A two-scalar pseudo-Hermitian model has a late-time attractor with constant Hubble rate and zero classical vacuum energy.
[7], where it was used to inves- tigate the variational principle and how Noether’s theo- rem is borne out in non-Hermitian deformations of oth- erwise Hermitian field theories
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Accelerated cosmological expansion from pseudo-Hermiticity
A two-scalar pseudo-Hermitian model has a late-time attractor with constant Hubble rate and zero classical vacuum energy.