论文标题
常规黑洞内可检测的宇宙
Detectable universes inside regular black holes
论文作者
论文摘要
虽然据信天体物理黑洞以外附近的时空被众所周知，但事件范围和内部仍然难以捉摸。在这里，我们发现了新型的一般相对性解决方案的堕落无限频谱，具有相同的质量能和熵，描述了天体物理黑洞内的黑能宇宙。这个常规的宇宙黑洞通过在双重宇宙黑孔事件地平线上施加的有限切向压力稳定，该压力局部为量子不确定性。我们从经典的流体熵中恢复了Bekenstein-Hawking熵公式，该公式在托尔曼温度等于宇宙学水平温度的情况下计算出来。我们进一步计算其重力准正常模式。我们发现，通过在$μ{\ rm hz}}中运行的重力波实验可以检测到宇宙黑洞 - {\ rm hz} $范围，就像丽莎太空式交易仪一样。
While spacetime in the vicinity outside astrophysical black holes is believed to be well understood, the event horizon and the interior remain elusive. Here, we discover a degenerate infinite spectrum of novel general relativity solutions with the same mass-energy and entropy that describe a dark energy universe inside an astrophysical black hole. This regular cosmological black hole is stabilized by a finite tangential pressure applied on the dual cosmological-black hole event horizon, localized up to a quantum indeterminacy. We recover the Bekenstein-Hawking entropy formula from the classical fluid entropy, calculated at a Tolman temperature equal to the cosmological horizon temperature. We further calculate its gravitational quasi-normal modes. We find that cosmological black holes are detectable by gravitational-wave experiments operating within the $μ{\rm Hz}-{\rm Hz}$ range, like LISA space-interferometer.
