Accelerated expansion of the Universe driven by G-essence

Abstract

In the present work we analyze the g-essence model for the particular Lagrangian: $L=R+2[\alpha X^n+\epsilon Y-V(\psi ,\bar{\psi })]$. The g-essence models were proposed recently as an alternative and as a generalization to the scalar k-essence. We have presented the 3 types solutions of the g-essence model. We reconstructed the corresponding potentials and the dynamics of the scalar and fermionic fields according the evolution of the scale factor. The obtained results shows that the g-essence model can describes the decelerated and accelerated expansion phases of the universe.

10 pages

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• Dark Energy Model with Spinor Matter and Its Quintom Scenario
• Cosmological model with non-minimally coupled fermionic field
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Cited by in corpus (1)

• G-essence with Yukawa Interactions