In this paper we have investigated Bianchi Type-I cosmological model with varying cosmological constant A in f (R, T) theory of gravity. In order to obtain an exact solution of the field equations, we have used a special law of Hubble parameter proposed by Banerjee and Das (Gen Relat Gravit 37 (2005) 1695-1703), which leads to a time dependent deceleration parameter. We have discussed the physical and kinematical properties of the model in detail. The statefinder diagnostic parameters have also been considered. It has been shown that our universe model is consistent with the recent observations and approaches the ACDM model at late times.
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Mangosuthu Univ Technol, Fac Nat Sci, ZA-4026 Jacobs, Kwazulu Natal, South AfricaMangosuthu Univ Technol, Fac Nat Sci, ZA-4026 Jacobs, Kwazulu Natal, South Africa
Beesham, A.
Tiwari, R. K.
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APS Univ, Dept Math Sci, Rewa 486001, Madhya Pradesh, IndiaMangosuthu Univ Technol, Fac Nat Sci, ZA-4026 Jacobs, Kwazulu Natal, South Africa
Tiwari, R. K.
Shukla, B. K.
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Govt Coll Bandri, Dept Math, Sagar 470442, Madhya Pradesh, IndiaMangosuthu Univ Technol, Fac Nat Sci, ZA-4026 Jacobs, Kwazulu Natal, South Africa
Shukla, B. K.
Sofuoglu, D.
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Istanbul Univ, Dept Phys, Vezneciler, TR-34134 Istanbul, TurkiyeMangosuthu Univ Technol, Fac Nat Sci, ZA-4026 Jacobs, Kwazulu Natal, South Africa
Sofuoglu, D.
Tiwari, A.
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JNCT, Dept Math, Rewa 486001, Madhya Pradesh, IndiaMangosuthu Univ Technol, Fac Nat Sci, ZA-4026 Jacobs, Kwazulu Natal, South Africa
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Imam Mohammad Ibn Saud Islamic Univ IMSIU, Dept Math & Stat, Riyadh 13318, Saudi Arabia
Univ Khartoum, Fac Sci, Dept Phys, POB 321, Khartoum 11115, Sudan
North West Univ, Ctr Space Res, ZA-2520 Potchefstroom, South AfricaGovt Coll, Dept Math, Bandri Sagar 470442, MP, India