A Comparison of Quintessence and Nonlinear Born-Infeld Scalar Field Using Gold Supernova data

dc.creatorFang, Wei
dc.creatorLu, H. Q.
dc.creatorLi, B.
dc.creatorZhang, K. F
dc.date2005-12-11
dc.date2005-12-21
dc.date.accessioned2026-07-07T07:40:54Z
dc.date.available2026-07-07T07:40:54Z
dc.descriptionWe study the Non-Linear Born-Infeld(NLBI) scalar field model and quintessence model with two different potentials($V(ϕ)=-sϕ$ and ${1/2}m^2ϕ^2$). We investigate the differences between those two models. We explore the equation of state parameter w and the evolution of scale factor $a(t)$ in both NLBI scalar field and quintessence model. The present age of universe and the transition redshift are also obtained. We use the Gold dataset of 157 SN-Ia to constrain the parameters of the two models. All the results show that NLBI model is slightly superior to quintessence model.
dc.description17 pages, 10 figures, some references added
dc.identifierhttps://arxiv.org/abs/hep-th/0512120
dc.identifierhttp://arxiv.org/abs/hep-th/0512120
dc.identifierInt.J.Mod.Phys. D15 (2006) 1947-1962
dc.identifierdoi:10.1142/S0218271806009194
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/121919
dc.subjectHigh Energy Physics - Theory
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleA Comparison of Quintessence and Nonlinear Born-Infeld Scalar Field Using Gold Supernova data
dc.typetext

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