1 Ocak 2021 Dergi makalesi Açık Erişim

Hassanabadi, H.; Chung, W. S.; Lutfuoglu, B. C.; Maghsoodi, E.

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  <identifier identifierType="URL">https://aperta.ulakbim.gov.tr/record/230882</identifier>
  <creators>
    <creator>
      <creatorName>Hassanabadi, H.</creatorName>
      <givenName>H.</givenName>
      <familyName>Hassanabadi</familyName>
    </creator>
    <creator>
      <creatorName>Chung, W. S.</creatorName>
      <givenName>W. S.</givenName>
      <familyName>Chung</familyName>
    </creator>
    <creator>
      <creatorName>Lutfuoglu, B. C.</creatorName>
      <givenName>B. C.</givenName>
      <familyName>Lutfuoglu</familyName>
    </creator>
    <creator>
      <creatorName>Maghsoodi, E.</creatorName>
      <givenName>E.</givenName>
      <familyName>Maghsoodi</familyName>
      <affiliation>Lorestan Univ, Fac Sci, Phys Dept, Khorramabad, Iran</affiliation>
    </creator>
  </creators>
  <titles>
    <title>Effects Of A New Extended Uncertainty Principle On Schwarzschild And Reissner-Nordstrom Black Holes Thermodynamics</title>
  </titles>
  <publisher>Aperta</publisher>
  <publicationYear>2021</publicationYear>
  <dates>
    <date dateType="Issued">2021-01-01</date>
  </dates>
  <resourceType resourceTypeGeneral="Text">Journal article</resourceType>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://aperta.ulakbim.gov.tr/record/230882</alternateIdentifier>
  </alternateIdentifiers>
  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsIdenticalTo">10.1142/S0217751X21500366</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">In this paper, we employ a new form of the extended uncertainty principle to investigate the thermal properties of the Schwarzschild and Reissner-Nordstrom. After we construct the formalism, we obtain the mass-temperature function for the Schwarzschild black hole. We follow a heuristic method to derive the entropy function after we obtained the heat capacity function. Then, we derive the mass-temperature and mass-charge-temperature functions of the Reissner-Nordstrom black hole in the new formalism. After we obtain the heat capacity and entropy functions, we present a comprehensive and comparative analysis of all these functions. We find that the deformation parameter changes drastically some of the thermodynamic function characteristics.</description>
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