Quantum effects for the stationary axisymmetric Sen black hole.

Computer Science

Scientific paper

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Black Holes: Thermodynamics, Black Holes: Hawking Radiation

Scientific paper

The solution of the Klein-Gordon equation near the event-horizon of the stationary axisymmetric Sen black hole is obtained by means of the Tortoise coordinates, the Hawking radiation formula is reduced. The authors results are compared with those of the ordinary Einstein black hole. They find that the dilaton field drastically affects the thermodynamic properties of the black hole.

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