Đã lưu trong:
| Tác giả chính: | |
|---|---|
| Định dạng: | Recurso digital |
| Ngôn ngữ: | |
| Được phát hành: |
Zenodo
2026
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| Những chủ đề: | |
| Truy cập trực tuyến: | https://doi.org/10.5281/zenodo.19420046 |
| Các nhãn: |
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Mục lục:
- <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>