期刊
ASTROPHYSICS AND SPACE SCIENCE
卷 348, 期 2, 页码 559-564出版社
SPRINGER
DOI: 10.1007/s10509-013-1579-y
关键词
Dark energy; Bianchi type-VI model; Viscous fluid; Cosmological constant
In this paper, we investigate Bianchi type-VI cosmological model for the universe filled with dark energy and viscous fluid in the presence of cosmological constant. Also, we show accelerating expansion of the universe by drawing volume scale, pressure and energy density versus cosmic time. In order to solve the Einstein's field equations, we assume the expansion scalar is proportional to a component of the shear tensor. Therefore, we obtain the directional scale factors and show the EOS parameter crosses over phantom divided-line.
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