Hawking Temperature of the Reissner-Nordstrom-Vaidya Black Hole
Triyanta1,2 & Anike N Bowaire1 1Division of Theoretical High Energy Physics and Instrumentation, Faculty of Mathematics and Natural sciences, Institut Teknologi Bandung Jalan Ganesha No. 10 Bandung 40132 Indonesia 2Indonesian Center for Theoretical and Mathematical Physics, Faculty of Mathematics and Natural Sciences, Institut Teknologi Bandung Jalan Ganesha No. 10 Bandung 40132 Indonesia Email: triyanta@fi.itb.ac.id
Abstract. We have derived the Hawking temperature of the Reissner-Nordstrom-Vaidya black hole by the use of both the radial null geodesic and the complex path methods. We have obtained that the mass dependence of the temperature in the Reissner-Nordstrom-Vaidya black hole is not as simple as that in the Schwarzschild black hole, but still we regain the conclusion, as in the case of the Schwarzschild black hole, that a higher Hawking temperature corresponds to a lower mass of a black hole.
Keywords: black hole horizon; charged black hole; complex path; extreme Reissner-Nordstrom-Vaidya black hole; Hamilton-Jacobi equation; Hawking temperature; radial null geodesic; Reissner-Nordstrom-Vaidya black hole.
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