1996
DOI: 10.1080/10556799608203019
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Microwave background radiation and cosmological large numbers

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Cited by 7 publications
(3 citation statements)
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“…It would be fair to acknowledge that for the static Universe, a similar thermalised radiation with T = 3 K was predicted even earlier, in 1926, by A.S. Eddington [120] and with T = 2.8 K by W. Nernst in 1937 [121]. For more comprehensive reviews as to the possibility of explaining the CMB radiation within the framework of static-Universe models see, for example, [122,123].…”
Section: Discussionmentioning
confidence: 75%
“…It would be fair to acknowledge that for the static Universe, a similar thermalised radiation with T = 3 K was predicted even earlier, in 1926, by A.S. Eddington [120] and with T = 2.8 K by W. Nernst in 1937 [121]. For more comprehensive reviews as to the possibility of explaining the CMB radiation within the framework of static-Universe models see, for example, [122,123].…”
Section: Discussionmentioning
confidence: 75%
“…Only much later, in 1953, G. Gamow made his prediction with respect to the CMBR and its temperature T = 7 K for the expanding-Universe model [63]. Several other authors, e.g., [64,65], were exploring CMBR properties in the 1990s and 2000s within the framework of a static universe model. The possibility of a local origin of the CMBR was already excluded by measurements of excitation lines in absorption features of quasar spectra [66], and by measuring the imprint of galaxy clusters on the CMBR via the Sunyaev-Zeldovich effect [67].…”
Section: Cosmological Redshift and The Cosmic Backgroundmentioning
confidence: 99%
“…From the point of view of the astrophysics community, the validity of the orthodox interpretation of CMB is largely resolved, with some doubts voiced from time to time (e.g., Baryshev, Raikov and Tron 1996). And as far as the general issue of the choice of cosmological models is concerned, the standard cosmological model seems to rest on a secure foundation (for review of some exotic alternatives, see Ellis 1984).…”
Section: Introductionmentioning
confidence: 99%