1 Ocak 2016 Dergi makalesi Açık Erişim

Sakalli, Izzet; Aslan, Onur Atilla

Citation Style Language JSON

{
  "DOI": "10.1007/s10509-016-2714-3", 
  "abstract": "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.", 
  "author": [
    {
      "family": "Sakalli", 
      "given": " Izzet"
    }, 
    {
      "family": "Aslan", 
      "given": " Onur Atilla"
    }
  ], 
  "container_title": "ASTROPHYSICS AND SPACE SCIENCE", 
  "id": "55543", 
  "issue": "4", 
  "issued": {
    "date-parts": [
      [
        2016, 
        1, 
        1
      ]
    ]
  }, 
  "title": "Hawking radiation of non-asymptotically flat rotating black holes", 
  "type": "article-journal", 
  "volume": "361"
}