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Fine structure constant measurements in quasar absorption systems

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arxiv 2310.01071 v1 pith:BHBBVQ2I submitted 2023-10-02 astro-ph.CO astro-ph.IM

classification astro-ph.COastro-ph.IM
keywords measurementsabsorptionconstantdipoleeffectsfinequasarsample
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Detecting any evolution of dimensionless in the ratios of physical quantities, such as the fine structure constant, would prove that the Weak Equivalence Principle is violated and lead to a paradigm shift in physics. High resolution spectroscopy of quasar absorption systems can be used to test cosmological variations in time and/or in space. A sample of 300 measurements using data from 8m class optical telescopes provides hints that such variations are indeed present in a form of a spatial dipole across the sky, although systematic effects could dominate. Two recent developments, one in instrumentation and the other in analysis methods, promise to produce a new sample of measurements free from all known systematic effects to test the tentative dipole.

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  1. The fine structure constant: a review of measurement results and possible space-time variations

    hep-ph 2025-06 accept novelty 1.0 of 10

    A review showing that the most precise recent measurements of the fine structure constant disagree with CODATA-2018 beyond 3σ, while laboratory and astrophysical searches have not confirmed any clear space-time variation.

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