Theoretical spectroscopy of quasars within Karlsson's law
Jacques Moret-Bailly

TL;DR
This paper presents a theoretical analysis of quasar spectra based on Karlsson's law, proposing that redshifts result from interactions of light with hydrogen atoms, simplifying cosmological models.
Contribution
It introduces a new theoretical framework linking quasar spectral lines to hydrogen interactions and Karlsson's law, challenging standard cosmological redshift explanations.
Findings
Spectral lines result from hydrogen interactions and redshifts at specific constants.
Redshifts align with Karlsson's law, bringing Lyman lines into resonance.
Universe modeling becomes simpler with this approach.
Abstract
The law introduced by Karlsson in spectroscopy of low-redshift quasars involves the Lyman spectrum of hydrogen atoms. Thus, it appears necessary to study the concepts introduced by a standard spectroscopy of quasars, studied here, with those deducted from -CDM.A visible absorption of a sharp and saturated spectral line in a gas requires a long path without perturbations as collisions or cosmological redshift. Spectra of absorbed, saturated lines of quasars obeying Karlsson's law mainly result from interactions of natural, thermal light radiated by quasar with relatively cold, low presure atomic hydrogen. These lines are produced by three processes: a) A conventional absorption in a relatively cold gas produces a set of lines; b) These lines are multiplied by absorption after fundamental 3K or 4K redshifts, where K is Karlsson's constant: Spectra show that redshifts 3K (or 4K)…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Galaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research
