THE PROPERTIS OF TIDAL FORCES IN THE KERR METRIC

Автор(и)

  • A. M. Rasulova The Herzen University; Institute of Limnology, RAS, Російська Федерація

DOI:

https://doi.org/10.18524/1810-4215.2015.28.70609

Ключові слова:

General relativity - geodesic deviation, Black hole - Kerr metric, Tidal forces

Анотація

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.

Посилання

Levi-Civita T.: 1926, The absolute differential calculus, London: Blackie and Son.

Synge J.L.: 1934, Element Ann. Math., 35, 705.

Synge J.L.: 1960, Relativity: The General Theory, North-Holland, Amsterdam; Interscience, NewYork.

Shapiro S.L., Teukolsky S.A.: 1983, Black Holes, White Dwarfs and Neutron Stars, Cornell Univ., Ithaca, New York.

Chandrasekhar S.: 1983, The Mathematical Theory of Black Holes, Oxford Univ. Press, Oxford.

Misner C.W., Thorne K.S., Wheeler J.A.: 1973, Gravitation, Freeman and Company Limited.

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Опубліковано

2016-06-10

Номер

Розділ

Космологія, гравітація, фізика астрочастинок, фізика високих енергій