D J Raine and D W Sciama 1997 Class. Quantum Grav. 14 A325 doi:10.1088/0264-9381/14/1A/024
D J Raine
and D W Sciama![]()
We present a simplified model of the collapse of a star to a black hole which can be treated as a dissipative open quantum system giving rise to Hawking radiation.
04.40.Dg Relativistic stars: structure, stability, and oscillations
04.70.Dy Quantum aspects of black holes, evaporation, thermodynamics
Issue 1A (January 1997)
D J Raine and D W Sciama 1997 Class. Quantum Grav. 14 A325
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