TILTED LRS BIANCHI TYPE-VIo DARK ENERGY COSMOLOGICAL MODEL

Main Article Content

Neha .
Mihiret Tulamo Tupala
Sultan Ahmad
Subrata Kumar Sahu

Abstract

Tilted LRS Bianchi-VIo dark energy cosmological model is investigated in Einstein’s theory of gravitation. We obtained solutions by considering shear scalar  proportional to expansion scalar and deceleration  parameter. Further we obtained an accelerating universe subject to the small value of the anisotropic parameter. Some physical and geometrical properties of the solutions are also discussed.

Downloads

Download data is not yet available.

Article Details

How to Cite
., N., Tupala, M., Ahmad, S., & Sahu, S. (2024). TILTED LRS BIANCHI TYPE-VIo DARK ENERGY COSMOLOGICAL MODEL. Journal of the Tensor Society, 17(01). https://doi.org/10.56424/jts.v17i01.198
Section
Articles

References

1. A.R .King, G.F.R .Ellis, Commun. Math. Phys.31, 209 (1973).
2. G.F.R .Ellis, A.R .King, Commun. Math. Phys.38, 119 (1974).
3. C.B. Collins, G.F.R .Ellis,Phys. Rep. 56, 65 (1979).
4. R. Bali, K. Sharma, Astrophys. Space Sci.271, 227 (2000).
5. R. Bali, K. Sharma,Pramana.58(3), 457 (2002).
6. D.D. Pawar,S.W. Bhaware, A.G. Deshmukh, Rom. J Phys.54, 187(2009).
7. V. U. M. Rao, M. V.Santhi, Y. Aditya, G. Suryanarayana, The African Review of Phy.11, 5(2016).
8. S.K. Sahu,A. G. Goda,G. G.Weldemariam,Astrophys Space Sci357,134 (2015).
9. S.K.Sahu,S.G.Ganebo, G.G.WeldemariamIran J. Sci. Tech.Trans. Sci. DOI 10.1007/s40995-017- 0178-0 (2017) .
10. A.G.Riess et al., Astron. J.116,1009 (1998).
11. A.G.Riess et al., Astrophys. J. 607, 665 (2004).
12. S. Perlmutter et al., Nature, 391, 51 (1998).
13. R. Knop et al.,Astrophys. J. 598, 102 (2003).
14. P. Astieret al., Astron. Astrophys., 447, 31 (2006).
15. D.J. Eisenstein et al., Astrophys. J. 633, 560 (2005).
16. P.A.R. Ade et al., Planck Collaboration , arXiv:1303.5076[astroph.CO] (2013).
17. P.A.R. Ade et al., Planck Collaboration), arXiv:1303.5082[astroph.CO] (2013)
18. B.Ratra , P.J.E. Peebles, Phys. Rev. D 37, 321 (1998).
19. R.R.Caldwell, Phys. Lett.B545, 23 (2002).
20. V. Sahni, A.Starobinsky, Int. J. Mod. Phys. D 15 (12),2105(2006).
21. M. Tegmark et al,Astrophys. J. 606 ,702 (2004).
22. J. Kujat, A. M. Linn, R. J. Scherrer, D. H. Weinberg,Astrophys. J. 572, 1 (2002).
23. M. Bartelmann, K. Dolagb, F. Perrotta et al., Astronomy Rev.49( 2–6), 199 (2005).
24. S. K. Tripathy, K.L Mahanta, Eur. Phys. J. 130 30 (2015).
25. A. G. Riess et al., Astrophys. J. 607, 665 (2004).
26. D. Rapetti et al., Mon. Not. Roy. Astron. Soc. 375, 1510 (2007).
27. R. Giostriet al., J. Cosmol. Astropart. Phys., 1203, 027 (2012).
28. P K Sahoo and M Sivakumar, Astrophysics and Space Science , 357,60 (2015)

Most read articles by the same author(s)

Obs.: This plugin requires at least one statistics/report plugin to be enabled. If your statistics plugins provide more than one metric then please also select a main metric on the admin's site settings page and/or on the journal manager's settings pages.