This work reports the effect of thermal radiation on singularities in the presence of holographic Ricci dark energy (HRDE) with generalized IR cut-off. The Eckart approach has been considered to initiate the study. The density of HRDE, which is a just particular cases of general Nojiri–Odintsov (NO) HDE [S. Nojiri and S. D. Odintsov, Unifying phantom inflation with late-time acceleration: Scalar phantom-non-phantom transition model and generalized holographic dark energy, Gen. Relativ. Gravit. 38(8) (2006) 1285–1304], in non-interacting and non-viscous case has been reconstructed and it is found that with the passage of cosmic time t, it is decreasing. The Equation of State (EoS) parameter of HRDE in non-interacting and viscous scenario, the EoS parameter of modified Chaplygin gas (MCG) in a non-interacting and non-viscous scenario and the EoS parameter of MCG in an interacting and non-viscous scenario have been reconstructed and studied. There is a chance of Type I, Type II, Type III, Type IV and $w$-singularities for the conditions we obtained. For the effect of thermal radiation of inhomogeneous viscous fluid in an interacting scenario, there is a scope of avoidance of Big-Rip Singularity.

这项工作报告了在具有广义 IR 截止的全息 Ricci 暗能量 (HRDE) 存在下热辐射对奇点的影响。Eckart 方法已被考虑启动该研究。HRDE 的密度，这是一般 Nojiri-Odintsov (NO) HDE [S. Nojiri 和 SD Odintsov，统一幻象膨胀与后期加速：标量幻象-非幻象过渡模型和广义全息暗能量，Gen. Relativ。重力。 38（8）（2006）1285-1304]，在非相互作用和非粘性情况下进行了重构，发现随着宇宙时间t的流逝, 它正在减少。非相互作用和粘性情景中 HRDE 的状态方程 (EoS) 参数、非相互作用和非粘性情景中改进的 Chaplygin 气体 (MCG) 的 EoS 参数以及相互作用和非粘性情景中 MCG 的 EoS 参数粘性情景已被重建和研究。有机会出现 I 型、II 型、III 型、IV 型和$w$- 我们获得的条件的奇点。对于相互作用场景中非均匀粘性流体的热辐射效应，存在一定范围的大裂口奇点规避。