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      "raw_name": "Herrera, Ram\u00f3n", 
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        {
          "country": "Chile", 
          "value": "Instituto de F\u00edsica, Pontificia Universidad Cat\u00f3lica de Valpara\u00edso, Avenida Brasil 2950, Casilla 4059, Valpara\u00edso, Chile"
        }
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      "surname": "Herrera", 
      "given_names": "Ram\u00f3n", 
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    {
      "raw_name": "Videla, Nelson", 
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          "country": "Chile", 
          "value": "Departamento de F\u00edsica, FCFM, Universidad de Chile, Blanco Encalada 2008, Santiago, Chile"
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      ], 
      "surname": "Videla", 
      "given_names": "Nelson", 
      "full_name": "Videla, Nelson"
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    {
      "raw_name": "Olivares, Marco", 
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        {
          "country": "Chile", 
          "value": "Facultad de Ingenier\u00eda, Universidad Diego Portales, Avenida Ej\u00e9rcito Libertador 441, Casilla 298-V, Santiago, Chile"
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      "surname": "Olivares", 
      "given_names": "Marco", 
      "full_name": "Olivares, Marco"
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  "record_creation_date": "2016-01-22T00:00:00", 
  "titles": [
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      "source": "Springer/Societ\u00e0 Italiana di Fisica", 
      "title": "Warm intermediate inflationary Universe model in the presence of a generalized Chaplygin gas"
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      "year": 2016
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  "abstracts": [
    {
      "source": "Springer/SIF", 
      "value": "A warm intermediate inflationary model in the context of generalized Chaplygin gas is investigated. We study this model in the weak and strong dissipative regimes, considering a generalized form of the dissipative coefficient \u0393=\u0393(T,\u03d5) , and we describe the inflationary dynamics in the slow-roll approximation. We find constraints on the parameters in our model considering the Planck 2015 data, together with the condition for warm inflation T>H , and the conditions for the weak and strong dissipative regimes."
    }
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