Cosmology in f(R, T) gravity with quadratic deceleration parameter
Bïnaya K. Bishi, Aroonkumar Beesham, K. L. Mahanta
Abstract
Bïnaya K. Bishi, Aroonkumar Beesham, K. L. Mahanta
Abstract
Abstract In this work, we have developed FLRW cosmological models in f(R, T) gravity. The solution of the modified field equations are obtained under the newly proposed Bakry and Shafeek, “The periodic universe with varying deceleration parameter of the second degree,” Astrophys. Space Sci., vol. 364, p. 135, 2019, quadratic form of the deceleration parameter. Further, we have discussed the state-finder parameter, om-diagnostic analysis and energy conditions of the proposed model. The variation of deceleration parameter with respect to cosmic time and red-shift is consistent with observational data.
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Abstract In this work, we have developed FLRW cosmological models in f(R, T) gravity. The solution of the modified field equations are obtained under the newly proposed Bakry and Shafeek, “The periodic universe with varying deceleration parameter of the second degree,” Astrophys. Space Sci., vol. 364, p. 135, 2019, quadratic form of the deceleration parameter. Further, we have discussed the state-finder parameter, om-diagnostic analysis and energy conditions of the proposed model. The variation of deceleration parameter with respect to cosmic time and red-shift is consistent with observational data.
Key concepts: Deceleration parameter, Friedmann–Lemaître–Robertson–Walker metric, Physics, Cosmology, Quadratic equation, Mathematical physics, Parameter space, Dark energy