论文标题
熵的基本程度如何？从非扩展统计和黑洞物理学到全息黑暗宇宙
How fundamental is entropy? From non-extensive statistics and black hole physics to the holographic dark universe
论文作者
论文摘要
我们提出了一种新的熵构建体，该结构将Tsallis，Rényi，Sharma-Mittal，Barrow，Kaniadakis和Loop量子重力熵概括并减少到Bekenstein-Hawking Entropy。该建议应用于Schwarzschild黑洞，并在空间均质和各向同性的宇宙学上应用，它表明它可以潜在地描述通货膨胀和/或全息暗能量。
We propose a new entropy construct that generalizes the Tsallis, Rényi, Sharma-Mittal, Barrow, Kaniadakis, and Loop Quantum Gravity entropies and reduces to the Bekenstein-Hawking entropy in a certain limit. This proposal is applied to the Schwarzschild black hole and to spatially homogeneous and isotropic cosmology, where it is shown that it can potentially describe inflation and/or holographic dark energy.
