1 Ocak 2016 Dergi makalesi Açık Erişim

Sakalli, Izzet; Aslan, Onur Atilla

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{
  "@context": "https://schema.org/", 
  "@id": 55543, 
  "@type": "ScholarlyArticle", 
  "creator": [
    {
      "@type": "Person", 
      "affiliation": "Eastern Mediterranean Univ, Dept Phys, North Cyprus 10, Mersin, Turkey", 
      "name": "Sakalli, Izzet"
    }, 
    {
      "@type": "Person", 
      "affiliation": "Eastern Mediterranean Univ, Dept Phys, North Cyprus 10, Mersin, Turkey", 
      "name": "Aslan, Onur Atilla"
    }
  ], 
  "datePublished": "2016-01-01", 
  "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.", 
  "headline": "Hawking radiation of non-asymptotically flat rotating black holes", 
  "identifier": 55543, 
  "image": "https://aperta.ulakbim.gov.tr/static/img/logo/aperta_logo_with_icon.svg", 
  "license": "http://www.opendefinition.org/licenses/cc-by", 
  "name": "Hawking radiation of non-asymptotically flat rotating black holes", 
  "url": "https://aperta.ulakbim.gov.tr/record/55543"
}