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.

Bibliographic Details
Main Author: A. M. Rasulova
Format: Article
Language:English
Published: Odessa I. I. Mechnykov National University 2016-06-01
Series:Odessa Astronomical Publications
Subjects:
Online Access:http://oap.onu.edu.ua/article/view/70609