{
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  "authors": [
    {
      "surname": "Dil", 
      "given_names": "Emre", 
      "raw_name": "Dil, Emre", 
      "affiliations": [
        {
          "country": "Turkey", 
          "value": "Department of Physics, Sinop University, Korucuk, 57000 Sinop, Turkey"
        }
      ], 
      "full_name": "Dil, Emre", 
      "orcid": "0000-0002-9042-7694"
    }, 
    {
      "raw_name": "Kolay, Erdin\u00e7", 
      "affiliations": [
        {
          "country": "Turkey", 
          "value": "Department of Statistics, Sinop University, Korucuk, 57000 Sinop, Turkey"
        }
      ], 
      "surname": "Kolay", 
      "given_names": "Erdin\u00e7", 
      "full_name": "Kolay, Erdin\u00e7"
    }
  ], 
  "titles": [
    {
      "source": "Hindawi Publishing Corporation", 
      "title": "Solution of Deformed Einstein Equations and Quantum Black Holes"
    }
  ], 
  "dois": [
    {
      "value": "10.1155/2016/3973706"
    }
  ], 
  "publication_info": [
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      "page_start": "3973706", 
      "material": "article", 
      "journal_title": "Advances in High Energy Physics", 
      "year": 2016
    }
  ], 
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  "acquisition_source": {
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    "source": "Hindawi Publishing Corporation", 
    "method": "Hindawi Publishing Corporation", 
    "submission_number": "161e1b74731f11e99fff02163e01809a"
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  "page_nr": [
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  "license": [
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      "url": "http://creativecommons.org/licenses/by/3.0/", 
      "license": "CC-BY-3.0"
    }
  ], 
  "copyright": [
    {
      "statement": "Copyright \u00a9 2016 Emre Dil and Erdin\u00e7 Kolay.", 
      "year": "2016"
    }
  ], 
  "control_number": "16474", 
  "record_creation_date": "2016-07-18T00:00:00", 
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  "abstracts": [
    {
      "source": "Hindawi Publishing Corporation", 
      "value": "Recently, one- and two-parameter deformed Einstein equations have been studied for extremal quantum black holes which have been proposed to obey deformed statistics by Strominger. In this study, we give a deeper insight into the deformed Einstein equations and consider the solutions of these equations for the extremal quantum black holes. We then represent the implications of the solutions, such that the deformation parameters lead the charged black holes to have a smaller mass than the usual Reissner-Nordstr\u00f6m black holes. This reduction in mass of a usual black hole can be considered as a transition from classical to quantum black hole regime."
    }
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      "date": "2016-07-18", 
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