1 Ocak 2016 Dergi makalesi Açık Erişim

Sakalli, Izzet; Aslan, Onur Atilla

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    <subfield code="a">Hawking radiation of non-asymptotically flat rotating black holes</subfield>
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    <subfield code="a">We study the Hawking radiation of non-asymptotically flat rotating linear dilaton black holes, which are the solutions to the 4D Einstein-Maxwell-dilaton-axion action by using the semi-classical radiation spectrum method. Using scalar perturbations, we show that both angular and radial equations produce exact analytical solutions. Thus, we obtain a precise radiation spectrum for the rotating linear dilaton black hole. The high-frequency regime does not yield the standard Hawking temperature of this black hole computed from the surface gravity. However, we show in detail that the specific low-frequency band of the radiation spectrum allows for the original Hawking temperature of the rotating linear dilaton black hole. The computations are also exhibited graphically.</subfield>
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