Cosmology of fermionic dark energy coupled to curvature

Abstract

A formulation of cosmology driven by fermions $\psi$ is studied. Assumption that the expectation value of the fermion bilinear is non-zero simplifies the homogeneous solution of the Dirac equations and connects the spinor field with the scale parameter of the universe. With coupling between the Einstein term and spinor field $1-\frac{\xi }{6}(\bar{\psi }\psi {)}^{-l}$, the possibility for a late time interaction emerges. In that way, the early universe agrees with $\Lambda$CDM model, but for the late universe the new integrating term dominates.

Accepted in Nuc. Phys. B

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Cited by in corpus (2)

• Alleviating both $H_0$ and ${\sigma }_8$ tensions in Tsallis cosmology
• Alleviating $H_0$ Tension with New Gravitational Scalar Tensor Theories