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We seek a power-law solution of the formQ(r)∝r n−1, wherenis the screening efficiency (51)

General Screening Behaviour (κ − ̸=κ + ̸= 0) Outside the source (r > R), the density contrast vanishes, the profile is determined by the nonlinear terms

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A Master Equation for Screening in Luminal Horndeski Gravity

gr-qc · 2026-05-05 · unverdicted · novelty 7.0

A master screening equation is derived for luminal Horndeski gravity that recovers Vainshtein and Chameleon mechanisms and introduces Phaedrus screening with screening radius scaling linearly with source mass.

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  • A Master Equation for Screening in Luminal Horndeski Gravity gr-qc · 2026-05-05 · unverdicted · none · ref 1

    A master screening equation is derived for luminal Horndeski gravity that recovers Vainshtein and Chameleon mechanisms and introduces Phaedrus screening with screening radius scaling linearly with source mass.