Logarithmic Entropy Corrected Holographic Dark Energy with F(R, T) Gravity

被引:11
|
作者
Amani, Ali R. [1 ]
Samiee-Nouri, A. [2 ]
机构
[1] Islamic Azad Univ, Ayatollah Amoli Branch, Dept Phys, Fac Sci, Amol, Mazandaran, Iran
[2] Islamic Azad Univ, Dept Phys, Cent Tehran Branch, Tehran, Iran
关键词
equation of state parameter; F(R; T); gravity; logarithmic entropy corrected holographic dark energy; FRW metric; Friedmann equation; PROBE WMAP OBSERVATIONS; BLACK-HOLE; COSMOLOGICAL CONSTANT; INFLATION; UNIVERSE; MODEL;
D O I
10.1088/0253-6102/64/4/485
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
In this paper, we consider F(R,T) gravity as a linear function of the curvature and torsion scalars and interact it with logarithmic entropy corrected holographic dark energy to evaluate cosmology solutions. The model is investigated by FRW metric, and then the energy density and the pressure of dark energy are calculated. Also we obtain equation of state (EoS) parameter of dark energy and plot it with respect to both variable of redshift and e-folding number. Finally, we describe the scenario in three status: early, late and future time by e-folding number.
引用
收藏
页码:485 / 490
页数:6
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