Model-independent confirmation of a constant speed of light over cosmological distances
Author
Melia, F.Affiliation
Department of Physics, The Applied Math Program, Department of Astronomy, The University of ArizonaIssue Date
2023-12-01
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Oxford University PressCitation
Fulvio Melia, Model-independent confirmation of a constant speed of light over cosmological distances, Monthly Notices of the Royal Astronomical Society, Volume 527, Issue 3, January 2024, Pages 7713–7718, https://doi.org/10.1093/mnras/stad3731Rights
© 2023 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society. This is an Open Access article distributed under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0/).Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
Recent attempts at measuring the variation of c using an assortment of standard candles and the redshift-dependent Hubble expansion rate inferred from the currently available catalogue of cosmic chronometers have tended to show that the speed of light appears to be constant, at least up to z ∼2. A notable exception is the use of high-redshift ultraviolet + X-ray quasars, whose Hubble diagram seems to indicate an ∼2.7σ deviation of c from its value c0 (2.99792458 × 1010 cm s-1) on Earth. We show in this paper, however, that this anomaly is due to an error in the derived relation between the luminosity distance, DL, and H(z) when c is allowed to vary with redshift, and an imprecise calibration of the quasar catalogue. When these deficiencies are addressed correctly, one finds that c/c0 = 0.95 ± 0.14 in the redshift range 0 z 2, fully consistent with zero variation within the measurement errors. © 2023 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society.Note
Open access articleISSN
0035-8711Version
Final Published Versionae974a485f413a2113503eed53cd6c53
10.1093/mnras/stad3731
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Except where otherwise noted, this item's license is described as © 2023 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society. This is an Open Access article distributed under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0/).