{
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  "authors": [
    {
      "affiliations": [
        {
          "country": "Brazil", 
          "value": "Departamento de F\u00edsica, Universidade Federal do Cear\u00e1 (UFC), Campus do Pici, Fortaleza, CE, 60455-760, Brazil", 
          "organization": "Universidade Federal do Cear\u00e1 (UFC)"
        }
      ], 
      "surname": "Lessa", 
      "given_names": "L.", 
      "full_name": "Lessa, L."
    }, 
    {
      "affiliations": [
        {
          "country": "Brazil", 
          "value": "Universidade Federal do Cariri (UFCA), Av. Tenente Raimundo Rocha, Cidade Universit\u00e1ria, Juazeiro do Norte, Cear\u00e1, CEP 63048-080, Brasil", 
          "organization": "Universidade Federal do Cariri (UFCA)"
        }
      ], 
      "surname": "Silva", 
      "email": "euclides.silva@ufca.edu.br", 
      "full_name": "Silva, J.", 
      "given_names": "J."
    }, 
    {
      "affiliations": [
        {
          "country": "Brazil", 
          "value": "Departamento de F\u00edsica, Universidade Federal do Cear\u00e1 (UFC), Campus do Pici, Fortaleza, CE, 60455-760, Brazil", 
          "organization": "Universidade Federal do Cear\u00e1 (UFC)"
        }
      ], 
      "surname": "Maluf", 
      "given_names": "R.", 
      "full_name": "Maluf, R."
    }, 
    {
      "affiliations": [
        {
          "country": "Brazil", 
          "value": "Departamento de F\u00edsica, Universidade Federal do Cear\u00e1 (UFC), Campus do Pici, Fortaleza, CE, 60455-760, Brazil", 
          "organization": "Universidade Federal do Cear\u00e1 (UFC)"
        }
      ], 
      "surname": "Almeida", 
      "given_names": "C.", 
      "full_name": "Almeida, C."
    }
  ], 
  "titles": [
    {
      "source": "Springer", 
      "title": "Modified black hole solution with a background Kalb\u2013Ramond field"
    }
  ], 
  "dois": [
    {
      "value": "10.1140/epjc/s10052-020-7902-1"
    }
  ], 
  "publication_info": [
    {
      "page_end": "9", 
      "journal_title": "European Physical Journal C", 
      "material": "article", 
      "journal_volume": "80", 
      "artid": "s10052-020-7902-1", 
      "year": 2020, 
      "page_start": "1", 
      "journal_issue": "4"
    }
  ], 
  "$schema": "http://repo.scoap3.org/schemas/hep.json", 
  "acquisition_source": {
    "date": "2020-04-22T14:30:38.051803", 
    "source": "Springer", 
    "method": "Springer", 
    "submission_number": "fbcfdba8849411eaad8602163e01809a"
  }, 
  "page_nr": [
    9
  ], 
  "license": [
    {
      "url": "https://creativecommons.org/licenses//by/4.0", 
      "license": "CC-BY-4.0"
    }
  ], 
  "copyright": [
    {
      "holder": "The Author(s)", 
      "year": "2020"
    }
  ], 
  "control_number": "53972", 
  "record_creation_date": "2020-04-22T14:30:38.051847", 
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  "collections": [
    {
      "primary": "European Physical Journal C"
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  ], 
  "arxiv_eprints": [
    {
      "categories": [
        "gr-qc", 
        "hep-th"
      ], 
      "value": "arXiv:1911.10296v1"
    }
  ], 
  "abstracts": [
    {
      "source": "Springer", 
      "value": "We study the gravitation effects on a static and spherically symmetric spacetime due to the vacuum expectation value (VEV) of a Kalb\u2013Ramond field. The Kalb\u2013Ramond VEV is a background tensor field which produces a local Lorentz symmetry breaking (LSB) of spacetime. Considering a non-minimal coupling between the Kalb\u2013Ramond (VEV) and the Ricci tensor, we obtain an exact parameterdependent power-law modified black hole. For a particular choice of the LSB parameter, the Lorentz violation produces a solution similar to the Reissner\u2013Nordstrom, despite the absence of charge. The near-horizon geometry is modified by including a new inner horizon and shifting the Schwarzschild horizon. Asymptotically, the usual Minkowski spacetime with a background tensor field is recovered. The vacuum configurations are studied considering the energy conditions and the Lorentz violating source properties. By means of the mercury perihelion test, an upper bound to the local Lorentz violation (LV) is obtained, and its corresponding effects on the black hole temperature is investigated."
    }
  ], 
  "imprints": [
    {
      "date": "2020-04-22", 
      "publisher": "Springer"
    }
  ]
}