Coordinates with non-singular curvature for a time dependent black hole horizon

Foundations of Physics

Volumn 37, Issue 8, 2007, Pages 1181-1196

  Lindesay, James ^a  

^a HOWARD UNIVERSITY   (United States)

Author keywords

Black holes; Complementarity and horizon evolution; Non orthogonal coordinates; River model; Singularities

Indexed keywords

EID: 34548666002     PISSN: 00159018     EISSN: None     Source Type: Journal    
DOI: 10.1007/s10701-007-9146-4     Document Type: Article

References (8)

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3. J. M. Bardeen, "Black holes do evaporate thermally," PRL 46, 382-385 (1981).
4. Informal discussions with Samuel L. Braunstein, concerning unpublished manuscript "Energy-momentum tensor near the Schwarzschild event horizon," March-April 2006.
5. L. Susskind and J. Lindesay, An Introduction to Black Holes, Information, and the String Theory Revolution: The Holographic Universe (World Scientific, Singapore, 2005).
6. W.G. Unruh, "Notes on black-hole evaporation," Phys. Rev. D 14, 870-892 (1976).
7. A.J.S. Hamilton and J.P. Lisle, "The river model of black holes," gr-qc/0411060 (2004) 14 pages.
8. J. Lindesay, "An Introduction of multiple scales in a dynamical cosmology," gr-qc/0605007 (2006) 8 pages.