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Universe Filled with a Binary Mixture of Perfect Fluid and Dark Energy

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Abstract

We consider a self consistent system of Bianchi type-V gravitational field and a binary mixture of perfect fluid and dark energy. The perfect fluid is taken to be the one obeying the usual equation of state, i.e., p=γρ, with γ∈[0,1] whereas, the dark energy is considered to be either the quintessence like equation of state or Chaplygin gas. The equation of state parameter for dark energy ω is found to be consistent with the recent observations of SNe Ia data (Knop et al., Astrophys. J. 598:102, 2003), SNe Ia data with CMBR anisotropy and galaxy clustering statistics (Tegmark et al., Astrophys. J. 606:702, 2004) and latest a combination of cosmological datasets coming from CMB anisotropies, luminosity distances of high redshift type Ia supernovae and galaxy clustering (Hinshaw et al., Astrophys. J. Suppl. 180:225, 2009; Komatsu et al., Astrophys. J. Suppl. Ser. 180:330, 2009). The physical and geometrical aspects of the models are also discussed in detail.

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Authors and Affiliations

  1. Department of Mathematics, Birla Institute of Technology and Science (BITS) Pilani, K K Birla, Goa Campus, NH 17B, bypass Road, Zuarinagar, 403726, Goa, India

    G. C. Samanta & S. N. Dhala

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  1. G. C. Samanta
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  2. S. N. Dhala
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Correspondence to S. N. Dhala.

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Samanta, G.C., Dhala, S.N. Universe Filled with a Binary Mixture of Perfect Fluid and Dark Energy. Int J Theor Phys 52, 3092–3105 (2013). https://doi.org/10.1007/s10773-013-1601-8

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  • DOI: https://doi.org/10.1007/s10773-013-1601-8

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