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Dilaton Solutions for Laboratory Constraints and Lunar Laser Ranging

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arxiv 2203.12512 v1 pith:NNY2CQ2O submitted 2022-03-23 gr-qc astro-ph.COhep-ph

classification gr-qcastro-ph.COhep-ph
keywords dilatonsolutionsequationsfieldlaserlunarrangingsystem
verification ladder T0 review T1 audit T2 compute T3 formal
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We derive approximate analytical solutions to the environment-dependent dilaton field theory equations in the presence of a one or two mirror system or a sphere. The one-dimensional equations of motion are integrated for each system. The solutions obtained herein can be applied to \textit{q}BOUNCE experiments, neutron interferometry and for the calculation of the dilaton field induced "Casimir force" in the \textsc{Cannex} experiment as well as for Lunar Laser Ranging. They are typical of the Damour-Polyakov screening mechanism whereby deviations from General Relativity are suppressed by a vanishingly small direct coupling of the dilaton to matter in dense environments.

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Cited by 2 Pith papers

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

  1. Weinberg's theorem, phantom crossing and screening

    astro-ph.CO 2025-07 conditional novelty 5.0 of 10

    Graviton-loop-induced screening forces single-field dilaton and chameleon dark energy models to keep their equation of state near -1, making observable phantom crossing impossible in this class.

  2. Experimental test of symmetron-field based dark energy model using neutron interferometry

    hep-ph 2026-06 unverdicted novelty 4.0 of 10

    Neutron interferometry finds no symmetron-induced phase shifts and sets constraints on this quintessence dark energy candidate.

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