Exponential Potentials and Attractor Solution of Dilatonic Cosmology

dc.creatorFang, Wei
dc.creatorLu, H. Q.
dc.creatorHuang, Z. G.
dc.date2006-06-05
dc.date2007-04-30
dc.date.accessioned2026-07-07T11:06:37Z
dc.date.available2026-07-07T11:06:37Z
dc.descriptionWe present the scalar-tensor gravitational theory with an exponential potential in which pauli metric is regarded as the physical space-time metric. We show that it is essentially equivalent to coupled quintessence(CQ) model. However for baryotropic fluid being radiation there are in fact no coupling between dilatonic scalar field and radiation. We present the critical points for baryotropic fluid and investigate the properties of critical points when the baryotropic matter is specified to ordinary matter. It is possible for all the critical points to be attractors as long as the parameters $λ$ and $β$ satisfy certain conditions. To demonstrate the attractor behaviors of these critical points, We numerically plot the phase plane for each critical point. Finally with the bound on $β$ from the observation and the fact that our universe is undergoing an accelerating expansion, we conclude that present accelerating expansion is not the eventual stage of universe. Moreover, we numerically describe the evolution of the density parameters $Ω$ and the decelerating factor $q$, and computer the present values of some cosmological parameters, which are consistent with current observational data.
dc.description10 pages, 8 figures, add some references, revised version for Int.J.Theor.Phys. appeared in Int.J.Theor.Phys
dc.identifierhttps://arxiv.org/abs/hep-th/0606032
dc.identifierhttp://arxiv.org/abs/hep-th/0606032
dc.identifierInt.J.Theor.Phys.46:2366-2377,2007
dc.identifierdoi:10.1007/s10773-007-9354-x
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/189580
dc.subjectHigh Energy Physics - Theory
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleExponential Potentials and Attractor Solution of Dilatonic Cosmology
dc.typetext

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