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Warm inflation in Horndeski gravity

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Abstract

In this paper, we investigate a class of Horndeski scalar-tensor theory of gravity for warm inflation. We present some models where the early-time acceleration is realized in the weak and in the strong dissipation regime. Cosmological perturbations are analyzed.

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Authors and Affiliations

  1. Department of General and Theoretical Physics and Eurasian Center for Theoretical Physics, Eurasian National University, Astana, Kazakhstan, 010008

    Lorenzo Sebastiani & Ratbay Myrzakulov

  2. Dipartimento di Fisica, Università di Trento, Trento, Italy

    Lorenzo Sebastiani

  3. Department of Theoretical and Nuclear Physics, Al-Farabi Kazakh National University, Al-Farabi, Almaty, Kazakhstan

    Shynaray Myrzakul

Authors
  1. Lorenzo Sebastiani
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  2. Shynaray Myrzakul
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  3. Ratbay Myrzakulov
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Correspondence to Lorenzo Sebastiani.

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Sebastiani, L., Myrzakul, S. & Myrzakulov, R. Warm inflation in Horndeski gravity. Gen Relativ Gravit 49, 90 (2017). https://doi.org/10.1007/s10714-017-2257-0

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  • DOI: https://doi.org/10.1007/s10714-017-2257-0

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