Review article | Physics and astronomy

Dressing light to illuminate axion-symmetry matter

The putative axion particles with parity-time symmetry do not interact with transverse electromagnetic fields; hence, they are thought to constitute at least a part of the cosmological dark matter. Structured optical fields with E⋅B≠0 have the right symmetry to interact with axion dark matter. With the goal of generating fields with E⋅B≠0 that can interact with axion quasiparticles in condensed phase, as a portal for detecting dark matter, we image the vectorial surface plasmon polariton fields with 15 nm spatial resolution and 50 attosecond precision (at the speed of light) to reveal E⋅B≠0 term within the plasmonic vortex cores.

Keywords:
E⋅B≠0parity-time symmetryaxion quasiparticlesspin-charge entanglementultrafast photoemission electron microscopy
Submitted
25 August, 2026
Accepted
10 October, 2026
Published Online
03 November, 2026

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