Abstract
In this paper, we have searched the existence of Λ-dominated anisotropic universe filled with magnetized strings. The observed acceleration of universe has been explained by introducing a positive cosmological constant Λ in the Einstein’s field equation which is mathematically equivalent to dark energy with equation of state (EOS) parameter set equal to −1. The present values of the matter and the dark energy parameters (Ω m )0 & (ΩΛ)0 are estimated for high red shift (.3 ≤ z ≤ 1.4) SN Ia supernova data’s of observed apparent magnitude along with their possible error taken from Union 2.1 compilation. It is found that the best fit value for (Ω m )0 & (ΩΛ)0 are 0.2920 & 0.7076 respectively which are in good agreement with recent astrophysical observations in the latest surveys like WMAP and Plank. Various physical parameters such as the matter and dark energy densities, the present age of the universe and the present value of deceleration parameter have been obtained on the basis of the values of (Ω m )0 & (ΩΛ)0.Also, we have estimated that the acceleration would have begun in the past at z = 0.6845 i. e. 6.2341 Gyrs before from now.
Similar content being viewed by others
References
Riess, A.G., et al.: APJ 116, 1009 (1998)
Perlmutter, S., et al.: APJ 517, 565 (1999)
Grøn, Ø., Hervik, S.: Einstien’s General Theory of Relativity: With Modern Application in Cosmology. Springer, New York (2007)
Carroll, S.M., Press, W.H., Turner, E.L.: Ann. Rev. Astron. Astrophys. 30, 499 (1992)
Copeland, E.J., Sami, M., Tsujikawa, S.: Int. J. Mod. Phys. D 15, 1753 (2006)
Alam, U., Sahni, V., Saini, T.D., Starobinsky, A.A.: MNRAS 344, 1057 (2003)
Komastu, E., et al.: Astrophys. J. Suppl. Ser. 180, 330 (2009)
Astier, P., et al.: Astron. Astrophys. 447, 31 (2006)
Yadav, A.K., Rahaman, F., Ray, S., Goswami, G.K.: Euro. Phys. J. Plus. 127, 127 (2012)
Yadav, A.K., Saha, B.: Astrophys. Space Sci. 341, 651 (2012)
Kumar, S., Yadav, A.K.: Mod. Phys. Lett. A 26, 647 (2011)
Yadav, A.K.: Astrophys. Space Sci. 335, 565 (2011)
Yadav, A.K., Rahaman, F., Ray, S.: Int. J. Theor. Phys. 50, 871 (2011)
Yadav, A.K., Yadav, L.: Int. J. Theor. Phys. 50, 218 (2011)
Sahoo, P.K. Forts. der Physik 64, 414 (2016)
Sahoo, P.K. Int. J. Theor. Phys. 49, 25 (2010)
Sahoo, P.K. Int. J. Theor. Phys. 48, 2022 (2009)
King, E.J., Coles, P.: CQG 24, 2061 (2007)
Barrow, J.D., Ferreira, P.G., Silk, J.: PRL 78, 3610 (1997)
Goswami, G.K., Yadav, A.K., Mishra, M.: Int. J. Theor. Phys. 54, 315 (2015)
Goswami, G.K., Dewangan, R.N., Yadav, A.K., Pradhan, A.: Astrophys. Space Sci. 361, 1 (2016a)
Goswami, G.K., Dewangan, R.N., Yadav, A.K.: Astrophys. Space Sci. 361, 119 (2016b)
Amanullah, R., et al.: Astrophys. J. 716, 712 (2010)
Acknowledgments
This work is supported by the CGCOST Minor Research Project 789/CGCOST/MRP/14. Authors are thankful to IUCAA, Pune, India for providing facility and support where part of this work was carried out.
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
Goswami, G.K., Yadav, A.K. & Dewangan, R.N. Magnetised Strings in Λ-Dominated Anisotropic Universe. Int J Theor Phys 55, 4651–4664 (2016). https://doi.org/10.1007/s10773-016-3086-8
Received:
Accepted:
Published:
Issue Date:
DOI: https://doi.org/10.1007/s10773-016-3086-8