Nonzero $Ω_Λ$ and a new type of the dissipative structure

dc.creatorFujii, Yasunori
dc.date1998-06-23
dc.date.accessioned2026-07-07T03:32:29Z
dc.date.available2026-07-07T03:32:29Z
dc.descriptionWe revisit the proposed theoretical model for a small but nonzero cosmological constant which seems supported increasingly better by recent observations. The model features two scalar fields which interact with each other through a specifically chosen nonlinear potential. We find a very sensitive dependence of the solutions of the scalar field equations on the initial values. We discuss how the behavior is similar to and different from those in well-known chaotic systems, coming to suggest an interesting new type of the dissipative structure.
dc.descriptionLaTex, 6 pages, 2 figures
dc.identifierhttps://arxiv.org/abs/gr-qc/9806089
dc.identifierhttp://arxiv.org/abs/gr-qc/9806089
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/36249
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.titleNonzero $Ω_Λ$ and a new type of the dissipative structure
dc.typetext

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