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arXiv 2209.04348gr-qchep-th
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Weyl型$f(Q,T)$引力中无发散减速参数的相互作用

Interaction of divergence-free deceleration parameter in Weyl-type $f(Q,T)$ gravity

Gaurav N. Gadbail, Simran Arora, Praveen Kumar, P. K. Sahoo

摘要:

研究了对称远程平行引力的一种推广,即Weyl型$f(Q,T)$引力和减速参数$q(z) = q_{0}+q_{1}\frac{z(1+z)}{1+z^2}$($q_{0}$和$q_{1}$为自由常数)的无发散参数化,以探讨宇宙的演化.考虑$q$的上述参数形式,我们导出了Hubble解,并进一步将其应用于Weyl型$f(Q, T)$引力的Friedmann方程中.为了观察该模型是否能够挑战$Λ$ CDM限制,我们使用观测哈勃数据($OHD$)和万神殿样本($SNe\,Ia$)的贝叶斯分析计算了模型参数的约束。此外,减速参数用当前值$q_0$和跃迁红移$z_t$(膨胀从减速过渡到加速)以及$1-σ$和$2-σ$置信水平来描述宇宙的加速行为。我们还研究了能量密度,压力和有效状态方程参数的演变。最后,我们证明了减速参数的无发散参数形式与Weyl型$f(Q,T)$引力是一致的。

英文摘要:

We study an extension of symmetric teleparallel gravity i.e. Weyl-type $f(Q,T)$ gravity and the divergence-free parametrization of the deceleration parameter $q(z) = q_{0}+q_{1}\frac{z(1+z)}{1+z^2}$ ($q_{0}$ and $q_{1}$ are free constants) to explore the evolution of the universe. By considering the above parametric form of $q$, we derive the Hubble solution and further impose it in the Friedmann equations of Weyl-type $f(Q, T)$ gravity. To see whether this model can challenge the $Λ$CDM limits, we computed the constraints on the model parameters using the Bayesian analysis for the Observational Hubble data ($OHD$) and the Pantheon sample ($SNe\,Ia$). Furthermore, the deceleration parameter depicts the accelerating behavior of the universe with the present value $q_0$ and the transition redshift $z_t$ (at which the expansion transits from deceleration to acceleration) with $1-σ$ and $2-σ$ confidence level. We also examine the evolution of the energy density, pressure, and effective equation of state parameters. Finally, we demonstrate that the divergence-free parametric form of the deceleration parameter is consistent with the Weyl-type $f(Q,T)$ gravity.

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