On the Final State of Black Holes ()
Abstract
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.
Share and Cite:
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.
References
|
[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.
https://doi.org/10.4236/jmp.2019.106047
|