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Massive Galileons and Vainshtein Screening

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arxiv 2008.01456 v2 pith:LMCEKQPI submitted 2020-08-04 hep-th astro-ph.COgr-qc

Massive Galileons and Vainshtein Screening

classification hep-th astro-ph.COgr-qc
keywords screeningtheoriesvainshteinmassivetermsfindgalileonsmechanism
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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The Vainshtein screening mechanism relies on nonlinear interaction terms becoming dominant close to a compact source. However, theories displaying this mechanism are generally understood to be low-energy theories: it is unclear that operators emerging from UV completion do not interfere with terms inducing Vainshtein screening. In this work, we find a set of interacting massive Galileon theories that exhibit Vainshtein screening; examining potential UV completions of these theories, we determine that the screening does not survive the extension. We find that neglecting operators when integrating out a heavy field is non-trivial, and either care must be taken to ensure that omitted terms are small for the whole domain, or one is forced to work solely with the UV theory. We also comment on massive deformations of the familiar Wess-Zumino Galileons.

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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. Radial Solutions of Multi-Field de Sitter Galileons

    hep-th 2026-06 unverdicted novelty 6.0

    Derives conditions for viable screened radial solutions in multi-field de Sitter Galileons, showing curvature can mitigate superluminality at the cost of a finite validity range set by the strong-coupling point.

  2. Light scalars in light of UV/IR mixing: classicalization via synergy between Vainshtein and chameleon screenings

    hep-ph 2025-11 conditional novelty 5.0

    Classicalizing k-essence scalars need m << Λ* and, when potentials or fermion couplings are present, a chameleon-like screening layer to keep Vainshtein screening and classicalon stability intact.