Conversion of Goldstone bosons into gravitons in anisotropic cosmology
The gravitational chiral anomaly makes possible the conversion of a Goldstone boson into a graviton in a background gravitational field. We show that the interaction Lagrangian for this process does not vanish if and only if the background metric has a nonvanishing Weyl tensor, i.e., if it is not co...
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| Formato: | Capítulo de libro |
| Lenguaje: | Inglés |
| Publicado: |
1990
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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 | 05230caa a22007337a 4500 | ||
|---|---|---|---|
| 001 | PAPER-511 | ||
| 003 | AR-BaUEN | ||
| 005 | 20250505095211.0 | ||
| 008 | 190411s1990 xx ||||fo|||| 00| 0 eng|d | ||
| 024 | 7 | |2 scopus |a 2-s2.0-35949009957 | |
| 040 | |a Scopus |b spa |c AR-BaUEN |d AR-BaUEN | ||
| 100 | 1 | |a Harari, Diego Darío | |
| 245 | 1 | 0 | |a Conversion of Goldstone bosons into gravitons in anisotropic cosmology |
| 260 | |c 1990 | ||
| 270 | 1 | 0 | |m Harari, D.D.; Instituto de Astronomía Y Física del Espacio, Casilla de Correo 67, Sucursal 28, 1428 Buenos Aires, Argentina |
| 504 | |a Adler, S., (1969) Phys. Rev., 177, p. 2426 | ||
| 504 | |a Bell, J., Jackiw, R., (1969) Nuovo Cimento, 60 A, p. 47 | ||
| 504 | |a Delbourgo, R., Salam, A., (1972) Phys. Lett., 40 B, p. 381 | ||
| 504 | |a Eguchi, T., Freund, P., (1976) Phys. Rev. Lett., 37, p. 1251 | ||
| 504 | |a Alvarez-Gaumé, L., Witten, E., (1983) Nucl. Phys., 234 B, p. 269 | ||
| 504 | |a Parker, L., (1989) Int. J. Theor. Phys., 28, p. 1163 | ||
| 504 | |a Perry, M.J., (1978) Nucl. Phys., 143 B, p. 114 | ||
| 504 | |a Hawking, S.W., Pope, C.N., (1978) Nucl. Phys., 146 B, p. 381 | ||
| 504 | |a Eguchi, T., Gilkey, P.B., Hanson, A.J., Gravitation, gauge theories and differential geometry (1980) Physics Reports, 66, p. 213 | ||
| 504 | |a Green, M.S., Schwarz, J.H., Witten, E., (1987) Superstring Theory, , Cambridge University Press, London | ||
| 504 | |a Peccei, R.D., Quinn, H., (1977) Phys. Rev. Lett., 38, p. 1440 | ||
| 504 | |a Weinberg, S., (1978) Phys. Rev. Lett., 40, p. 223 | ||
| 504 | |a Weinberg, S., (1978) Phys. Rev. Lett., 40, p. 279. , F. Wilczek | ||
| 504 | |a Dicus, D.A., Kolb, E.W., Teplitz, V.L., Wagoner, R.V., (1978) Phys. Rev. D, 18, p. 1829 | ||
| 504 | |a Abbott, L.F., Sikivie, P., (1983) Phys. Lett., 120 B, p. 133 | ||
| 504 | |a Dine, M., Fischler, W., (1983) Phys. Lett., 120 B, p. 137 | ||
| 504 | |a Preskill, J., Wise, M.B., Wilczek, F., (1983) Phys. Lett., 120 B, p. 127 | ||
| 504 | |a Sikivie, P., (1983) Phys. Rev. Lett., 51, p. 1415 | ||
| 504 | |a Wuensch, W.U., (1989) Phys. Rev. D, 40, p. 3153 | ||
| 504 | |a Maiani, L., Petronzio, R., Zavattini, E., (1986) Phys. Lett. B, 175, p. 359 | ||
| 504 | |a Holman, R., Wang, Y., (1989) Phys. Rev. D, 40, p. 3204 | ||
| 504 | |a MacCallum, M.A.H., (1979) General Relativity: An Einstein Centenary Survey, , edited by, S. W. Hawking, W. Israel, Cambridge University Press, London | ||
| 504 | |a Landau, L., Lifchitz, E., (1970) Classical Field Theory, , Pergamon, New York | ||
| 504 | |a Birrell, N.D., Davies, P.C.W., (1982) Quantum Fields in Curved Space, , Cambridge University Press, London | ||
| 504 | |a Parker, L., Fulling, S.A., (1977) Phys. Rev. D, 9, p. 341 | ||
| 504 | |a Ford, L.H., Parker, L., (1977) Phys. Rev. D, 16, p. 1601 | ||
| 504 | |a Hu, B.L., (1978) Phys. Rev. D, 18, p. 969 | ||
| 504 | |a Sikivie, P., (1988) Phys. Rev. Lett., 61, p. 783 | ||
| 504 | |a Hawking, S.W., Ellis, G.F.R., (1973) The Large Scale Structure of Space-Time, , Cambridge University Press, London | ||
| 504 | |a Misner, C.W., The Isotropy of the Universe (1968) The Astrophysical Journal, 151, p. 431 | ||
| 504 | |a Witten, E., (1985) Phys. Lett., 153 B, p. 243 | ||
| 504 | |a Davis, R.L., (1985) Phys. Rev. D, 32, p. 3172 | ||
| 504 | |a Vilenkin, A., Vachaspati, T., (1987) Phys. Rev. D, 35, p. 1138 | ||
| 504 | |a Harari, D., Sikivie, P., (1987) Phys. Lett. B, 195, p. 361 | ||
| 504 | |a Davis, R.L., Shellard, E.P.S., (1989), MIT | ||
| 506 | |2 openaire |e Política editorial | ||
| 520 | 3 | |a The gravitational chiral anomaly makes possible the conversion of a Goldstone boson into a graviton in a background gravitational field. We show that the interaction Lagrangian for this process does not vanish if and only if the background metric has a nonvanishing Weyl tensor, i.e., if it is not conformally flat. No conversion takes place in an isotropic expanding universe. We evaluate the probability for the conversion of Goldstone bosons into gravitons in Bianchi type-I background metrics, the simplest anisotropic cosmological backgrounds. © 1990 The American Physical Society. |l eng | |
| 593 | |a Instituto de Astronomía Y Física del Espacio, Casilla de Correo 67, Sucursal 28, 1428 Buenos Aires, Argentina | ||
| 593 | |a Departamento de Física, Facultad de Ciencias Exactas Y Naturales, Ciudad Universitaria, Pab. I, 1428 Buenos Aires, Argentina | ||
| 700 | 1 | |a Mazzitelli, F.D. | |
| 773 | 0 | |d 1990 |g v. 42 |h pp. 2632-2637 |k n. 8 |x 05562821 |w (AR-BaUEN)CENRE-394 |t Physical Review D | |
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| 856 | 4 | 0 | |u https://doi.org/10.1103/PhysRevD.42.2632 |y DOI |
| 856 | 4 | 0 | |u https://hdl.handle.net/20.500.12110/paper_05562821_v42_n8_p2632_Harari |y Handle |
| 856 | 4 | 0 | |u https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_05562821_v42_n8_p2632_Harari |y Registro en la Biblioteca Digital |
| 961 | |a paper_05562821_v42_n8_p2632_Harari |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 61464 | ||