Astronomy and Astrophysics – Astrophysics
Scientific paper
2001-04-03
Hadronic J.Suppl. 16 (2001) 125-150
Astronomy and Astrophysics
Astrophysics
22 pages, 0 figures
Scientific paper
Although the extraordinary weakness of gravity makes it by far the weakest of the interactions, viewing little black holes (LBH) as a class of elementary particles puts them in a league with hadrons as strongly interacting particles. They interact strongly both in the subatomic and macroscopic realms. An enormous universal gravitational attractive force ~ 10^43 /B 2 Newtons acts between identical black holes for any mass M >> M Planck at a center-to-center separation of 2 BR H (B > 1). For M ~ M Planck, there is a comparably large repulsive force. The Hawking model of LBH radiation permits a luminosity from a single LBH comparable to that of the entire universe, whereas this luminosity is greatly attenuated in the Rabinowitz model. In interacting with each other, and with large macroscopic bodies such as stars, neutron stars, and planets, LBH can exhibit strong interactions with large-scale manifestations. Although previously dismissed, an LBH is a potential candidate in accounting for the 1908 devastation of Tungus Siberia, since important LBH interactions were overlooked. LBH passing through neutron star pulsars are capable of causing a sudden change in frequency which may not be fully accounted for by other theories. The existence of black holes is also discussed.
No associations
LandOfFree
Macroscopic Hadronic Little Black Hole Interactions does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Macroscopic Hadronic Little Black Hole Interactions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Macroscopic Hadronic Little Black Hole Interactions will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-173186