Phantom universe from CPT symmetric QFT
Alexander A. Andrianov, Francesco Cannata, Alexander Y. Kamenshchik

TL;DR
This paper develops a classical cosmological scalar field model based on CPT-symmetric non-Hermitian quantum theory, enabling a smooth transition from dark energy to phantom energy.
Contribution
It introduces a novel scalar field model derived from CPT-symmetric non-Hermitian quantum theory for cosmological applications.
Findings
Successfully models a smooth transition from dark energy to phantom energy.
Provides a new theoretical framework linking CPT symmetry with cosmological scalar fields.
Demonstrates potential for CPT-symmetric quantum theories to inform cosmological models.
Abstract
Inspired by the generalization of quantum theory for the case of non-Hermitian Hamiltonians with CPT symmetry, we construct a simple classical cosmological scalar field based model describing a smooth transition from ordinary dark energy to the phantom one.
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