Cosmological Adiabatic Geometric Phase of a Scalar Field in a Bianchi Spacetime

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dc.creatorMostafazadeh, A.
dc.date2001-01-22
dc.date.accessioned2026-07-07T03:25:37Z
dc.date.available2026-07-07T03:25:37Z
dc.descriptionA two-component formulation of the Klein-Gordon equation is used to investigate the cyclic and noncyclic adiabatic geometric phases due to spatially homogeneous (Bianchi) cosmological models. It is shown that no adiabatic geometric phases arise for Bianchi type I models. For general Bianchi type IX models the problem of the adiabatic geometric phase is shown to be equivalent to the one for nuclear quadrupole interactions of a spin. For these models nontrivial non-Abelian adiabatic geometrical phases may occur in general.
dc.descriptionPresented in the IX Regional Conference on Mathematical Physics Ref: Turkish J. Phys. 24, 411-128 (2000)
dc.identifierhttps://arxiv.org/abs/gr-qc/0101087
dc.identifierhttp://arxiv.org/abs/gr-qc/0101087
dc.identifierTurk.J.Phys. 24 (2000) 411-428
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/33777
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleCosmological Adiabatic Geometric Phase of a Scalar Field in a Bianchi Spacetime
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