Phantom Accretion by Five Dimensional Charged Black Hole

Abstract

This paper deals with the dynamical behavior of phantom field near five dimensional charged black hole. We formulate equations of motion for steady-state spherically symmetric flow of phantom fluids. It is found that phantom energy accretes onto black holes for $u<0$. Further, the location of critical point of accretion are evaluated that leads to mass to charge ratio for 5D charged black hole. This ratio implies that accretion cannot transform a black hole into a naked singularity. We would like to mention here that this work is an irreducible extension of 4D charged black hole.

8 pages, accepted for publication in Mod. Phys. Lett. A

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• Evaporation of Black Hole Under the Effect of Quantum Gravity
• Thermodynamics of Phantom Energy Accreting onto a Black Hole in Einstein-Power-Maxwell Gravity
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• Spherical Accretion Flow onto General Parameterized Spherically Symmetric Black Hole Spacetimes
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• Accretion on High Derivative Asymptotically Safe Black Holes
• Constraints from accretion onto a Tangherlini-Reissner-Nordstrom black hole
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• Accretion onto a Charged Black Hole in Consistent 4D Einstein-Gauss-Bonnet Gravity
• Accretion Process as a Probe of Extra Dimensions in MOG Compact Object Spacetimes
• Binary X-ray sources in massive Brans-Dicke gravity
• Black holes in asymptotic safety with higher derivatives: accretion and stability analysis
• Spherical accretion onto higher-dimensional Reissner-Nordström Black Hole