Study of Hawking effect in Vaidya-Bonner black hole by means of second quantization.

Physics

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Black Holes: Hawking Radiation

Scientific paper

The Hawking thermal spectrum of a spherically charged evaporating black hole can be obtained by means of the second quantization and Bogolubov transformation on the Klein-Gordon scalar field near the event horizon of Vaidya-Bonner space-time. It is shown that the ingoing vacuum state becomes an outgoing state involving thermal particles after scattering on the surface of the horizon. These particles show a Planck spectrum whose temperature is T.

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