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Hawking radiation of non-asymptotically flat rotating black holes

Sakalli, Izzet; Aslan, Onur Atilla


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        "affiliation": "Eastern Mediterranean Univ, Dept Phys, North Cyprus 10, Mersin, Turkey", 
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        "affiliation": "Eastern Mediterranean Univ, Dept Phys, North Cyprus 10, Mersin, Turkey", 
        "name": "Aslan, Onur Atilla"
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    "description": "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.", 
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