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No chiral light bending by clumps of axion-like particles

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arxiv 1910.06128 v1 pith:DJ5FWRFP submitted 2019-10-14 hep-ph astro-ph.COhep-th

No chiral light bending by clumps of axion-like particles

classification hep-ph astro-ph.COhep-th
keywords lightaxion-likeclumpsdifferentfrequencyparticlesvariationsabsorb
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We study the propagation of light in the presence of a parity-violating coupling between photons and axion-like particles (ALPs). Naively, this interaction could lead to a split of light rays into two separate beams of different polarization chirality and with different refraction angles. However, by using the eikonal method we explicitly show that this is not the case and that ALP clumps do not produce any spatial birefringence. This happens due to non-trivial variations of the photon's frequency and wavevector, which absorb time-derivatives and gradients of the ALP field. We argue that these variations represent a new way to probe the ALP-photon couping with precision frequency measurements.

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Cited by 4 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Spinoptics in the presence of axion-like particles in curved spacetime

    gr-qc 2026-07 accept novelty 6.5

    Spinoptics equations for axion–Maxwell theory yield helicity-dependent photon trajectory corrections from both spacetime curvature and arbitrary axion profiles.

  2. Sideband Structure of Axion Electrodynamics

    hep-ph 2026-07 unverdicted novelty 6.0

    Introduces a sideband ladder formulation of axion electrodynamics that classifies instabilities and conversion channels via Krein signatures in periodic backgrounds.

  3. Searching for axions with time resolved pulsar polarimetry

    hep-ph 2026-03 unverdicted novelty 6.0

    Time-resolved optical polarimetry of the Crab pulsar is used to place bounds on the axion-photon coupling via oscillating axion fields induced by the pulsar's magnetic field.

  4. Gravitational Wave Birefringence from Fuzzy Dark Matter

    gr-qc 2024-06 unverdicted novelty 5.0

    Fuzzy dark matter induces frequency-dependent amplitude birefringence in gravitational waves with periodic time modulation set by the scalar mass, but no velocity birefringence.