论文标题
评论Lyra几何形状中的Brans-Dicke标量宇宙学模型
Comment on Brans-Dicke Scalar Field Cosmological Model in Lyra's Geometry
论文作者
论文摘要
在本研究中，我们在Lyra的几何形状[Maurya \＆Zia，Phys。 Rev. D \ TextBf {100}，023503（2019）]。在此评论中，我们调查物理作者提出的模型中没有加速。 Rev. d \ textbf {100}，023503（2019）。因此，尽管有相反的说法，但在Lyra的几何形状中，Brans-Dicke标量宇宙学模型具有高brans-dicke（BD）耦合参数$ω$ $ω$和常数$β$无法在宇宙中产生较晚的加速度。
In the present study, we comment on Brans-Dicke scalar field cosmological model in Lyra's geometry [Maurya \& Zia, Phys. Rev. D \textbf{100}, 023503 (2019)]. In this comment, we investigate that there is no acceleration in the model proposed by the authors of Phys. Rev. D \textbf{100}, 023503 (2019). Therefore, despite the claims to the contrary the Brans-Dicke Scalar Field Cosmological Model in Lyra's Geometry with high Brans-Dicke (BD) coupling parameter $ω$ and constant $β$ can not produce late time acceleration in the universe.
