Black-hole relics in string gravity: last stages of Hawking evaporation
Black-hole relics in string gravity: last stages of Hawking evaporation
复制标题
弦引力中的黑洞遗迹：霍金蒸发的最后阶段
DOI：
10.1088/0264-9381/19/16/314
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发表时间：
2002
影响因子：
3.5
通讯作者：
Russia.
中科院分区：
文献类型：
--
作者：
S. Alexeyev;A. Barrau;G. Boudoul;O. Khovanskaya;M. Sazhin;Institut des Sciences Nucleaires;Grenoble;France.;Sternberg Astronomical Institute;Moscow;Russia.
黑洞蒸发的终点是现代物理学中一个非常有趣的问题。基于爱因斯坦-膨胀-高斯-博内特四维弦引力模型，我们证明黑洞不会消失，应该在蒸发过程结束时成为遗迹。研究了通过实验检测此类残余黑洞的可能性。如果它们真的存在，这些物体可能构成我们宇宙中非重子暗物质的很大一部分。
The endpoint of black-hole evaporation is a very intriguing problem of modern physics. Based on the Einstein-dilaton-Gauss–Bonnet four-dimensional string gravity model, we show that black holes do not disappear and should become relics at the end of the evaporation process. The possibility of experimental detection of such remnant black holes is investigated. If they really exist, these objects could form a considerable part of the non-baryonic dark matter in our universe.