Working Notes (First Draft-2): Relativistic Shedding as Threshold Emission into Hidden Sectors

27 September 2025, Version 1
This content is an early or alternative research output and has not been peer-reviewed by Cambridge University Press at the time of posting.

Abstract

This is a first-pass sketch to capture the idea and obvious checks before polishing. I propose a kinematic-threshold mechanism: when a highly boosted excitation outruns the phase velocity of some field mode in its environment, an emissive channel opens. In ordinary dielectrics this is Cherenkov light; here I hypothesize that, in the early universe and in certain laboratory media, analogous thresholds also open into a hidden sector, potentially producing (i) a stable cold dark-matter remnant χ, (ii) a small amount of hidden radiation (kept under current ∆Neff bounds), and (iii) an ultra-light, shift-symmetric scalar ϕ whose potential energy today behaves like dark energy. The emphasis in this draft is on testability and built-in failure modes; details are provisional and meant to be tightened after basic consistency checks.

Keywords

dark photon
kinetic mixing
vector portal
hidden sector
Cherenkov-like emission
in-medium mixing
refractive index
dispersion relation
threshold emission
missing-momentum (LDMX)

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