Two-Field Quintom Models in the w-w' Plane

dc.creatorGuo, Zong-Kuan
dc.creatorPiao, Yun-Song
dc.creatorZhang, Xinmin
dc.creatorZhang, Yuan-Zhong
dc.date2006-08-08
dc.date2006-12-06
dc.date.accessioned2026-07-07T10:39:45Z
dc.date.available2026-07-07T10:39:45Z
dc.descriptionThe w-w' plane, defined by the equation of state parameter for the dark energy and its derivative with respect to the logarithm of the scale factor, is useful to the study of classifying the dynamical dark energy models. In this note, we examine the evolving behavior of the two-field quintom models with w crossing the w=-1 barrier in the w-w' plane. We find that these models can be divided into two categories, type A quintom in which w changes from >-1 to <-1 and type B quintom in which w changes from <-1 to >-1 as the universe expands.
dc.description5 pages, 2 figures, RevTeX, Accepted for publication as a Brief Report in Physical Review D
dc.identifierhttps://arxiv.org/abs/astro-ph/0608165
dc.identifierhttp://arxiv.org/abs/astro-ph/0608165
dc.identifierPhys.Rev.D74:127304,2006
dc.identifierdoi:10.1103/PhysRevD.74.127304
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/181137
dc.subjectAstrophysics
dc.titleTwo-Field Quintom Models in the w-w' Plane
dc.typetext

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