On the post-Newtonian approximation of the Einstein-Cartan-Sciama-Kibble theory
The post-Newtonian approximation of the Einstein-Cartan-Sciama-Kibble or ECSK theory is developed. It is used to obtain a drastic reduction on the density of the source needed to detect the spin. It is also proved that if we know the structure of the source, up to order -v, the spin can be detected,...
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| Otros Autores: | , |
| Formato: | Capítulo de libro |
| Lenguaje: | Inglés |
| Publicado: |
Kluwer Academic Publishers-Plenum Publishers
1985
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| Acceso en línea: | Registro en Scopus DOI Handle Registro en la Biblioteca Digital |
| Aporte de: | Registro referencial: Solicitar el recurso aquí |
| LEADER | 03058caa a22004217a 4500 | ||
|---|---|---|---|
| 001 | PAPER-1065 | ||
| 003 | AR-BaUEN | ||
| 005 | 20241205092041.0 | ||
| 008 | 190411s1985 xx ||||fo|||| 00| 0 eng|d | ||
| 024 | 7 | |2 scopus |a 2-s2.0-34250117303 | |
| 040 | |a Scopus |b spa |c AR-BaUEN |d AR-BaUEN | ||
| 100 | 1 | |a Castagnino, Mario Alberto | |
| 245 | 1 | 3 | |a On the post-Newtonian approximation of the Einstein-Cartan-Sciama-Kibble theory |
| 260 | |b Kluwer Academic Publishers-Plenum Publishers |c 1985 | ||
| 270 | 1 | 0 | |m Castagnino, M.; Instituto de Fisica de Rosario (CONICET-UNR), Avenida Pellegrini 250, Rosario, 2000, Argentina |
| 504 | |a Smalley, L., (1980) Phys. Rev. D, 21, p. 328 | ||
| 504 | |a Schweizer, M., Straumann, N., Wipf, A., (1980) Gen. Rel. Grav., 12, p. 951 | ||
| 504 | |a Will, C.M., (1981) Theory and Experiment in Gravitational Physics, p. 151. , Cambridge University Press, Cambridge, England | ||
| 504 | |a Hehl, F.W., von der Heyde, P., Kerlick, G.A., Nester, G.M., (1976) Rev. Mod. Phys., 48 (3), p. 393 | ||
| 504 | |a Weinberg, S., (1972) Gravitation and Cosmology, pp. 211-223. , Wiley, New York | ||
| 504 | |a Ray, J.R., Smalley, L.L., (1983) Phys. Rev. D, 27, p. 1383 | ||
| 504 | |a Yasskin, P.B., Stoeger, W.R., (1979) Phys. Rev. D, 21, p. 2081 | ||
| 506 | |2 openaire |e Política editorial | ||
| 520 | 3 | |a The post-Newtonian approximation of the Einstein-Cartan-Sciama-Kibble or ECSK theory is developed. It is used to obtain a drastic reduction on the density of the source needed to detect the spin. It is also proved that if we know the structure of the source, up to order -v, the spin can be detected, and if we know it up to order -v2 the theory can be verified. © 1985 Plenum Publishing Corporation. |l eng | |
| 593 | |a Instituto de Fisica de Rosario (CONICET-UNR), Avenida Pellegrini 250, Rosario, 2000, Argentina | ||
| 593 | |a Instituto de Astronomía y Física del Espacio, (CONICET), Sucursal 28, Buenos Aires, C. C. 67, Argentina | ||
| 593 | |a Departamento de Matemática, Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires, Pabellón I, Ciudad Universitaria, Buenos Aires, Argentina | ||
| 700 | 1 | |a Levinas, M.L. | |
| 700 | 1 | |a Umerez, N. | |
| 773 | 0 | |d Kluwer Academic Publishers-Plenum Publishers, 1985 |g v. 17 |h pp. 683-693 |k n. 7 |p Gen Relat Gravit |x 00017701 |w (AR-BaUEN)CENRE-369 |t General Relativity and Gravitation | |
| 856 | 4 | 1 | |u https://www.scopus.com/inward/record.uri?eid=2-s2.0-34250117303&doi=10.1007%2fBF00763029&partnerID=40&md5=0417ea0e40398ba4e1b971112a4907a3 |y Registro en Scopus |
| 856 | 4 | 0 | |u https://doi.org/10.1007/BF00763029 |y DOI |
| 856 | 4 | 0 | |u https://hdl.handle.net/20.500.12110/paper_00017701_v17_n7_p683_Castagnino |y Handle |
| 856 | 4 | 0 | |u https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00017701_v17_n7_p683_Castagnino |y Registro en la Biblioteca Digital |
| 961 | |a paper_00017701_v17_n7_p683_Castagnino |b paper |c PE | ||
| 962 | |a info:eu-repo/semantics/article |a info:ar-repo/semantics/artículo |b info:eu-repo/semantics/publishedVersion | ||
| 963 | |a VARI | ||
| 999 | |c 62018 | ||