Abstract
We present in this paper a LRS Bianchi type I cosmological model with dark matter and anisotropic ghost dark energy in presence of magnetic field. We have solved the Einstein’s field equations with a particular form of Hubble parameter. The physical and geometrical behaviors of the model are discussed. It is observed that the anisotropy of the universe and that of the ghost dark energy tends to zero at late times and the universe becomes spatially homogeneous, isotropic and flat. The coincidence parameter increases with time. We have also studied the statefinder parameters. The results obtained are in agreement with the recent days observations.
This is a preview of subscription content, log in via an institution to check access.
Similar content being viewed by others
References
Ade, P.A.R., et al.: arXiv:1303.5076 (2013)
Adhav, K.S.: Int. J. Astron. Astrophys. 1, 204 (2011)
Adhav, K.S., Bansod, A.S., Munde, S.L., Nakwal, R.G.: Astrophys. Space Sci. 332, 497 (2012)
Akarsu, Ö., Kilinc, C.B.: Astrophys. Space Sci. 326, 315 (2010)
Armendariz-Picon, C., et al.: Phys. Rev. D 63, 103510 (2001)
Bagla, J.S., Jassal, H.K., Padmanabhan, T.: Phys. Rev. D 67, 063504 (2003)
Barreiro, T., Copeland, E.J., Nunes, N.J.: Phys. Rev. D 61, 12730 (2000)
Bali, R., Pradhan, A.: Chin. Phys. Lett. 24, 585 (2007)
Bali, R., Pareek, U.K., Pradhan, A.: Chin. Phys. Lett. 24, 2455 (2007)
Bento, M.C., Bertolami, O., Sen, A.A.: Phys. Rev. D 66, 043507 (2002)
Bento, M.C., Bertolami, O., Sen, A.A.: Phys. Rev. D 67, 063003 (2003)
Berman, M.S.: Nuovo Cimento B 74, 182 (1983)
Cai, R.G., Tuo, Z.L., Zhang, H.B., Su, Q.: Phys. Rev. D 84, 123501 (2011)
Cai, R.G., Tuo, Z.L., Wu, Y.B., Zhao, Y.Y.: arXiv:1201.2494v2 [astro-ph.CO] (2012)
Caldwell, R.R.: Phys. Lett. B 23, 545 (2002)
Cadwell, R.R., Doran, M.: Phys. Rev. D 69, 103517 (2004)
Copeland, E.J., Sami, M., Tsujikawa, S.: Int. J. Mod. Phys. D 15, 1753 (2006)
Daniel, S.F.: Phys. Rev. D 77, 103513 (2008)
Ellis, G.F.R.: Gen. Relativ. Gravit. 38, 1003 (2006)
Fedeli, C., Moscardini, L., Bartelmann, M.: Astron. Astrophys. 500, 667 (2009)
Hajj-Boutros, J., Sfeila, J.: Int. J. Theor. Phys. 26, 98 (1987)
Holdom, B.: Phys. Lett. B 697, 351–356 (2011). arXiv:1012.0551 [hep-ph]
Katore, S.D., Adhav, K.S., Sancheti, M.M.: Astrophys. Space Sci. 337, 393 (2012)
Khurshudyan, M., Khurshudyan, A.: arXiv:1307.7859v2 (2014)
Koivisto, T., Mota, D.F.: Phys. Rev. D 73, 083502 (2006)
Koivisto, T., Mota, D.F., Cosmol, J.: Astropart. Phys. 08, 021 (2008)
Kumar, S., Yadav, A.K.: Mod. Phys. Lett. A 26, 647 (2011)
Li, M.: Phys. Lett. B 603, 1 (2004)
Lidsey, J.E.: Class. Quantum Gravity 9, 1239 (1992)
MacCallum, M.A.H., Hawking, S.W., Israel, W.: General Relativity. Cambridge University Press, Cambridge (1979)
Mazumder, A.: Gen. Relativ. Gravit. 26, 307 (1994)
Melvin, M.A.: Ann. N.Y. Acad. Sci. 262, 253 (1975)
Misner, C.W.: Astrophys. J. 151, 431 (1968)
Ohta, N.: Phys. Lett. B 695, 41 (2011)
Permutter, S., et al.: Astrophys. J. 517, 565 (1999)
Pradhan, A., Chouhan, D.S.: Astrophys. Space Sci. 331, 697 (2011)
Pradhan, A., Yadav, V.K., Chakrabarty, I.: Indian J. Pure Appl. Math. 32, 789 (2001)
Saha, B.: Mod. Phys. Lett. A 20, 2127 (2005)
Sahni, V., Saini, T.D., Starobinsky, A.A., Alam, U.: JETP Lett. 77, 201 (2003)
Sarkar, S.: Astrophys. Space Sci. 351, 361 (2014)
Urban, F.R., Zhitnitsky, A.R.: Phys. Lett. B 688, 9 (2010)
Weinberg, S.: Rev. Mod. Phys. 61, 1 (1989)
Yadav, A.K., Yadav, L.: Int. J. Theor. Phys. (2010). doi:10.1007/s10773-010-0510-3
Yadav, A.K., Pradhan, A., Singh, A.K.: Astrophys. Space Sci. 337, 379 (2012a)
Yadav, A.K., Rahman, F., Ray, S., Goswami, G.K.: arXiv:1204.0223v3 (2012b)
Zhitnitsky, A.R.: Phys. Rev. D 82, 103520 (2010). arXiv:1004.2040 [gr-qc]
Zhitnitsky, A.R.: arXiv:1105.6088 [hep-th] (2011)
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
Das, K., Sultana, T. Magnetized anisotropic ghost dark energy cosmological model. Astrophys Space Sci 357, 118 (2015). https://doi.org/10.1007/s10509-015-2346-z
Received:
Accepted:
Published:
DOI: https://doi.org/10.1007/s10509-015-2346-z