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Frequency shifts induced by light scalar fields

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arxiv 2410.11567 v2 pith:H6FNCCPM submitted 2024-10-15 hep-ph astro-ph.COgr-qchep-thquant-ph

classification hep-phastro-ph.COgr-qchep-thquant-ph
keywords frequencyinducedscalarshiftsfieldsuseddarkinterferometry
verification ladder T0 review T1 audit T2 compute T3 formal

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abstract

Light scalar fields are frequently used in modern physics, for example, as candidates for dark energy or dark matter. Open quantum dynamical effects, like frequency shifts, induced by such fields in probe particles used in interferometry experiments might open up new perspectives for constraining such models. In this article, we consider a probe scalar particle as a rough approximation for an atom in matter wave interferometry and discuss the frequency shifts induced by interactions with an environment comprising either one of two screened scalar field models: chameleons or symmetrons. For the $n=-4$ chameleon, we revise a previously obtained expression for the induced frequency shift, but confirm that it can likely not be used to obtain new constraints. However, for symmetrons, we find that induced frequency shifts have the potential to tightly constrain previously unreachable parts of the parameter space.

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Forward citations

Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. An Open Effective Field Theory for light in a medium

    hep-th 2024-12 conditional novelty 6.0 of 10

    A dissipative open EFT for photons in a medium is constructed, featuring a deformed advanced gauge symmetry and a noise constraint vμ(jμ+ξμ)=0.

  2. Direct detection of solar chameleons with electron recoil data from XENONnT

    hep-ph 2025-11 conditional novelty 5.0 of 10

    XENONnT electron-recoil data bound solar chameleons to log10 β_eff < −6.9, independent of the potential index n for inverse power-law chameleons at the dark-energy scale.

  3. Particles in finite volumes and a toy model of decaying neutrons

    hep-ph 2025-04 reject novelty 4.0 of 10

    A toy scalar model of neutron decay suggests finite-volume effects and initial neutron-daughter correlations can shift the predicted neutron lifetime to about 887 seconds, but the agreement is obtained by tuning a parameter.

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