1 Ocak 2016 Dergi makalesi Açık Erişim

Sakalli, Izzet; Aslan, Onur Atilla

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  <identifier identifierType="URL">https://aperta.ulakbim.gov.tr/record/55543</identifier>
  <creators>
    <creator>
      <creatorName>Sakalli, Izzet</creatorName>
      <givenName>Izzet</givenName>
      <familyName>Sakalli</familyName>
      <affiliation>Eastern Mediterranean Univ, Dept Phys, North Cyprus 10, Mersin, Turkey</affiliation>
    </creator>
    <creator>
      <creatorName>Aslan, Onur Atilla</creatorName>
      <givenName>Onur Atilla</givenName>
      <familyName>Aslan</familyName>
      <affiliation>Eastern Mediterranean Univ, Dept Phys, North Cyprus 10, Mersin, Turkey</affiliation>
    </creator>
  </creators>
  <titles>
    <title>Hawking Radiation Of Non-Asymptotically Flat Rotating Black Holes</title>
  </titles>
  <publisher>Aperta</publisher>
  <publicationYear>2016</publicationYear>
  <dates>
    <date dateType="Issued">2016-01-01</date>
  </dates>
  <resourceType resourceTypeGeneral="Text">Journal article</resourceType>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://aperta.ulakbim.gov.tr/record/55543</alternateIdentifier>
  </alternateIdentifiers>
  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsIdenticalTo">10.1007/s10509-016-2714-3</relatedIdentifier>
  </relatedIdentifiers>
  <rightsList>
    <rights rightsURI="http://www.opendefinition.org/licenses/cc-by">Creative Commons Attribution</rights>
    <rights rightsURI="info:eu-repo/semantics/openAccess">Open Access</rights>
  </rightsList>
  <descriptions>
    <description descriptionType="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.</description>
  </descriptions>
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