Photon motion in the ECSK theory

Working within the scheme of the Einstein-Cartan-Sciama-Kibble Theory (ECSK) we find the trajectory of the photon up to its third order with respect to the velocity of slow motion sources. For the general case, discrepancies from the predictions of General Relativity (GR) are found. We apply the res...

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Autor principal: Castagnino, Mario Alberto
Otros Autores: Levinas, M.
Formato: Capítulo de libro
Lenguaje:Inglés
Publicado: Kluwer Academic Publishers-Plenum Publishers 1988
Acceso en línea:Registro en Scopus
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100 1 |a Castagnino, Mario Alberto 
245 1 0 |a Photon motion in the ECSK theory 
260 |b Kluwer Academic Publishers-Plenum Publishers  |c 1988 
270 1 0 |m Castagnino, M.; Institute de Astronomía y Física del Espacio (CONICET), C.C. 67, Suc. 28, Buenos Aires, 1428, Argentina 
504 |a Castagnino, M., Levinas, M., Umerez, N., (1985) Gen. Rel. Grav., 17, p. 683 
504 |a Castagnino, M., Levinas, M., (1987) Gen. Rel. Grav., 19, p. 563 
504 |a Domenech, G., Levinas, M., Umerez, N., (1988) Proceedings of the VIth Latin-American Simposium on Relativity and Gravity, Rio de Janeiro, Brasil, , M., Novello, World Scientific, Singapore 
504 |a Misner, C., Thorne, K., Wheeler, J., (1973) Gravitation, , Freeman and Co., San Francisco 
504 |a Will, C., (1981) Theory and Experiment in Gravitational Physics, , Cambridge University Press, Cambridge 
504 |a Weinberg, S., (1972) Gravitation and Cosmology, , John Wiley & Sons, New York 
504 |a Ray, J., Smalley, L., (1982) Phys. Rev. Lett., 49, p. 15 
504 |a De Ritis, R., Lavorgna, M., Platania, G., Stornaiolo, C., (1983) Phys. Rev. D, 28, p. 713 
506 |2 openaire  |e Política editorial 
520 3 |a Working within the scheme of the Einstein-Cartan-Sciama-Kibble Theory (ECSK) we find the trajectory of the photon up to its third order with respect to the velocity of slow motion sources. For the general case, discrepancies from the predictions of General Relativity (GR) are found. We apply the results to a model of polarized spin and find that in this particular case ECSK and GR theories coincide. We also perform a multipole expansion of the gravitational potentials in order to find the motion of photons far away from localized sources. © 1988 Plenum Publishing Corporation.  |l eng 
593 |a Institute de Astronomía y Física del Espacio (CONICET), C.C. 67, Suc. 28, Buenos Aires, 1428, Argentina 
593 |a Instituto de Física de Rosario (CONICET-UNR), Avenida Pellegrini 250, Rosario, 2000, Argentina 
593 |a Departamento de Matemática, Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires, Pab. 1, Cdad. Universitaria, Buenos Aires, Argentina 
593 |a Comisión de Investigaciones Científicas (CIC), Calle 526 e/10 y 11, La Plata, 1900, Argentina 
700 1 |a Levinas, M. 
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