论文标题
扩展$ F（R，G，T）$ GREATITY中的能量条件
Energy Conditions in Extended $f(R,G,T)$ Gravity
论文作者
论文摘要
在本文中，我们考虑了在有完美的流体型号和扩展的$ f（r，g，t）$重力的情况下的Friedmann Lematre Robertson-Walke指标（其中$ r $是RICCI Scalar，$ G $是Gauss Bonnet不变的，而$ t $ t $ to thus to truce to the Energy Momensum Momensum Tensor）。在这种情况下，我们假设一些特定的现实$ f（r，g，t）$模型配置，可用于探索在延迟宇宙加速阶段中出现的有限时间的未来奇异性。在这种情况下，我们选择了哈勃，减速，快速和混蛋参数的最新估计值，以开发由不同能量条件引起的模型参数上的可行性和边界。
In this paper, we consider the flat Friedmann Lematre Robertson-Walke metric in the presence of perfect fluid models and extended $f(R,G,T)$ gravity (where $R$ is the Ricci scalar, $G$ is the Gauss Bonnet invariant and $T$ stands for trace of energy momentum tensor). In this context, we assume some specific realistic $f(R,G,T)$ models configuration that could be used to explore the finite-time future singularities that arise in late-time cosmic accelerating phases. In this scenario, we choose the most recent estimated values for the Hubble, deceleration, snap and jerk parameters to develop the viability and bounds on the models parameters induced by different energy conditions.
