Dynamical Study of a Constant Viscous Dark Energy Model in Classical and Loop Quantum Cosmology

被引:1
作者
Benchikh, Sara [1 ]
Mebarki, Noureddine [1 ]
Aberkane, Dalel [1 ]
机构
[1] Mentouri Univ, Lab Phys Math & Subatom, Route Ain El Bey, Constantine 25000, Algeria
关键词
CURVATURE; EQUATION; UNIVERSE;
D O I
10.1088/0256-307X/33/5/059501
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Dynamical behaviors and stability properties of a flat space Friedmann-Robertson-Walker universe filled with pressureless dark matter and viscous dark energy are studied in the context of standard classical and loop quantum cosmology. Assuming that the dark energy has a constant bulk viscosity, it is found that the bulk viscosity effects influence only the quintessence model case leading to the existence of a viscous late time attractor solution of de-Sitter type, whereas the quantum geometry effects influence the phantom model case where the big rip singularity is removed. Moreover, our results of the Hubble parameter as a function of the redshift are in good agreement with the more recent data.
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页数:5
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