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Space-time evolution induced by spinor fields with canonical and non-canonical kinetic terms

  • Regular Article - Theoretical Physics
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Abstract

We study spinor field theories as an origin to induce space-time evolution. Self-interacting spinor fields with canonical and non-canonical kinetic terms are considered in a Friedman–Robertson–Walker universe. The deceleration parameter is calculated by solving the equation of motion and the Friedman equation, simultaneously. It is shown that the spinor fields can accelerate and decelerate the universe expansion. To construct realistic models we discuss the contributions from the dynamical symmetry breaking.

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Authors and Affiliations

  1. Information Media Center, Hiroshima University, Higashi-Hiroshima, 739-8521, Japan

    Tomohiro Inagaki

  2. Graduate School of Integrated Arts and Sciences, Hiroshima University, Higashi-Hiroshima, 739-8521, Japan

    Tomohiro Inagaki & Yury Rybalov

  3. Department of Physics, Nankai University, Tianjin, 300071, P.R. China

    Xinhe Meng

Authors
  1. Tomohiro Inagaki
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  2. Yury Rybalov
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  3. Xinhe Meng
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Correspondence to Tomohiro Inagaki.

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Inagaki, T., Rybalov, Y. & Meng, X. Space-time evolution induced by spinor fields with canonical and non-canonical kinetic terms. Eur. Phys. J. C 71, 1656 (2011). https://doi.org/10.1140/epjc/s10052-011-1656-8

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  • DOI: https://doi.org/10.1140/epjc/s10052-011-1656-8

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