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New Physics and the Proton Radius Problem

1 Pith paper cite this work. Polarity classification is still indexing.

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abstract

Background: The recent disagreement between the proton charge radius extracted from Lamb shift measurements of muonic and electronic hydrogen invites speculation that new physics may be to blame. Several proposals have been made for new particles that account for both the Lamb shift and the muon anomalous moment discrepancies. Purpose: We explore the possibility that new particles' couplings to the muon can be fine-tuned to account for all experimental constraints. Method: We consider two fine-tuned models, the first involving new particles with scalar and pseudoscalar couplings, and the second involving new particles with vector and axial couplings. The couplings are constrained by the Lamb shift and muon magnetic moments measurements while mass constraints are obtained by kaon decay rate data. Results: For the scalar-pseudoscalar model, masses between 100 to 200 MeV are not allowed. For the vector model, masses below about 200 MeV are not allowed. The strength of the couplings for both models approach that of electrodynamics for particle masses of about 2 GeV. Conclusions: New physics with fine tuned couplings may be entertained as a possible explanation for the Lamb shift discrepancy.

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2025 1

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representative citing papers

New Constraints on Neutrino-Dark Matter Interactions: A Comprehensive Analysis

hep-ph · 2025-07-01 · conditional · novelty 6.0

Most benchmark neutrino-dark matter couplings adopted in previous studies are excluded when laboratory meson and Z decay bounds are combined with cosmological and astrophysical constraints, leaving only special galactic-spike scenarios for observable supernova-neutrino attenuation.

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  • New Constraints on Neutrino-Dark Matter Interactions: A Comprehensive Analysis hep-ph · 2025-07-01 · conditional · none · ref 226 · internal anchor

    Most benchmark neutrino-dark matter couplings adopted in previous studies are excluded when laboratory meson and Z decay bounds are combined with cosmological and astrophysical constraints, leaving only special galactic-spike scenarios for observable supernova-neutrino attenuation.