy and Astrophysics, Nanjing University, Ministry of Education, Nanjing 210023, China; Corresponding author at: School of Astronomy and Space Science, Nanjing University, Nanjing 210023, China.We investigate weak and strong deflection gravitational lensings of the regular black hole predicted by a non-minimal Einstein–Yang–Mills theory. We find that its weak deflection lensing is the same as a Reissner–Nordström black hole's. Observables in the strong deflection lensing, including the apparent radius of the photon sphere (shadow) as well as the angular separation, brightness difference and time delay between relativistic images, are obtained and analyzed for the supermassive black holes Sgr A* and M87* in the Galactic Center and at the center of M87. We find that only the apparent radii of the photon spheres are within the ability of current technology, whereas there is not enough resolution to distinguish the regular Einstein–Yang–Mills black hole from the Reissner–Nordström one. Meanwhile, caution needs to be paid when the diameter of M87*'s shadow measured by the Event Horizon Telescope is directly taken to constrain such a regular black hole. Keywords: Non-minimal Einstein–Yang–Mills theory, Regular black hole, Gravitational lensinghttp://www.sciencedirect.com/science/article/pii/S0370269319304356
collection DOAJ
language English
format Article
sources DOAJ
author Feng-Yuan Liu
Yi-Fan Mai
Wen-Yu Wu
Yi Xie
spellingShingle Feng-Yuan Liu
Yi-Fan Mai
Wen-Yu Wu
Yi Xie
Probing a regular non-minimal Einstein-Yang-Mills black hole with gravitational lensings
Physics Letters B
author_facet Feng-Yuan Liu
Yi-Fan Mai
Wen-Yu Wu
Yi Xie
author_sort Feng-Yuan Liu
title Probing a regular non-minimal Einstein-Yang-Mills black hole with gravitational lensings
title_short Probing a regular non-minimal Einstein-Yang-Mills black hole with gravitational lensings
title_full Probing a regular non-minimal Einstein-Yang-Mills black hole with gravitational lensings
title_fullStr Probing a regular non-minimal Einstein-Yang-Mills black hole with gravitational lensings
title_full_unstemmed Probing a regular non-minimal Einstein-Yang-Mills black hole with gravitational lensings
title_sort probing a regular non-minimal einstein-yang-mills black hole with gravitational lensings
publisher Elsevier
series Physics Letters B
issn 0370-2693
publishDate 2019-08-01
description We investigate weak and strong deflection gravitational lensings of the regular black hole predicted by a non-minimal Einstein–Yang–Mills theory. We find that its weak deflection lensing is the same as a Reissner–Nordström black hole's. Observables in the strong deflection lensing, including the apparent radius of the photon sphere (shadow) as well as the angular separation, brightness difference and time delay between relativistic images, are obtained and analyzed for the supermassive black holes Sgr A* and M87* in the Galactic Center and at the center of M87. We find that only the apparent radii of the photon spheres are within the ability of current technology, whereas there is not enough resolution to distinguish the regular Einstein–Yang–Mills black hole from the Reissner–Nordström one. Meanwhile, caution needs to be paid when the diameter of M87*'s shadow measured by the Event Horizon Telescope is directly taken to constrain such a regular black hole. Keywords: Non-minimal Einstein–Yang–Mills theory, Regular black hole, Gravitational lensing
url http://www.sciencedirect.com/science/article/pii/S0370269319304356
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AT yifanmai probingaregularnonminimaleinsteinyangmillsblackholewithgravitationallensings
AT wenyuwu probingaregularnonminimaleinsteinyangmillsblackholewithgravitationallensings
AT yixie probingaregularnonminimaleinsteinyangmillsblackholewithgravitationallensings
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