论文标题
用$ f（r，t）$ dravility在thde中重建thde的典型领域
Reconstruction of quintessence field for the THDE with swampland correspondence in $f(R,T)$ gravity
论文作者
论文摘要
在目前的工作中，我们在$ f（r，t）$重力中构建了tsallis全息典型模型，其中哈勃式的地平线为红外线。在平坦的FRW背景中，与Tsallis全息密度的典型模型的能量密度之间的对应关系允许重建动力学和典当场的电位。 THDE密度对两种特定情况的建议的Hubble地平线截止值：（i）THDE 1和（ii）THDE 2。我们已经重建了TSALLIS全息图中的tsallis全息质量模型$ω_λ_λ> - 两种情况的EOS参数。此外，用赃物猜想分析了THDE模型的典型阶段，以描述宇宙的加速膨胀。
In the present work, we construct the Tsallis holographic quintessence model of dark energy in $f(R, T)$ gravity with Hubble horizon as IR cut-off. In a flat FRW background, the correspondence among the energy density of the quintessence model with the Tsallis holographic density permits the reconstruction of the dynamics and the potentials for the quintessence field. The suggested Hubble horizon infrared cut-off for the THDE density acts for two specific cases: (i) THDE 1 and (ii) THDE 2. We have reconstructed the Tsallis holographic quintessence model in the region $ω_Λ > -1$ for the EoS parameter for both the cases. In addition, the quintessence phase of the THDE models is analyzed with swampland conjecture to describe the accelerated expansion of the Universe.
