蒸发的四维黑洞形成光球和色球吗？
Do Evaporating 4D Black Holes Form Photospheres and/or Chromospheres?
摘要：
一些作者声称，由于发射粒子之间的QED或QCD相互作用，在黑洞周围形成光球或色球，从而显著地改变了微观黑洞的可观测霍金发射。分析这些模型，我们确定了一些物理和几何效果，使他们无效。在所有的情况下，我们发现，宇宙或银河系背景的黑洞或一个单独的黑洞的观测签名基本上仍然是那些标准的霍金模型，几乎没有改变的检测概率。
英文摘要：
Several authors have claimed that the observable Hawking emission from a microscopic black hole is significantly modified by the formation of a photosphere or chromosphere around the black hole due to QED or QCD interactions between the emitted particles. Analyzing these models we identify a number of physical and geometrical effects which invalidate them. In all cases, we find that the observational signatures of a cosmic or Galactic background of black holes or an individual black hole remain essentially those of the standard Hawking model, with little change to the detection probability.
机构、总结、中文摘要均由AI分析而来，可能存在错误，请以论文正文为准。
