Rotating ideal magnetohydrodynamic flow in General relativity

In this study we obtain the solution of the spherically symmetric de Sitter solution of black holes using a general form of distribution functions which include Gaussian, Rayleigh, and Maxwell-Boltzmann distribution as a special case. We investigate the properties of thermodynamics variables such as the Hawking temperature, the entropy, the mass and the heat capacity of black holes. Moreover, we show that the strong energy condition which includes the null energy condition is satisfied. Finally, we show the regularity of the solution by calculating the scalar curvature and invariant curvature in general distribution form.

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Spherically symmetric de Sitter solution of black holes

Mourad

Hussein

Eisa

et al. 2020

Indian J Phys

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Rotating charged fluids: Theorems and results for Weyl-type systems

Basso,

Zanchin

2023

Phys. Rev. D

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Rotating ideal magnetohydrodynamic flow in General relativity

Cited by 2 publications

References 11 publications

Spherically symmetric de Sitter solution of black holes

Spherically symmetric de Sitter solution of black holes

Rotating charged fluids: Theorems and results for Weyl-type systems

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