Abstract
We investigate the anisotropic locally rotationally symmetric (LRS) Bianchi type I cosmological model with dark matter and anisotropic dark energy. We assume that the shear scalar \((\sigma )\) is proportional to expansion scalar \((\theta )\). A special law is introduced for two skewness parameters that describe the deviation of pressure from isotropy. This law can lead to models: the hybrid expansion, the big rip and the little rip. The behavior of the Universe is discussed depending on the numerical parameters of the models.
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References
Ade, P.A.R., et al., (Planck Collaboration) Astron. Astrophys. 594, A11 (2016a)
Ade, P.A.R., et al., (Planck Collaboration) Astron. Astrophys. 594, A13 (2016b)
Ade, P.A.R., et al., (Planck Collaboration) Astron. Astrophys. 594, A16 (2016c)
Ade, P.A.R., et al., (Planck Collaboration) Astron. Astrophys. 594, A20 (2016d)
Akarsu, O., et al.: J. Cosmol. Astropart. Phys. 01, 022 (2014)
Akarsu, O., Kilinc, C.B.: Gen. Relativ. Gravit. 42, 119 (2010)
Bali, R., Banerjee, R., Banerjee, S.K.: Astrophys. Space Sci. 317, 21 (2008)
Bennett, C.L., et al.: Astrophys. J. 464, L1–L4 (1996)
Caldwell, R.R., Kamionkowski, M., Weinberg, N.N.: Phys. Rev. Lett. 91, 071301 (2003)
Collins, C.B.: Phys. Lett. A 60, 397 (1977)
Collins, C.B., Glass, E.N., Wilkinson, D.A.: Gen. Relativ. Gravit. 12, 805 (1980)
Copi, C.J., et al.: Mon. Not. R. Astron. Soc. 367, 79–102 (2006)
Ellis, G.F.R.: Gen. Relativ. Gravit. 38(6), 1003–1015 (2006)
Eriksen, H.K., et al.: Astrophys. J. 605, 14–20 (2004)
Frampton, P.H., Takahashi, T.: Phys. Lett. B 557, 135 (2003)
Hinshaw, G., et al.: Astrophys. J. Suppl. Ser. 148, 135 (2003)
Hinshaw, G., et al.: Astrophys. J. Suppl. Ser. 170, 288 (2007)
Hinshaw, G., et al.: Astrophys. J. Suppl. Ser. 180, 225–245 (2009)
Kantowski, R., Sachs, R.K.: J. Math. Phys. 7, 433 (1966)
Koivisto, T., Mota, D.F.: Astrophys. J. 679, 1 (2008)
Koivisto, T., Mota, D.F., Koivisto, T., Mota, D.F.: (2008). arXiv:0801.3676v2
Komatsu, E., et al.: Astrophys. J. Suppl. Ser. 180, 330 (2009)
Kristian, J., Sachs, R.K.: Astrophys. J. 143, 379 (1966)
Melchiorri, A., Mersimi, L., Odman, C.J., Trodden, M.: Phys. Rev. D 68, 043509 (2003)
Nojiri, S., Odintsov, S.D.: Phys. Rev. D 72, 023003 (2005)
Nolta, M.R., et al.: Astrophys. J. Suppl. Ser. 180, 296–305 (2009)
Parsons, P., Barrow, J.D.: Class. Quantum Gravity 12, 1715 (1995)
Rodrigues, D.C.: Phys. Rev. D 77, 023534 (2008)
Roy, S.R., Banerjee, S.K.: Class. Quantum Gravity 11, 1943 (1995)
Roy, S.R., Singh, J.P., Narin, S.: Aust. J. Phys. 38, 239 (1985)
Saha, B., Yadav, A.K.: Astrophys. Space Sci. 337, 759 (2012)
Sharif, M., Zubair, M.: Astrophys. Space Sci. 330, 399 (2010)
Smoot, G.F., et al.: Astrophys. J. 396, L1 (1992)
Thorne, K.S.: Astrophys. J. 148, 51 (1967)
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)
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Muharlyamov, R.K., Pankratyeva, T.N. The anisotropic distribution of the dark energy within the scope of LRS Bianchi type I model. Astrophys Space Sci 363, 32 (2018). https://doi.org/10.1007/s10509-018-3253-x
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DOI: https://doi.org/10.1007/s10509-018-3253-x