Dimming of supernovae by photon-pseudoscalar conversion and the intergalactic plasma

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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 oscillati...

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Autor principal: Deffayet, C.
Otros Autores: Harari, Diego Darío, Uzan, J.-P, Zaldarriaga, M.
Formato: Capítulo de libro
Lenguaje:Inglés
Publicado: 2002
Acceso en línea:Registro en Scopus
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Biblioteca Central Dr. Luis F. Leloir (FCEN) de Universidad de Buenos Aires
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100 1 |a Deffayet, C. 
245 1 0 |a Dimming of supernovae by photon-pseudoscalar conversion and the intergalactic plasma 
260 |c 2002 
270 1 0 |m Deffayet, C.; NYU Department of Physics, 4 Washington Place, New York, NY 10003, United States; email: cjd2@physics.nyu.edu 
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506 |2 openaire  |e Política editorial 
520 3 |a 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.  |l eng 
593 |a NYU Department of Physics, 4 Washington Place, New York, NY 10003, United States 
593 |a Departamento de Física, FCEyN-Universidad de Buenos Aires, Ciudad Universitaria-Pab. 1, 1428 Buenos Aires, Argentina 
593 |a Laboratoire de Physique Thréorique, UMR 8627 du CNRS, Bâtiment 210, F-91405 Orsay Cedex, France 
593 |a Institut d'Astrophysique de Paris, 98bis Bd. Arago, 75014 Paris, France 
593 |a Institute for Advanced Study, Einstein Drive, Princeton, NJ 08540, United States 
690 1 0 |a ARTICLE 
690 1 0 |a CALCULATION 
690 1 0 |a COSMOS 
690 1 0 |a LIGHT 
690 1 0 |a MAGNETIC FIELD 
690 1 0 |a MATHEMATICAL ANALYSIS 
690 1 0 |a OSCILLATION 
690 1 0 |a PHOTON 
690 1 0 |a PROBABILITY 
700 1 |a Harari, Diego Darío 
700 1 |a Uzan, J.-P. 
700 1 |a Zaldarriaga, M. 
773 0 |d 2002  |g v. 66  |k n. 4  |p -  |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.66.043517  |y DOI 
856 4 0 |u https://hdl.handle.net/20.500.12110/paper_05562821_v66_n4_p_Deffayet  |y Handle 
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963 |a VARI 
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