Artículo
Deffayet, C.; Harari, D.; Uzan, J.-P.; Zaldarriaga, M. "Dimming of supernovae by photon-pseudoscalar conversion and the intergalactic plasma" (2002) Physical Review D. 66(4)
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Abstract:
It has been suggested recently that the observed dimming of distant type la supernovae may be a consequence of mixing of the photons with very light axions. We point out that the effect of the plasma, in which the photons are propagating, must be taken into account. This effect changes the oscillation probability and renders the dimming frequency dependent, contrary to observations. One may hope to accommodate the data by averaging the oscillations over many different coherence domains. We estimate the effect of coherence loss, either due to the inhomogeneities of the magnetic field or of the intergalactic plasma. These estimates indicate that the achromaticity problem can be resolved only with very specific, and probably unrealistic, properties of the intergalactic medium. ©2002 The American Physical Society.
Registro:
| Documento: | Artículo |
| Título: | Dimming of supernovae by photon-pseudoscalar conversion and the intergalactic plasma |
| Autor: | Deffayet, C.; Harari, D.; Uzan, J.-P.; Zaldarriaga, M. |
| Filiación: | NYU Department of Physics, 4 Washington Place, New York, NY 10003, United States Departamento de Física, FCEyN-Universidad de Buenos Aires, Ciudad Universitaria-Pab. 1, 1428 Buenos Aires, Argentina Laboratoire de Physique Thréorique, UMR 8627 du CNRS, Bâtiment 210, F-91405 Orsay Cedex, France Institut d'Astrophysique de Paris, 98bis Bd. Arago, 75014 Paris, France Institute for Advanced Study, Einstein Drive, Princeton, NJ 08540, United States |
| Palabras clave: | article; calculation; cosmos; light; magnetic field; mathematical analysis; oscillation; photon; probability |
| Año: | 2002 |
| Volumen: | 66 |
| Número: | 4 |
| DOI: | http://dx.doi.org/10.1103/PhysRevD.66.043517 |
| Título revista: | Physical Review D |
| Título revista abreviado: | - |
| ISSN: | 05562821 |
| Registro: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_05562821_v66_n4_p_Deffayet |
Referencias:
- Raffelt, G.G., Stodolsky, L., (1988) Phys. Rev. D, 37, p. 1237
- Sikivie, P., (1983) Phys. Rev. Lett., 51, p. 1415
- Sikivie, P., (1984) Phys. Rev. Lett., 52, p. 695
- Morris, D.E., (1986) Phys. Rev. D, 34, p. 843
- Gertsenshtein, M.E., (1962) Sov. Phys. JETP, 14, p. 84
- Zel'dovich, Ya.B., Novikov, I.D., The structure and evolution of the universe (1983) Relativistic Astrophysics Vol. 2, , Chicago University Press, Chicago
- Van Bibber, K., (1989) Phys. Rev. D, 39, p. 2089
- Hagmann, C., (1998) Phys. Rev. Lett., 80, p. 2043
- Kim, J.E., (1998) Phys. Rev. D, 58, p. 055006
- Sikivie, P., (1998) Phys. Lett. B, 432, p. 139
- Georgi, H., Ginsparg, P., Glashow, S.L., (1983) Nature (London), 306, p. 765
- Raffelt, G.G., Proceedings of Neutrino '98, , Japan, edited by Y. Suzuki and Y. Totsuka
- (1999) Nucl. Phys. B (Proc. Suppl.), 77, p. 456
- Perlmutter, S., (1999) Astrophys. J., 517, p. 565
- Riess, A.G., (1998) Astrophys. J., 116, p. 1009
- Riess, A.G., (2001) Astrophys. J., 560, p. 49
- Csaki, C., Kaloper, N., Terning, J., (2002) Phys. Rev. Lett., 88, p. 161302
- Erlich, J., Grojean, C., (2002) Phys. Rev. D, 65, p. 123510
- Harari, D., Sikivie, P., (1992) Phys. Lett. B, 289, p. 67
- Carlson, E., Garretson, W., (1994) Phys. Rev. Lett., 336, p. 431
- Grifols, J.A., Masso, E., Toldra, R., (1996) Phys. Rev. Lett., 77, p. 2372
- Brockway, J.W., Carlson, E.D., Raffelt, G.G., (1996) Phys. Lett. B, 383, p. 439
- Magueijo, J.C.R., (1994) Phys. Rev. D, 49, p. 671
- Chen, P., (1995) Phys. Rev. Lett., 74, p. 634
- Cillis, A.N., Harari, D., (1996) Phys. Rev. D, 54, p. 4757
- Deffayet, C., Uzan, J.-P., (2000) Phys. Rev. D, 62, p. 063507
- Adler, S.L., (1971) Ann. Phys, 67, p. 599. , N.Y
- Heisenberg, W., Euler, H., (1936) Z. Phys., 88, p. 714
- Itzykson, C., Zuber, J.-B., (1980) Quantum Field Theory, , McGraw-Hill, New York
- Landau, L.D., Lifschitz, E.M., (1960) Electrodynamics of Continuous Media, , Mir, Moscow
- (1972) American Institute of Physics Handbook, 3rd Ed., , edited by D.E. Gray (McGraw-Hill, New York)
- Gunri, J.E., Peterson, B.A., (1965) Astrophys. J., 142, p. 1633
- Peebles, P.J.E., (1993) Principles of Physical Cosmology, , Princeton University Press, Princeton, NJ
- Furlanetto, S.R., Loeb, A., (2001) Astrophys. J., 556, p. 619
- Kronberg, P., (1994) Rep. Prog. Phys., 57, p. 325
- Farrar, G.R., Piran, T., (2000) Phys. Rev. Lett., 84, p. 3527
- Dave, R., (2001) Astrophys. J., 552, p. 473
- Csaki, C., Kaloper, N., Terning, J., (2002) Phys. Lett. B, 535, p. 33
Citas:
---------- APA ----------
Deffayet, C., Harari, D., Uzan, J.-P. & Zaldarriaga, M. (2002) . Dimming of supernovae by photon-pseudoscalar conversion and the intergalactic plasma. Physical Review D, 66(4).http://dx.doi.org/10.1103/PhysRevD.66.043517
---------- CHICAGO ----------
Deffayet, C., Harari, D., Uzan, J.-P., Zaldarriaga, M. "Dimming of supernovae by photon-pseudoscalar conversion and the intergalactic plasma" . Physical Review D 66, no. 4 (2002).http://dx.doi.org/10.1103/PhysRevD.66.043517
---------- MLA ----------
Deffayet, C., Harari, D., Uzan, J.-P., Zaldarriaga, M. "Dimming of supernovae by photon-pseudoscalar conversion and the intergalactic plasma" . Physical Review D, vol. 66, no. 4, 2002.http://dx.doi.org/10.1103/PhysRevD.66.043517
---------- VANCOUVER ----------
Deffayet, C., Harari, D., Uzan, J.-P., Zaldarriaga, M. Dimming of supernovae by photon-pseudoscalar conversion and the intergalactic plasma. -. 2002;66(4).http://dx.doi.org/10.1103/PhysRevD.66.043517
