Parametrizations of the Dark Energy Density and Scalar Potentials

Simple item page
dc.creatorGuo, Zong-Kuan
dc.creatorOhta, Nobuyoshi
dc.creatorZhang, Yuan-Zhong
dc.date2006-03-04
dc.date2007-01-23
dc.date.accessioned2026-07-07T11:25:20Z
dc.date.available2026-07-07T11:25:20Z
dc.descriptionWe develop a theoretical method of constructing the scalar (quintessence or phantom) potential directly from the dimensionless dark energy function X(z), the dark energy density in units of its present value. We apply our method to two parametrizations of the dark energy density, the quiessence-Lambda ansatz and the generalized Chaplygin gas model, and discuss some features of the constructed potentials.
dc.description8 pages, 2 figures, ws-mpla.cls, Accepted for publication in Mod. Phys. Lett. A
dc.identifierhttps://arxiv.org/abs/astro-ph/0603109
dc.identifierhttp://arxiv.org/abs/astro-ph/0603109
dc.identifierMod.Phys.Lett.A22:883-890,2007
dc.identifierdoi:10.1142/S0217732307022839
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/195475
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleParametrizations of the Dark Energy Density and Scalar Potentials
dc.typetext

Files

Collections

arXiv