On the post-Newtonian approximation of the ECSK theory II

We complete the PNA program for the ECSK theory. We find the general post-Newtonian equations of motion for the source. The different components of the complete affine connection, the torsion, and the energy-momentum tensor, as well as the conservation theorems of the theory, are developed for the c...

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Autor principal: Castagnino, Mario Alberto
Otros Autores: Levinas, M.L
Formato: Capítulo de libro
Lenguaje:Inglés
Publicado: Kluwer Academic Publishers-Plenum Publishers 1987
Acceso en línea:Registro en Scopus
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100 1 |a Castagnino, Mario Alberto 
245 1 3 |a On the post-Newtonian approximation of the ECSK theory II 
260 |b Kluwer Academic Publishers-Plenum Publishers  |c 1987 
270 1 0 |m Castagnino, M.A.; Instituto de Fisica de Rosario (CONICET-UNR), Avenida Pellegrini 250, Rosario, 2000, Argentina 
504 |a Castagnino, M., Levinas, M., Umerez, N., (1985) Gen. Rel. Grav., 17, p. 683 
504 |a Hehl, F., von der Heyde, P., Kerlick, G., Nester, G., (1976) Rev. Mod. Phys., 48 (3), p. 393 
504 |a Weinberg, S., (1972) Gravitation and Cosmology, , John Wiley & Sons, New York 
504 |a Misner, C., Thorne, K., Wheeler, S., (1973) Gravitation, , W. H. Freeman and Co., San Francisco 
504 |a Will, C., (1981) Theory and Experiment in Gravitational Physics, , Cambridge University Press, Cambridge 
504 |a Ray, J., Smalley, L., (1983) Phys. Rev., 27 D, p. 1383 
504 |a De Ritis, R., Lavorgna, M., Platania, G., Stornaiolo, C., (1985) Phys. Rev., 31 D, p. 1854 
504 |a Tsamparlis, M., (1981) Phys. Rev., 24 D, p. 1451 
504 |a Castagnino, M., Domenech, G., Levinas, M., Umerez, N., (1986) Phys. Lett., 179 B (1-2), p. 83 
506 |2 openaire  |e Política editorial 
520 3 |a We complete the PNA program for the ECSK theory. We find the general post-Newtonian equations of motion for the source. The different components of the complete affine connection, the torsion, and the energy-momentum tensor, as well as the conservation theorems of the theory, are developed for the case of an ideal fluid with spin in order to find the post-Newtonian trajectories of test particles exterior to the sources distribution. The main results are compared with the corresponding ones of general relativity. © 1987 Plenum Publishing Corporation.  |l eng 
593 |a Instituto de Fisica de Rosario (CONICET-UNR), Avenida Pellegrini 250, Rosario, 2000, Argentina 
593 |a Instituto de Astronomia y Fisica del Espacio (CONICET), C.C.67, Sucursal 28, Buenos Aires, Argentina 
593 |a Departamento de Matematica, Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires, Pabellon 1, Ciudad Universitaria, Buenos Aires, Argentina 
700 1 |a Levinas, M.L. 
773 0 |d Kluwer Academic Publishers-Plenum Publishers, 1987  |g v. 19  |h pp. 545-562  |k n. 6  |p Gen Relat Gravit  |x 00017701  |w (AR-BaUEN)CENRE-369  |t General Relativity and Gravitation 
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