A Doppler-looking redshift observed in the labs; application to quasars

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dc.creatorMoret-Bailly, Jacques
dc.date1998-10-29
dc.date.accessioned2026-07-07T02:28:48Z
dc.date.available2026-07-07T02:28:48Z
dc.descriptionIt is known since 1968 that the interaction of a pulse of light with matter redshifts the spectrum; the theory is clarified, to obtain the conditions for which, with incoherent light, one gets a redshift similar to a Doppler shift rather than Raman lines. The explanation of the appearance of the same absorption line with various z becomes trivial, requiring. only a static halo and a static magnetic field.
dc.description4 pages
dc.identifierhttps://arxiv.org/abs/astro-ph/9810473
dc.identifierhttp://arxiv.org/abs/astro-ph/9810473
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13212
dc.subjectAstrophysics
dc.titleA Doppler-looking redshift observed in the labs; application to quasars
dc.typetext

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