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.

A.A. Andrianov, F. Cannata, A.Y. Kamenshchik (2006). Phantom universe from CPT symmetric QFT. INTERNATIONAL JOURNAL OF MODERN PHYSICS D, 15, 1299-1310 [10.1142/S021827180600911X].

Phantom universe from CPT symmetric QFT.

KAMENCHTCHIK, ALEXANDR
2006

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.
2006
A.A. Andrianov, F. Cannata, A.Y. Kamenshchik (2006). Phantom universe from CPT symmetric QFT. INTERNATIONAL JOURNAL OF MODERN PHYSICS D, 15, 1299-1310 [10.1142/S021827180600911X].
A.A. Andrianov; F. Cannata; A.Y. Kamenshchik
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11585/34559
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