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Generalized second law of thermodynamics in the emergent universe for some viable models of f(T) gravity

机译:f(T)引力某些可行模型在涌现宇宙中的热力学广义第二定律

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The present work is motivated by the study of the paper K. Karami, A. Abdolmaleki, J. Cosmol. Astropart. Phys. 04, 007 (2012), where the generalized second law (GSL) of thermodynamics has been investigated for a flat FRW universe for three viable models of f(T) gravity. We have here considered a non-flat universe and, accordingly, studied the behaviors of the equation-of-state (EoS) parameter. and of the deceleration parameter q. Subsequently, using the first law of thermodynamics, we derived the expressions for the time derivative of the total entropy of a universe enveloped by apparent horizon. In the next phase, with the choice of scale factor a(t) pertaining to an emergent universe, we have investigated the sign of the time derivatives of total entropy for the models of f(T) gravity considered.
机译:当前的工作是由对论文K.Karami,A.Abdolmaleki,J.Cosmol的研究激发的。天体物理04,007(2012),其中针对三个可行的f(T)重力模型研究了平坦FRW宇宙的热力学广义第二定律(GSL)。我们在这里考虑了非平坦的宇宙,因此研究了状态方程(EoS)参数的行为。和减速参数q。随后,使用热力学第一定律,我们得出了被视界包围的宇宙总熵的时间导数的表达式。在下一阶段,选择与出现的宇宙有关的比例因子a(t),我们研究了所考虑的f(T)引力模型的总熵的时间导数的符号。

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