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This paper argues that the effect of Hawking radiation on an astrophysical black hole situated in a realistic cosmological context is not total evaporation of the black hole; rather there will always be a remnant mass.
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G T Horowitz and J Maldacena (2004) “The black hole final state”. JHEP
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E Poisson (2004). A Relativist’s Toolkit: The Mathematics of Black-Hole Mechanics
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B J Carr (2005) “Primordial Black Holes: Do They Exist and Are They Useful?” In Proceedings of ”Inflating Horizon of Particle Astrophysics and Cosmology”, Universal Academy Press Inc and Yamada Science arXiv:astro-ph/0511743
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S W Hawking (2005) “Information loss in black holes”: arXiv:hep-th/0507171
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A B Nielsen and M Visser (2006) “Production and decay of evolving horizons” Class.Quant.Grav . 23
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A Peltola (2009) “Local Approach to Hawking Radiation” Class.Quant.Grav . 26
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P Peter and J-P Uzan (2009) Primordial Cosmology (Oxford: Oxford University Press)
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J Larena and T Rothman (2010) “Quasi-evaporating black holes and cold dark matter” Astrophys Space Sci 327
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J Lindesay and P Sheldon (2010) “Penrose Diagram for a Transient Black Hole”: arXiv:1005.4449
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S B Giddings (2013) “Black holes. quantum information, and the foundations of phyiscs” Phyiscs Today April 2013: 30-35
2013
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D S Lemon (2013) A Student’s guide to Entropy (Cambridge: Cambridge University Press)
2013
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