首页> 外文期刊>International journal of modern physics, D. Gravitation, astrophysics, cosmology >Study of some cosmological parameters for interacting new holographic dark energy model in f(T) gravity
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Study of some cosmological parameters for interacting new holographic dark energy model in f(T) gravity

机译:f(T)重力作用下与新全息暗能量模型相互作用的一些宇宙学参数的研究

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The present work is based on the idea of an interacting framework of new holographic dark energy (HDE) with cold dark matter in the background of f(T) gravity. Here, we have considered the flat modified Friedmann universe for f(T) gravity which is filled with new HDE and dark matter. We have derived some cosmological parameters like deceleration parameter, equation of state (EoS) parameter, state-finder parameters, cosmographic parameters, Om parameter and graphically investigated the nature of these parameters for the above mentioned interacting scenario. The results are found to be consistent with the accelerating universe. Also, we have graphically investigated the trajectories in omega-omega' plane for different values of the interacting parameter and explored the freezing region and thawing region in omega-omega' plane. Finally, we have analyzed the stability of this model.
机译:当前的工作是基于f(T)引力背景下新的全息暗能量(HDE)与冷暗物质相互作用框架的想法。在这里,我们已经考虑了f(T)引力的平坦修改的Friedmann宇宙,其中充满了新的HDE和暗物质。我们得出了一些宇宙学参数,例如减速参数,状态方程(EoS)参数,状态查找器参数,宇宙学参数,Om参数,并以图形方式研究了上述交互场景下这些参数的性质。发现结果与宇宙加速一致。此外,我们已经图形化地研究了欧米茄-欧米茄'平面中相互作用参数的不同值的轨迹,并探索了欧米茄-欧米茄'平面中的冻结区域和解冻区域。最后,我们分析了该模型的稳定性。

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