论文标题
统计方法和Schwarzschild黑洞中的Bekenstein界定
Statistical approaches and the Bekenstein bound conjecture in Schwarzschild black holes
论文作者
论文摘要
当今理论物理学的挑战之一是充分了解像区域（如熵）这样的几何对象与恒温物体（如熵）之间的联系，因为区域像熵一样行为相似。 Bekenstein Bound提出了对平坦空间中区域熵的普遍约束。黑洞的Bekenstein-Hawking熵满足了Bekenstein结合的猜想。在本文中，我们已经表明，当我们使用重要的非高斯熵（例如Barrow，Tsallis和Kaniadakis）时，为了描述Schwarzschild Black Hole时，Bekenstein Boundure的猜想似乎失败了。
One of the challenges of today's theoretical physics is to fully understand the connection between a geometrical object like area and a thermostatistical one like entropy, since area behaves analogously like entropy. The Bekenstein bound suggests a universal constraint for the entropy of a region in a flat space. The Bekenstein-Hawking entropy of black holes satisfies the Bekenstein bound conjecture. In this paper we have shown that when we use important non-Gaussian entropies, like the ones of Barrow, Tsallis and Kaniadakis in order to describe the Schwarzschild black hole, then the Bekenstein bound conjecture seems to fail.
