标题： 广义幽灵暗能量在f(Q)引力中 显示英文标题

标题： Generalized Ghost Dark Energy in f(Q) Gravity

摘要： 在本文中，我们使用对应原理构建广义鬼暗能量$f(Q)$模型，其中$Q$是非度规性。 为此，我们使用具有幂律尺度因子的弗里德曼-罗伯逊-沃尔克宇宙模型。 此模型中的能量密度线性依赖于哈勃参数，具有$H^{2}$的次主导项，从而得到能量密度$\rho_D=\xi H+\zeta H^{2}$，其中$\xi$和$\zeta$是任意常数。 我们重构了这种暗能量与暗物质的相互作用流体情景。 重新表述的$f(Q)$引力模型展示了这种修改引力模型如何再现宇宙历史的不同时期。 模型的物理特性通过状态方程参数与平面$\omega_{D}-\omega'_{D}$和$r-s$进行讨论。 我们还通过声速的平方探讨了相互作用模型的稳定性准则。 状态方程参数表明宇宙处于幻影相，而声速的平方表示相互作用模型的稳定性。 $(\omega_{D}-\omega^{\prime}_{D})$平面表示冻结区域，而$(r-s)$平面对应于 Chaplygin 气体。 我们得出结论，我们的发现与最新的观测数据一致。 显示英文摘要

摘要： In this manuscript, we use the correspondence principle to construct the generalized ghost dark energy $f(Q)$ model, where $Q$ is the non-metricity. For this purpose, we use the Friedman-Robertson-Walker universe model with power-law scale factor. The energy density in this model linearly depends on the Hubble parameter, with a sub-leading term of $H^{2}$, resulting in an energy density $\rho_D=\xi H+\zeta H^{2}$, where $\xi$ and $\zeta$ are arbitrary constants. We reconstruct interacting fluid scenario of this dark energy with dark matter. The reformulated $f(Q)$ gravity model shows how different epochs of the cosmic history can be reproduced by this modified gravity model. The physical characteristics of the model are discussed through the equation of state parameter with the planes of $\omega_{D}-\omega'_{D}$ and $r-s$. We also explore the stability criteria for the interacting model using the squared speed of sound. The equation of state parameter indicates phantom phase of the universe and the squared speed of sound represents stability of the interacting model. The $(\omega_{D}-\omega^{\prime}_{D})$-plane indicates freezing region, while the $(r-s)$-plane corresponds to the Chaplygin gas. We conclude that our findings coincide with the latest observational data.