{
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  "authors": [
    {
      "affiliations": [
        {
          "country": "Mexico", 
          "value": "Facultad de F\u00edsica, Universidad Veracruzana, Xalapa, Veracruz, 91000, M\u00e9xico", 
          "organization": "Universidad Veracruzana"
        }
      ], 
      "surname": "Cruz", 
      "email": "miguelcruz02@uv.mx", 
      "full_name": "Cruz, Miguel", 
      "given_names": "Miguel"
    }, 
    {
      "affiliations": [
        {
          "country": "Chile", 
          "value": "Departamento de F\u00edsica, Universidad de Concepci\u00f3n, Casilla 160, Concepci\u00f3n, 4070105, Chile", 
          "organization": "Universidad de Concepci\u00f3n"
        }
      ], 
      "surname": "Izaurieta", 
      "email": "fizaurie@udec.cl", 
      "full_name": "Izaurieta, Fernando", 
      "given_names": "Fernando"
    }, 
    {
      "affiliations": [
        {
          "country": "Chile", 
          "value": "Instituto de F\u00edsica, Facultad de Ciencias, Pontificia Universidad Cat\u00f3lica de Valpara\u00edso, Av. Brasil 2950, Valpara\u00edso, Chile", 
          "organization": "Pontificia Universidad Cat\u00f3lica de Valpara\u00edso"
        }
      ], 
      "surname": "Lepe", 
      "email": "samuel.lepe@pucv.cl", 
      "full_name": "Lepe, Samuel", 
      "given_names": "Samuel"
    }
  ], 
  "titles": [
    {
      "source": "Springer", 
      "title": "Non-zero torsion and late cosmology"
    }
  ], 
  "dois": [
    {
      "value": "10.1140/epjc/s10052-020-8128-y"
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  "publication_info": [
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      "page_end": "9", 
      "journal_title": "European Physical Journal C", 
      "material": "article", 
      "journal_volume": "80", 
      "artid": "s10052-020-8128-y", 
      "year": 2020, 
      "page_start": "1", 
      "journal_issue": "6"
    }
  ], 
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    "source": "Springer", 
    "method": "Springer", 
    "submission_number": "49a9ee70ddc511eab30802163e01809a"
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  "page_nr": [
    9
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  "license": [
    {
      "url": "https://creativecommons.org/licenses//by/4.0", 
      "license": "CC-BY-4.0"
    }
  ], 
  "copyright": [
    {
      "holder": "The Author(s)", 
      "year": "2020"
    }
  ], 
  "control_number": "55242", 
  "record_creation_date": "2020-07-09T13:58:33.602821", 
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  "collections": [
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      "primary": "European Physical Journal C"
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  "abstracts": [
    {
      "source": "Springer", 
      "value": "In this work, we study some thermodynamical aspects associated with torsion in a flat FLRW spacetime cosmic evolution. By implementing two Ansatze for the torsion term, we find that the model admits a phantom regime or a quintessence behavior. This scheme differs from the $$\\Lambda $$ <math><mi>\u039b</mi></math> CDM model at the thermodynamical level. The resulting cosmic expansion is not adiabatic, the fulfillment of the second law of thermodynamics requires a positive torsion term, and the temperature of the cosmic fluid is always positive. The entropy of the torsion phantom scenario is negative, but introducing chemical potential solves this issue. For a Dirac-Milne type Universe, the torsion leads to a growing behavior for the temperature of the fluid but has no incidence on the rate of expansion."
    }
  ], 
  "imprints": [
    {
      "date": "2020-06-19", 
      "publisher": "Springer"
    }
  ]
}