Image de couverture de livre

CHRONAL DYNAMICS. Evolution of the fundamental constants: ħ(z), α(z).

Fuente: Zenodo

Enregistré dans:

Détails bibliographiques
Auteur principal:	Kovalov, Hennadii
Format:	Recurso digital
Publié:	Zenodo 2026
Sujets:	evolution of Planck's constant, fine-structure constant, quasars, CMB, fundamental constants
Accès en ligne:	Acceder al recurso
Tags:	Ajouter un tag Pas de tags, Soyez le premier à ajouter un tag!

_version_	1866901256325300224
author	Kovalov, Hennadii
author_facet	Kovalov, Hennadii
contents	<p><span lang="EN-US">In the previous work (<strong>Absolute Time: </strong></span><strong><span>τ</span></strong><strong><span lang="EN-US">_CMB and Chronal Second</span></strong><span lang="EN-US">) it was shown that the CMB gives the absolute pulse of time </span><span>τ</span><span lang="EN-US">_CMB = ħ/(k· T_CMB). If </span><span>τ</span><span lang="EN-US">_CMB is fixed as a unit of time (a chronal second), then Planck's constant ħ cannot remain a constant—it must evolve with the expansion of the universe.</span></p> <p><span lang="EN-US">In this paper, the dependence ħ(z) = ħ₀· (1+z) and, as a result, the dependence of the fine-structure constant </span><span>α</span><span lang="EN-US">(z) = </span><span>α</span><span lang="EN-US">₀/(1+z). It is shown that this prediction is verifiable by the spectra of distant quasars: the expected relative change in </span><span>α</span><span lang="EN-US"> is </span><span>Δα</span><span lang="EN-US">/</span><span>α</span><span lang="EN-US"> ≈ -z at low z.</span></p> <p><span lang="EN-US">Experimental tests have been proposed: quasar spectroscopy (VLT, Keck), CMB (Planck) measurements, laboratory searches for drift </span><span>α</span><span lang="EN-US">.</span></p> <p><strong><span>Keywords:</span></strong><span> evolution of Planck's constant, fine-structure constant, quasars, CMB, fundamental constants</span></p>
format	Recurso digital
id	zenodo_https___doi_org_10_5281_zenodo_19420046
institution	Zenodo
language
publishDate	2026
publisher	Zenodo
record_format	zenodo
spellingShingle	CHRONAL DYNAMICS. Evolution of the fundamental constants: ħ(z), α(z). Kovalov, Hennadii evolution of Planck's constant, fine-structure constant, quasars, CMB, fundamental constants <p><span lang="EN-US">In the previous work (<strong>Absolute Time: </strong></span><strong><span>τ</span></strong><strong><span lang="EN-US">_CMB and Chronal Second</span></strong><span lang="EN-US">) it was shown that the CMB gives the absolute pulse of time </span><span>τ</span><span lang="EN-US">_CMB = ħ/(k· T_CMB). If </span><span>τ</span><span lang="EN-US">_CMB is fixed as a unit of time (a chronal second), then Planck's constant ħ cannot remain a constant—it must evolve with the expansion of the universe.</span></p> <p><span lang="EN-US">In this paper, the dependence ħ(z) = ħ₀· (1+z) and, as a result, the dependence of the fine-structure constant </span><span>α</span><span lang="EN-US">(z) = </span><span>α</span><span lang="EN-US">₀/(1+z). It is shown that this prediction is verifiable by the spectra of distant quasars: the expected relative change in </span><span>α</span><span lang="EN-US"> is </span><span>Δα</span><span lang="EN-US">/</span><span>α</span><span lang="EN-US"> ≈ -z at low z.</span></p> <p><span lang="EN-US">Experimental tests have been proposed: quasar spectroscopy (VLT, Keck), CMB (Planck) measurements, laboratory searches for drift </span><span>α</span><span lang="EN-US">.</span></p> <p><strong><span>Keywords:</span></strong><span> evolution of Planck's constant, fine-structure constant, quasars, CMB, fundamental constants</span></p>
title	CHRONAL DYNAMICS. Evolution of the fundamental constants: ħ(z), α(z).
topic	evolution of Planck's constant, fine-structure constant, quasars, CMB, fundamental constants
url	https://doi.org/10.5281/zenodo.19420046