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Black Holes in Bulk Viscous Cosmology

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Abstract

We investigate the effects of the accretion of phantom energy with non-zero bulk viscosity onto a Schwarzschild black hole and show that black holes accreting viscous phantom energy will lose mass rapidly compared to the non-viscous case. When matter is incorporated along with the phantom energy, the black holes meet with the same fate as bulk viscous forces dominate matter accretion. If the phantom energy has large bulk viscosity, then the mass of the black hole will reduce faster than in the small viscosity case.

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Authors and Affiliations

  1. Department of Physics, University of Lecce, Via Arnesano, Lecce, 73100, Italy

    Francesco De Paolis

  2. Center for Advanced Mathematics and Physics, National University of Sciences and Technology, Rawalpindi, 46000, Pakistan

    Mubasher Jamil & Asghar Qadir

Authors
  1. Francesco De Paolis
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  2. Mubasher Jamil
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  3. Asghar Qadir
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Corresponding author

Correspondence to Mubasher Jamil.

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De Paolis, F., Jamil, M. & Qadir, A. Black Holes in Bulk Viscous Cosmology. Int J Theor Phys 49, 621–632 (2010). https://doi.org/10.1007/s10773-009-0242-4

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  • DOI: https://doi.org/10.1007/s10773-009-0242-4

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