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Higher dimensional power-Maxwell charged black holes in Einstein and Rastall gravity

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arxiv 1809.10075 v4 pith:LUJU743S submitted 2018-09-26 gr-qc

Kai Lin , Yunqi Liu , Wei-Liang Qian This is my paper · ORCID
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keywords blackholesolutionsrastalleinsteingravityobtainedpower-maxwell
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The black hole solutions in higher-dimensional spacetimes with the presence of the power-Maxwell field, surrounded by quintessence, are investigated for Einstein as well as Rastall gravity. The obtained solutions accommodate for spherical, planar and hyperbolic symmetries with the presence of the cosmological constant. Besides, we show that several known black hole solutions in literature such as those for linear Maxwell theory and BTZ black hole can be obtained as special cases. The implications of Rastall's theory related to the present study and the thermodynamics of the black hole solutions are discussed.

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Cited by 1 Pith paper

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  1. Exploring Hubble Tension Alleviation through Neutrino-Coupled Perturbed $f(R)$ Gravity

    gr-qc 2025-02 reject novelty 2.0 of 10

    A fit of Hu-Sawicki f(R) gravity with a fitted neutrino interaction to CMB, lensing, BAO, CC, and Pantheon data returns H0 near 70 km/s/Mpc, partially easing but not resolving the Hubble and S8 tensions.

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