论文标题
新的熵，黑洞和全息暗能量
New entropies, black holes, and holographic dark energy
论文作者
论文摘要
Bekenstein-Hawking熵是地平线热力学的基石，但量子效应纠正了，而不相等的熵也出现在非扩展的热力学中。回顾我们以前的工作，我们主张建立一种新的熵结构，该结构包括最近和旧的建议，并满足了四个最小的关键特性。然后将新提案应用于黑洞和全息暗能量，并显示有可能引起早期宇宙通胀或减轻当前的哈勃张力。然后，我们分析与替代熵一致的黑洞温度和质量。
The Bekenstein-Hawking entropy is a cornerstone of horizon thermodynamics but quantum effects correct it, while inequivalent entropies arise also in non-extensive thermodynamics. Reviewing our previous work, we advocate for a new entropy construct that comprises recent and older proposals and satisfies four minimal key properties. The new proposal is then applied to black holes and to holographic dark energy and shown to have the potential to cause early universe inflation or to alleviate the current Hubble tension. We then analyze black hole temperatures and masses consistent with alternative entropies.
