Role of a tachyonic field in accelerating the Universe in the presence of a perfect fluid

被引:4
|
作者
Chakraborty, Writambhara [2 ]
Debnath, Ujjal [1 ]
机构
[1] Bengal Engn & Sci Univ, Dept Math, Sibpur 711103, Howrah, India
[2] New Alipore Coll, Dept Math, Kolkata 700053, India
关键词
acceleration; tachyonic field; perfect fluid;
D O I
10.1007/s10509-008-9795-6
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Recently, a tachyonic field was presented as a dark energy model to represent the present acceleration of the Universe. In this paper, we consider a mixture of tachyonic fluid with a perfect fluid. For this purpose we consider barotropic fluid and Generalized Chaplygin gas (GCG). We present a particular form of the scale factor. We solve the equations of motion to get exact solutions of the density, tachyonic potential and the tachyonic field. We introduce a coupling term to show that the interaction decays with time. We also show that the nature of the potentials vary, so the interaction term reduces the potential in both cases.
引用
收藏
页码:73 / 78
页数:6
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