On the Final State of Black Holes

Abstract Full-Text HTML Download Download as PDF (Size:395KB) PP. 725-728
DOI: 10.4236/jmp.2019.107052    293 Downloads   563 Views  
Author(s)    Leave a comment


The final state of a black hole and its force balance is considered, in the limit where all available energy is radiated away and all matter remains in the lowest form of Zero Point Energy (ZPE). In conventional theory without the concept of ZPE, the gravitational contraction would transfer the system into a mass point, being questionable from the theoretical point of view. But the inclusion of ZPE makes a force balance possible, resulting in a finite characteristic radius of a black hole mass distribution. This radius is of the same order as that of the so-called Schwarzschild radius, but is not related to the physics of the latter, which is due to particle trapping in the gravitational field.

Cite this paper

Lehnert, B. (2019) On the Final State of Black Holes. Journal of Modern Physics, 10, 725-728. doi: 10.4236/jmp.2019.107052.

Conflicts of Interest

The author declares no conflicts of interest regarding the publication of this paper.


[1] Schwarzschild, K. (1916) Sitzungsber.Preuss.Akad.Wiss.Berlin (Math.Phys.), 189-196.
[2] Misner, C.W., Thorne, K.S. and Wheeler, J.A. (1973) Gravitation. Chap. 33, W.H. Freeman and Co., San Francisco and Reading.
[3] Planck, M. (1900) Verh. Dtsch Phys. Ges., 2, 237.
[4] Bergmann, P.G. (1942) Introduction to the Theory of Relativity. Chap. X, Prentice Hall, Inc., New York.
[5] Lehnert, B. (2019) Journal of Modern Physics, 10, 663-672.

comments powered by Disqus

Copyright © 2020 by authors and Scientific Research Publishing Inc.

Creative Commons License

This work and the related PDF file are licensed under a Creative Commons Attribution 4.0 International License.