K-Chameleon and the Coincidence Problem

dc.creatorWei, Hao
dc.creatorCai, Rong-Gen
dc.date2004-12-06
dc.date2005-02-09
dc.date.accessioned2026-07-07T10:50:28Z
dc.date.available2026-07-07T10:50:28Z
dc.descriptionIn this paper we present a hybrid model of k-essence and chameleon, named as k-chameleon. In this model, due to the chameleon mechanism, the directly strong coupling between the k-chameleon field and matters (cold dark matters and baryons) is allowed. In the radiation dominated epoch, the interaction between the k-chameleon field and background matters can be neglected, the behavior of the k-chameleon therefore is the same as that of the ordinary k-essence. After the onset of matter domination, the strong coupling between the k-chameleon and matters dramatically changes the result of the ordinary k-essence. We find that during the matter-dominated epoch, only two kinds of attractors may exist: one is the familiar {\bf K} attractor and the other is a completely {\em new}, dubbed {\bf C} attractor. Once the universe is attracted into the {\bf C} attractor, the fraction energy densities of the k-chameleon $Ω_ϕ$ and dust matter $Ω_m$ are fixed and comparable, and the universe will undergo a power-law accelerated expansion. One can adjust the model so that the {\bf K} attractor do not appear. Thus, the k-chameleon model provides a natural solution to the cosmological coincidence problem.
dc.descriptionRevtex, 17 pages; v2: 18 pages, two figures, more comments and references added, to appear in PRD, v3: published version
dc.identifierhttps://arxiv.org/abs/hep-th/0412045
dc.identifierhttp://arxiv.org/abs/hep-th/0412045
dc.identifierPhys.Rev.D71:043504,2005
dc.identifierdoi:10.1103/PhysRevD.71.043504
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/184544
dc.subjectHigh Energy Physics - Theory
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.titleK-Chameleon and the Coincidence Problem
dc.typetext

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