中文

CMB Birefringence from Vacuum Interfaces

高能物理 - 理论 2026-05-14 v1 宇宙学与河外天体物理 广义相对论与量子宇宙学 高能物理 - 唯象学 量子物理

摘要

Hints of cosmic microwave background polarization rotation (Δϑ103\Delta\vartheta \sim 10^{-3} rad) are commonly attributed to late-time dynamics of ultralight axions. We show that such ultralight degrees of freedom are not required. Polarization rotation naturally arises as a geometric interface phase acquired when photons cross interfaces between topologically distinct dark sector vacua. The effect is a discrete phase shift fixed by the normalization of a wall-supported electromagnetic Chern--Simons interaction and protected by an emergent 11-form symmetry of the low energy effective theory. This mechanism reproduces the familiar adiabatic rotation induced by light axion domain walls, but persists for arbitrarily thin walls where the axion is heavy or absent. In this regime the rotation manifests as a Pancharatnam phase localized at vacuum interfaces, independent of redshift and photon frequency below a natural ultraviolet cutoff. Cosmic birefringence thus emerges as a probe of vacuum structure in the dark sector, rather than of light-field dynamics.

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引用

@article{arxiv.2605.11065,
  title  = {CMB Birefringence from Vacuum Interfaces},
  author = {Nemanja Kaloper},
  journal= {arXiv preprint arXiv:2605.11065},
  year   = {2026}
}

备注

26 pages, LaTeX