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  "authors": [
    {
      "affiliations": [
        {
          "country": "Mexico", 
          "value": "Facultad de Ingenier\u00eda, Centro Universitario Cerro de las Campanas, Universidad Aut\u00f3noma de Quer\u00e9taro, Santiago de Quer\u00e9taro, 76010, Mexico", 
          "organization": "Universidad Aut\u00f3noma de Quer\u00e9taro"
        }
      ], 
      "surname": "Hern\u00e1ndez-Almada", 
      "email": "ahalmada@uaq.mx", 
      "full_name": "Hern\u00e1ndez-Almada, A.", 
      "given_names": "A."
    }, 
    {
      "affiliations": [
        {
          "country": "Mexico", 
          "value": "Unidad Acad\u00e9mica de F\u00edsica, Universidad Aut\u00f3noma de Zacatecas, Calzada Solidaridad esquina con Paseo a la Bufa S/N C.P., Zacatecas, 98060, Mexico", 
          "organization": "Unidad Acad\u00e9mica de F\u00edsica, Universidad Aut\u00f3noma de Zacatecas"
        }, 
        {
          "country": "Mexico", 
          "value": "Consejo Nacional de Ciencia y Tecnolog\u00eda, Av. Insurgentes Sur 1582. Colonia Cr\u00e9dito Constructor, Del. Benito Ju\u00e1rez C.P., Mexico City, 03940, Mexico", 
          "organization": "Consejo Nacional de Ciencia y Tecnolog\u00eda"
        }
      ], 
      "surname": "Garc\u00eda-Aspeitia", 
      "given_names": "Miguel", 
      "full_name": "Garc\u00eda-Aspeitia, Miguel"
    }, 
    {
      "affiliations": [
        {
          "country": "Mexico", 
          "value": "Departamento de F\u00edsica, Instituto Nacional de Investigaciones Nucleares, Apartado Postal 18-1027, Mexico City, 11801, Mexico", 
          "organization": "Departamento de F\u00edsica, Instituto Nacional de Investigaciones Nucleares"
        }
      ], 
      "surname": "Rodr\u00edguez-Meza", 
      "given_names": "M.", 
      "full_name": "Rodr\u00edguez-Meza, M."
    }, 
    {
      "affiliations": [
        {
          "country": "Chile", 
          "value": "Facultad de Ciencias, Instituto de F\u00edsica y Astronom\u00eda, Universidad de Valpara\u00edso, Avda. Gran Breta\u00f1a, Valparaiso, 1111, Chile", 
          "organization": "Universidad de Valpara\u00edso"
        }
      ], 
      "surname": "Motta", 
      "given_names": "V.", 
      "full_name": "Motta, V."
    }
  ], 
  "titles": [
    {
      "source": "Springer", 
      "title": "A hybrid model of viscous and Chaplygin gas to tackle the Universe acceleration"
    }
  ], 
  "dois": [
    {
      "value": "10.1140/epjc/s10052-021-09104-w"
    }
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  "publication_info": [
    {
      "page_end": "9", 
      "journal_title": "European Physical Journal C", 
      "material": "article", 
      "journal_volume": "81", 
      "artid": "s10052-021-09104-w", 
      "year": 2021, 
      "page_start": "1", 
      "journal_issue": "4"
    }
  ], 
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    "source": "Springer", 
    "method": "Springer", 
    "submission_number": "d5456ec4a14911ed93fbd61508239648"
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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": "2021"
    }
  ], 
  "control_number": "61241", 
  "record_creation_date": "2021-04-08T20:30:20.816502", 
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  "collections": [
    {
      "primary": "European Physical Journal C"
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  ], 
  "abstracts": [
    {
      "source": "Springer", 
      "value": "Motivated by two seminal models proposed to explain the Universe acceleration, this paper is devoted to study a hybrid model which is constructed through a generalized Chaplygin gas with the addition of a bulk viscosity. We call the model a viscous generalized Chaplygin gas (VGCG) and its free parameters are constrained through several cosmological data like the Observational Hubble Parameter, Type Ia Supernovae, Baryon Acoustic Oscillations, Strong Lensing Systems, HII Galaxies and using Joint Bayesian analysis. In addition, we implement a Om-diagnostic to analyze the VGCC dynamics and its difference with the standard cosmological model. The hybrid model shows important differences when compared with the standard cosmological model. Finally, based on our Joint analysis we find that the VGCG could be an interesting candidate to alleviate the well-known Hubble constant tension."
    }
  ], 
  "imprints": [
    {
      "date": "2021-04-08", 
      "publisher": "Springer"
    }
  ]
}