Abstract
A spatially homogeneous and anisotropic Bianchi type-III universe filled with two minimally interacting fields is investigated: matter and holographic dark energy components in the framework of the Brans-Dicke (Phys. Rev. 124:925, 1961) theory of gravitation. To obtain determinate solutions of the field equations we have used (i) scalar expansion proportional to the shear scalar and (ii) special law of variation for Hubble’s parameter proposed by Berman (Nuovo Comento B 74:182, 1983). Some physical and kinematical properties of the model are also discussed.
This is a preview of subscription content, log in via an institution to check access.
Similar content being viewed by others
References
Adhav, K.S., et al.: Astrophys. Space Sci. 353, 249 (2014)
Adhav, K.S., et al.: Astrophys. Space Sci. 359, 24 (2015)
Banerjee, N., Pavon, D.: Phys. Rev. D 63, 043504 (2001)
Berman, M.S.: Nuovo Cimento B 74, 182 (1983)
Bertolami, O., Martins, P.J.: Phys. Rev. D 61, 0604007 (2000)
Bertotti, B., et al.: Nature 425, 374 (2003)
Brans, C.H., Dicke, R.H.: Phys. Rev. 124, 925 (1961)
Cohen, A.G., et al.: Phys. Rev. Lett. 82, 4971 (1999)
Collins, C.B., et al.: Gen. Relativ. Gravit. 12805 (1983)
Das, S., Mammon, A.A.: Astrophys. Space Sci. 351, 651 (2014)
Felice, A.D., et al.: Phys. Rev. D 74, 103005 (2006)
Hooft, G.: arXiv:gr-qc/9310026 (1995)
Horova, P., Minic, D.: Phys. Rev. Lett. 85, 1610 (2000)
Hsu, S.D.H.: Phys. Lett. B 594, 13 (2004)
Kiran, M., et al.: Astrophys. Space Sci. 354, 577 (2014a)
Kiran, M., et al.: Astrophys. Space Sci. 356, 407 (2014b)
Li, M.: Phys. Lett. B 603, 1 (2004)
Linde, A.: Phys. Lett. B 238, 160 (1990)
Mathiazhagan, C., Johri, V.B.: Class. Quantum Gravity 1, 129 (1984)
Nojiri, S., Odintsov, S.D.: Phys. Rev. D 68, 123512 (2003)
Perlmutter, S., et al.: Astrophys. J. 517, 567 (1999)
Pimental, L.O.: Mod. Phys. Lett. A 12, 1865 (1997)
Reiss, A., et al.: Astron. J. 116, 1009 (1998)
Saez, D., Ballester, V.J.: Phys. Lett. A 113, 467 (1986)
Sarkar, S.: Astrophys. Space Sci. 352, 859 (2014a)
Sarkar, S.: Astrophys. Space Sci. 349, 985 (2014b)
Sarkar, S., Mahanta, C.R.: Int. J. Theor. Phys. 52, 1482 (2013)
Setare, M.R.: Phys. Lett. B 644, 99 (2007)
Setare, M.R., Vagenas, E.C.: Int. J. Mod. Phys. D 18, 147 (2009)
Sheykhi, A.: arXiv:0907.5458v4 [hep-th] (2009)
Thomas, S.: Phys. Rev. Lett. 89, 081301 (2002)
Vidyasagar, T., et al.: Eur. Phys. J. Plus 129, 36 (2014)
Author information
Authors and Affiliations
Corresponding author
Ethics declarations
Compliance with ethical standards
The authors declare that they have no potential conflict and will abide by the ethical standards of this journal.
Rights and permissions
About this article
Cite this article
Umadevi, S., Ramesh, G. Minimally interacting holographic dark energy model in Bianchi type-III universe in Brans-Dicke theory. Astrophys Space Sci 359, 51 (2015). https://doi.org/10.1007/s10509-015-2497-y
Received:
Accepted:
Published:
DOI: https://doi.org/10.1007/s10509-015-2497-y