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Cosmological Constraints on Lorentz Violation in Electrodynamics

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arxiv hep-ph/0111026 v1 pith:HOV77O3U submitted 2001-11-02 hep-ph astro-phhep-th

classification hep-phastro-phhep-th
keywords cosmologicallorentzviolationboundedcoefficientsconstrainconstraintselectrodynamics
verification ladder T0 review T1 audit T2 compute T3 formal
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Infrared, optical, and ultraviolet spectropolarimetry of cosmological sources is used to constrain the pure electromagnetic sector of a general Lorentz-violating standard-model extension. The coefficients for Lorentz violation are bounded to less than 3x10^{-32}.

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Cited by 2 Pith papers

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

  1. Exact Black Hole Solutions in Bumblebee Gravity with Lightlike or Spacelike VEVS

    gr-qc 2025-10 conditional novelty 5.0 of 10

    New exact Schwarzschild-like, (A)dS-like, and charged black holes in bumblebee gravity with a two-component vector VEV keep Lorentz-violating corrections even when the VEV is lightlike, with Wald and first-law entropi...

  2. Geometric optics analysis in Lorentz violating Chern-Simons electrodynamics

    hep-ph 2025-01 reject novelty 4.0 of 10

    Geometric optics in the Maxwell-Carroll-Field-Jackiw theory gives a polarization rotation proportional to the integrated background vector, with the standard intensity transport equation unchanged.

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