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Zamorano, P. ; Gambi Fernández, José María ; Romero Pérez, Mª Pilar ; García del Pino, M.L. | Società Italiana di Fisica | 2002-04The orbital motion about a central symmetric massive body appears very well described in terms of polar Gaussian coordinates because these are the only coordinates that can be materialized by a proper reference frame with origin at the centre of[...]texto impreso
Gambi, J.M. ; Romero Pérez, Mª Pilar ; Zamorano, P. ; García del Pino, M.L. | Società Italiana di Fisica | 2000-02Conditions for the compatibility of the exterior metric of a spherically symmetric object with the field equations for the empty space and equations of motion and of trajectories for test particles, written in polar Gaussian and Fermi coordinate[...]texto impreso
Gambi, J.M. ; Zamorano, P. ; Romero Pérez, Mª Pilar ; García del Pino, M.L. | Kluwer Academic | 1996The orbital motion of test particles about a central body at rest is described in terms of a coordinate system that, unlike the usual coordinates, can be materialized by a proper (Fermi) reference frame with origin located at the body's centre w[...]
