{
  "id": "1701.01027",
  "version": "v1",
  "published": "2016-12-26T14:21:22.000Z",
  "updated": "2016-12-26T14:21:22.000Z",
  "title": "The Starobinsky model within the $f(R,T)$ formalism as a cosmological model",
  "authors": [
    "P. H. R. S. Moraes",
    "R. A. C. Correa",
    "G. Ribeiro"
  ],
  "categories": [
    "gr-qc",
    "hep-th"
  ],
  "abstract": "In this paper we derive a cosmological model from the $f(R,T)$ theory of gravity, for which $R$ is the Ricci scalar and $T$ is the trace of the energy-momentum tensor. We consider $f(R,T)=f(R)+f(T)$, with $f(R)$ being the Starobinksy model $R+\\alpha R^{2}$ and $f(T)=\\gamma T$, with $\\alpha$ and $\\gamma$ constants. We find that from such a functional form, it is possible to describe the cosmological scenario of a radiation-dominated universe, which has shown to be a non-trivial feature within the $f(R,T)$ formalism.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2016-12-26T14:21:22.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "cosmological model",
      "starobinsky model",
      "non-trivial feature",
      "functional form",
      "starobinksy model"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}