Minimally interacting holographic Dark energy model in Brans-Dicke theory

In this paper, we have studied the anisotropic and homogeneous Bianchi type-V universe filled with two minimally interacting fields, matter and holographic dark energy components in the frame work of Brans and Dicke (Phys. Rev. 124:925, 1961 ) theory of gravitation. To obtain a determinate solution...

Full description

Saved in:
Bibliographic Details
Published inAstrophysics and space science Vol. 356; no. 2; pp. 407 - 411
Main Authors Kiran, M., Reddy, D. R. K., Rao, V. U. M.
Format Journal Article
LanguageEnglish
Published Dordrecht Springer Netherlands 01.04.2015
Springer Nature B.V
Subjects
Anisotropy
Astrobiology
Astronomy
Astrophysics
Astrophysics and Astroparticles
Cosmology
Dark energy
Frames
Gravitation
Holography
Law
Mathematical analysis
Mathematical models
Observations and Techniques
Original Article
Physics
Physics and Astronomy
Scalars
Shear
Space Exploration and Astronautics
Space Sciences (including Extraterrestrial Physics
Universe
Bianchi type-V universe
Brans-Dicke theory
Holographic dark energy
Online AccessGet full text

Cover

More Information
Summary:In this paper, we have studied the anisotropic and homogeneous Bianchi type-V universe filled with two minimally interacting fields, matter and holographic dark energy components in the frame work of Brans and Dicke (Phys. Rev. 124:925, 1961 ) theory of gravitation. To obtain a determinate solution of the field equations we have used (i) the scalar expansion is proportional to the shear scalar and (ii) special law of variation for Hubble’s parameter proposed by Berman (Nuovo Cimento B 74:182, 1983 ). Some physical and kinematical properties of the model are also discussed.
Bibliography:ObjectType-Article-1
SourceType-Scholarly Journals-1
ObjectType-Feature-2
content type line 23
ISSN:0004-640X
1572-946X
DOI:10.1007/s10509-014-2213-3