Black holes in 4D AdS Einstein Gauss Bonnet gravity with power: Yang Mills field

Biswas, Anindya Kumar

doi:10.1007/s10714-022-03047-7

Cited by 6 publications

(4 citation statements)

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“…In the coupling of nonlinear YM field in terms of the power q of the YM invariant given as F (a) µν F µν(a) q with GB gravity, Mazharimousavi and Halilsoy [58] obtained a BH solution in D-dimensions. Recently, Biswas [59] derived a BH solution in EGB theory with a power-Yang-Mills (PYM) field in 4D AdS spacetime.…”

Section: Jcap10(2023)058mentioning

confidence: 99%

“…Motivated by this, it is noteworthy to consider YM invariant with a power q ̸ = 1. Therefore, a BH solution arising from 4D EGB gravity in the PYM field [59] may give interesting properties of the coupling of the theories.…”

Section: Jcap10(2023)058mentioning

confidence: 99%

“…Thus, the non-rotating BH solution for Λ = 0 in ref. [59] will be converted into its rotating counterpart and further shadows will be studied via the method of impact parameters. Moreover, the distortion and energy emission rate will also be studied using shadows' results.…”

Section: Jcap10(2023)058mentioning

confidence: 99%

“…We present a brief discussion of the four-dimensional EGB BH immersed in the PYM field. The action of GB gravity in D dimensions coupled with the PYM field reads [58,59]…”

Section: The Static Black Holementioning

confidence: 99%

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4D Einstein-Gauss-Bonnet black hole in Power-Yang-Mills field: a shadow study

Zubair,

Raza,

Sarikulov

et al. 2023

J. Cosmol. Astropart. Phys.

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We consider a static black hole immersed in the Power-Yang-Mills field in four-dimensional Einstein-Gauss-Bonnet gravity and investigate the effect of various parameters on the radius of the photon sphere. The modified form of the Newman-Janis algorithm is used for obtaining a rotating black hole solution in this gravity. Further, we try to explore the influence of the Yang-Mills magnetic charge Q with power q, Gauss-Bonnet parameter α, and spin a on the horizon radius. The geodesic equations are constructed by incorporating the Hamilton-Jacobi formalism. The radial component of the geodesic equations gives the effective potential which is further used in deriving the mathematical structure for the shadows by using Bardeen's procedure for a fixed observer at infinity. The shadows are calculated and plotted in terms of two celestial coordinates for an equatorial observer. It is observed that all the parameters have a very significant effect on the shadow and related physical observables. We also obtain the constraint values for the spin, magnetic charge, and Gauss-Bonnet parameters, using the shadow size of supermassive black holes Sagittarius A* and M87* from the EHT observations for the cases of q = 0.6 and q = 0.9. It is shown that there are upper and lower bounds for the charge and spin of M87* at q = 0.6, while only the upper bounds for the charge and spin of Sagittarius A*. Finally, we investigate the energy emission rate in the Hawking radiation around the 4D Einstein-Gauss-Bonnet black hole in the Power-Yang-Mills field.

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Section: Jcap10(2023)058mentioning

confidence: 99%

Section: Jcap10(2023)058mentioning

confidence: 99%

Section: Jcap10(2023)058mentioning

confidence: 99%

“…We present a brief discussion of the four-dimensional EGB BH immersed in the PYM field. The action of GB gravity in D dimensions coupled with the PYM field reads [58,59]…”

Section: The Static Black Holementioning

confidence: 99%

See 2 more Smart Citations