THE PROPERTIS OF TIDAL FORCES IN THE KERR METRIC
The expression for the tidal forces of the two relativistic protons at a distance of the order of the Compton wavelength near a rotating black hole is found. The analysis shows that the tidal forces are dependent on the plane of incidence and sharply increase with increasing Lorentz factor.
Main Author: | A. M. Rasulova |
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Format: | Article |
Language: | English |
Published: |
Odessa I. I. Mechnykov National University
2016-06-01
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Series: | Odessa Astronomical Publications |
Subjects: | |
Online Access: | http://oap.onu.edu.ua/article/view/70609 |
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