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Test‐particle motion in superposed Weyl fields
Author(s) -
Semerák O.,
Žáček M.,
Zellerin T.
Publication year - 1999
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1046/j.1365-8711.1999.t01-1-02749.x
Subject(s) - physics , test particle , geodesic , event horizon , schwarzschild radius , gravitational field , motion (physics) , event (particle physics) , classical mechanics , schwarzschild metric , massive particle , space (punctuation) , field (mathematics) , equations of motion , einstein , particle (ecology) , gravitation , general relativity , astrophysics , dark matter , mathematical analysis , oceanography , geology , linguistics , philosophy , mathematics , pure mathematics
In a previous paper (Paper I), several superposed Weyl solutions of Einstein equations were investigated that might have some astrophysical relevance. We drew the gravitational field lines in the superposed space–times and the distortions of the Schwarzschild event horizon induced by the additional matter. Here we are concerned with the motion of free test particles in the same fields. In particular, the influence of the parameters (mass and location) of the additional sources on the positions of important circular equatorial geodesics is studied.

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