Spinor field dark energy in spherically symmetric FLRW spacetime is constrained with observational data, producing best-fit parameters consistent with current Hubble and deceleration values.
Physics of Particles and Nuclei 49(2), 146 (2018)
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Constraining parameters of spinor field dark energy: An alternative to $\Lambda$CDM model under the spherically symmetric FLRW space-time
Spinor field dark energy in spherically symmetric FLRW spacetime is constrained with observational data, producing best-fit parameters consistent with current Hubble and deceleration values.