Brane-world cosmology and varying G
We consider a brane-world cosmological model coupled to a bulk scalar field. Since the brane tension turns out to be proportional to Newton's coupling G, in such a model a time variation of G naturally occurs. By resorting to available bounds on the variation of G, the parameters of the model a...
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| Formato: | Capítulo de libro |
| Lenguaje: | Inglés |
| Publicado: |
2010
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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 | 04760caa a22006617a 4500 | ||
|---|---|---|---|
| 001 | PAPER-7750 | ||
| 003 | AR-BaUEN | ||
| 005 | 20230518203731.0 | ||
| 008 | 190411s2010 xx ||||fo|||| 00| 0 eng|d | ||
| 024 | 7 | |2 scopus |a 2-s2.0-77955254293 | |
| 040 | |a Scopus |b spa |c AR-BaUEN |d AR-BaUEN | ||
| 030 | |a IMPAE | ||
| 100 | 1 | |a Amarilla, L. | |
| 245 | 1 | 0 | |a Brane-world cosmology and varying G |
| 260 | |c 2010 | ||
| 270 | 1 | 0 | |m Amarilla, L.; Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires, Ciudad Universitaria (1428), Pabellón 1, Buenos Aires, Argentina |
| 506 | |2 openaire |e Política editorial | ||
| 504 | |a Dirac, P.A.M., (1937) Nature, 139, p. 323 | ||
| 504 | |a Dirac, P.A.M., (1938) Proc. R. Soc. A, 165, p. 199 | ||
| 504 | |a Brans, C., Dicke, R.H., (1961) Phys. Rev., 124, p. 925 | ||
| 504 | |a Uzan, P.J., (2003) Rev. Mod. Phys., 75, p. 403 | ||
| 504 | |a Kaluza, T., (1921) Sitzungsber. Preuss. Akad. Wiss. Berlin (Math. Phys.), K1, p. 966 | ||
| 504 | |a Klein, O., (1926) Z. Phys., 37, p. 895 | ||
| 504 | |a Randall, L., Sundrum, R., (1999) Phys. Rev. Lett., 83, p. 4690 | ||
| 504 | |a Brax, Ph., Bruck De C.Van, Davis, A.C., (2004) Rep. Progr. Phys., 67, p. 2183 | ||
| 504 | |a Egyed, L., (1960) Geofis. Pura Appl., 45, p. 115 | ||
| 504 | |a McElhinny, M.W., Taylor, S.R., Stevenson, D.J., (1978) Nature, 271, p. 316 | ||
| 504 | |a Accetta, F.S., Krauss, L.M., Romanelli, P., (1990) Phys. Lett. B, 248, p. 146 | ||
| 504 | |a K. C. Chan and M. C. Chu, arXiv:astro-ph/0611851v2; Ishihara, H., (2001) Phys. Rev. Lett., 86, p. 381 | ||
| 504 | |a D. N. Spergel et al., arXiv:astro-ph/0603449v2; Csaki, C., Erlich, J., Grojean, Ch., Hollowood, T.J., (2000) Nucl. Phys. B, 584, p. 359 | ||
| 504 | |a Brax, P., Bruck De C.Van, Davis, A.C., (2001) J. High Energy Phys., 110, p. 026 | ||
| 504 | |a Mennim, A., Battye, R.A., (2001) Class. Quantum Grav., 18, p. 2171 | ||
| 504 | |a Bińetruy, P., Deffayet, C., Langlois, D., (2000) Nucl. Phys. B, 565, p. 269 | ||
| 504 | |a Brax, Ph., Davis, A.C., (2001) J. High Energy Phys., 105, p. 007 | ||
| 504 | |a E. G. Adelberger, B. R. Heckel, S. Hoedl, C. D. Hoyle, D. J. Kapner and A. Upadhye, arXiv:hep-ph/0611223v3; Copi, C.J., Davis, A.N., Krauss, L.M., (2004) Phys. Rev. Lett., 92, p. 171301 | ||
| 504 | |a Williams, J.G., Turyshev, S.G., Boggs, D.H., (2004) Phys. Rev. Lett., 93, p. 261101 | ||
| 504 | |a Benvenuto, O.G., Althaus, L.G., Torres, D.F., (1999) Mon. Not. R. Astron. Soc., 305, p. 905 | ||
| 504 | |a Brax, Ph., Davis, A.C., (2001) Phys. Lett. B, 497, p. 289 | ||
| 504 | |a Langlois, D., (2003) Progr. Theor. Phys. Suppl., 148, p. 181 | ||
| 504 | |a Maartens, R., (2004) Living Rev. Rel., 7, p. 7 | ||
| 504 | |a Langlois, D., (2006) Progr. Theor. Phys. Suppl., 163, p. 258 | ||
| 520 | 3 | |a We consider a brane-world cosmological model coupled to a bulk scalar field. Since the brane tension turns out to be proportional to Newton's coupling G, in such a model a time variation of G naturally occurs. By resorting to available bounds on the variation of G, the parameters of the model are constrained. The constraints coming from nucleosynthesis and CMB result to be the severest ones. © 2010 World Scientific Publishing Company. |l eng | |
| 536 | |a Detalles de la financiación: Consejo Nacional de Investigaciones Científicas y Técnicas | ||
| 536 | |a Detalles de la financiación: The authors are grateful to G. Giribet for useful discussions. The work of L. Amarilla was supported by CONICET. | ||
| 593 | |a Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires, Ciudad Universitaria (1428), Pabellón 1, Buenos Aires, Argentina | ||
| 593 | |a Facultad de Ciencias Astronómicas y Geofísicas, Universidad Nacional de la Plata, Paseo del Bosque S/N (1900), La Plata, Argentina | ||
| 690 | 1 | 0 | |a BRANE-WORLD COSMOLOGY |
| 690 | 1 | 0 | |a VARYING CONSTANTS |
| 700 | 1 | |a Vucetich, H. | |
| 773 | 0 | |d 2010 |g v. 25 |h pp. 3835-3856 |k n. 18-19 |p Int. J. Mod. Phys. A |x 0217751X |w (AR-BaUEN)CENRE-596 |t International Journal of Modern Physics A | |
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| 856 | 4 | 0 | |u https://doi.org/10.1142/S0217751X10049700 |y DOI |
| 856 | 4 | 0 | |u https://hdl.handle.net/20.500.12110/paper_0217751X_v25_n18-19_p3835_Amarilla |y Handle |
| 856 | 4 | 0 | |u https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0217751X_v25_n18-19_p3835_Amarilla |y Registro en la Biblioteca Digital |
| 961 | |a paper_0217751X_v25_n18-19_p3835_Amarilla |b paper |c PE | ||
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| 963 | |a VARI | ||
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