Correspondence between Yang-Mills Condensate Dark Energy with Various Kinds of Scalar Field Models of Dark Energy

被引：2
|
作者：
Saha, Pameli [1 ]
Debnath, Ujjal [1 ]
机构：
[1] Indian Inst Engn Sci & Technol, Dept Math, Sibpur 711103, Howrah, India
来源：
COMMUNICATIONS IN THEORETICAL PHYSICS | 2016年 / 66卷 / 05期
关键词：
dark energy; scalar field models; correspondence; GALAXY REDSHIFT SURVEY; COSMOLOGICAL CONSEQUENCES; MICROWAVE; MATTER; UNIVERSE; QUANTUM; PHANTOM; PERTURBATIONS; OMEGA(LAMBDA); DECELERATION;
D O I：
10.1088/0253-6102/66/5/579
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
In this work, we study a new kind of dark energy (DE), which is named as "Yang-Mills condensate" (YMC). We study the stability and w(de) - w'(de) analysis of YMC DE model. Then we correspond it with quintessence, k-essence, tachyon, phantom, dilaton, DBI-essence and hessence scalar field models of DE in FRW spacetime to reconstruct potentials as well as the dynamics for these scalar fields for describing the acceleration of the universe. We also analyze the models in graphically to interpret the nature of the scalar fields and corresponding potentials.
引用
收藏
页码：579 / 588
页数：10
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