论文标题
严重的热发动机大量重力
Critical Heat Engines in Massive Gravity
论文作者
论文摘要
在扩展的热力学中，我们研究了效率$η_k$的关键加热发动机，用于球形（$ k = 1 $），FLAT（$ k = 0 $）和双曲线（$ k = -1 $）拓扑的巨大重力（$ k = 1 $）。虽然，$η_k$通常是双曲线（球形）拓扑的较高（较低），但我们表明，该顺序可以在球形拓扑的关键热引擎中逆转，效率较高，尤其是顺序：$η_{\ rm -1}^{\ rm -1}^{ 0}^{\ phantom {0}}<η_{\ rm +1}^{\ phantom {+1}} $。此外，对临界孔的近地平线区域的研究表明，除了已知的$ q \ rightarrow \ infty $条件外，还需要基于几何学的拓扑结构的其他大量重力参数，以揭示出具有消失的宇宙学常数的完全脱钩的Rindler时空。
With in the extended thermodynamics, we study the efficiency $η_k$ of critical heat engines for charged black holes in massive gravity for spherical ($k=1$), flat ($k=0$) and hyperbolic ($k=-1$) topologies. Although, $η_k$ is in general higher (lower) for hyperbolic (spherical) topology, we show that this order can be reversed in critical heat engines with efficiency higher for spherical topology, following in particular the order: $ η_{\rm -1}^{\phantom{-1}} < η_{\rm 0}^{\phantom{0}} < η_{\rm +1}^{\phantom{+1}}$. Furthermore, the study of the near horizon region of the critical hole shows that, apart from the known $q\rightarrow \infty $ condition, additional scalings of massive gravity parameters, based on the topology of the geometry are required, to reveal the presence of a fully decoupled Rindler space-time with vanishing cosmological constant.
