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The status of varying constants: a review of the physics, searches and implications

2017/08/14 by C. J. A. P. Martins, C J A P Martins · 1 voice · 1 citation
Physics and Astronomy · #Consistency (knowledge bases) #Cosmology #Cosmology and Gravitation Theories #Physics beyond the Standard Model #Preference #Radioactive Decay and Measurement Techniques #Range (aeronautics) #Relativity and Gravitational Theory #Stability (learning theory) #Statistical hypothesis testing #Task (project management) #astro-ph.CO #gr-qc #hep-ph #hep-th

paper · pdf · doi:10.1088/1361-6633/aa860e

Invited review for Reports on Progress in Physics (49 pages, 6 figures, 11 tables; submitted 24 January 2017, accepted 14 August 2017)

openalex publication_date 2017/08/14 · openalex created_date 2017/08/31 · arxiv created 2017/09/09 · arxiv published 2017/09/09 · arxiv updated 2017/09/12 · openalex updated_date 2026/08/05

Abstract

The observational evidence for the recent acceleration of the universe demonstrates that canonical theories of cosmology and particle physics are incomplete-if not incorrect-and that new physics is out there, waiting to be discovered. A key task for the next generation of laboratory and astrophysical facilities is to search for, identify and ultimately characterize this new physics. Here we highlight recent developments in tests of the stability of nature's fundamental couplings, which provide a direct handle on new physics: a detection of variations will be revolutionary, but even improved null results provide competitive constraints on a range of cosmological and particle physics paradigms. A joint analysis of all currently available data shows a preference for variations of α and μ at about the two-sigma level, but inconsistencies between different sub-sets (likely due to hidden systematics) suggest that these statistical preferences need to be taken with caution. On the other hand, these measurements strongly constrain Weak Equivalence Principle violations. Plans and forecasts for forthcoming studies with facilities such as ALMA, ESPRESSO and the ELT, which should clarify these issues, are also discussed, and synergies with other probes are briefly highlighted. The goal is to show how a new generation of precision consistency tests of the standard paradigm will soon become possible.

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