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Probing kinematics and fate of the universe with linearly time-varying deceleration parameter
The parametrizations q = q 0+q 1 z and q = q 0+q 1(1 - a/a 0) (Chevallier-Polarski-Linder parametrization) of the deceleration parameter, which are linear in cosmic redshift z and scale factor a, have been frequently utilized in the literature to study the kinematics of the Universe. In this paper,
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