1 Ocak 2016 Dergi makalesi Açık Erişim

Sakalli, Izzet; Aslan, Onur Atilla

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  <dc:creator>Sakalli, Izzet</dc:creator>
  <dc:creator>Aslan, Onur Atilla</dc:creator>
  <dc:date>2016-01-01</dc:date>
  <dc: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.</dc:description>
  <dc:identifier>https://aperta.ulakbim.gov.trrecord/55543</dc:identifier>
  <dc:identifier>oai:zenodo.org:55543</dc:identifier>
  <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
  <dc:rights>http://www.opendefinition.org/licenses/cc-by</dc:rights>
  <dc:source>ASTROPHYSICS AND SPACE SCIENCE 361(4)</dc:source>
  <dc:title>Hawking radiation of non-asymptotically flat rotating black holes</dc:title>
  <dc:type>info:eu-repo/semantics/article</dc:type>
  <dc:type>publication-article</dc:type>
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