期刊论文详细信息
Symmetry
Unbounded Energy Collisions inside and outside Black Holes
Pawel Gusin1  Andrzej Radosz1  Andy T. Augousti2  Romuald J. Ściborski3 
[1] Department of Quantum Technologies, Wroclaw University of Science and Technology, 52-213 Wroclaw, Poland;Faculty of Science, Engineering and Computing, Kingston University London, London SW15 3DW, UK;School of Health Sciences, The European-African Cluster for Public Health and Biotechnology, Jaramogi Oginga Odinga University of Science and Technology, P.O. Box 210, Bondo 40601, Kenya;
关键词: Penrose mechanism;    unbounded energy release;    Schwarzschild;    Reissner–Nordström and Kerr black holes;    event horizon;   
DOI  :  10.3390/sym14061242
来源: DOAJ
【 摘 要 】

The possibility of on-horizon collisions of unbounded energy in the case of an extreme Kerr black hole is known as the BSW effect. It is also a widely accepted point of view that the energy collision of two identical particles of mass m near the horizon of a Schwarzschild black hole is limited to a value of 25 m. We show that there are two possible scenarios for unbounded energy collisions both for the exterior and for the interior of spherically symmetric black holes. Similar scenarios are found for axially symmetric black holes. It is shown that divergent (infinite) energy on-(inner)horizon collisions are excluded due to the anisotropic character of the dynamics of black hole interiors.

【 授权许可】

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