Computation of the spectra of the quasars
| dc.creator | Moret-Bailly, Jacques | |
| dc.date | 2003-08-25 | |
| dc.date | 2003-08-28 | |
| dc.date.accessioned | 2026-07-07T02:09:18Z | |
| dc.date.available | 2026-07-07T02:09:18Z | |
| dc.description | The repartition of redshifts of the lines observed in the spectra of the quasars is generally considered as stochastic, but several authors showed that the difference of two redshifts is the product of an integer by a basic redshift zf = 0.062. This property results from a coherent Raman effect during the propagation of the incoherent light in a halo of atomic hydrogen, without any jet of gas, or dark matter. The coherence forbids a blur of the images or of the spectra. The computation of zf does not require any new spectroscopic parameter. The non-linearity of the combination of Lyman absorptions and coherent Raman effect explains both the observed positions of the spectral lines and their high contrast. | |
| dc.description | Improvement of astro-ph/0307140 | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0308425 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0308425 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/6382 | |
| dc.subject | Astrophysics | |
| dc.title | Computation of the spectra of the quasars | |
| dc.type | text |