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Limits on Lorentz Violation from Synchrotron and Inverse Compton Sources

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arxiv hep-ph/0603138 v1 pith:N6TB2SBI submitted 2006-03-17 hep-ph astro-phhep-th

B. Altschul This is my paper · ORCID
classification hep-phastro-phhep-th
keywords boundscoefficientscomptondataelectroninverselevellorentz
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We derive new bounds on Lorentz violations in the electron sector from existing data on high-energy astrophysical sources. Synchrotron and inverse Compton data give precisely complementary constraints. The best bound on a specific combination of electron Lorentz-violating coefficients is at the 6 x 10^(-20) level, and independent bounds are available for all the Lorentz-violating c coefficients at the 2 x 10^(-14) level or better. This represents an improvement in some bounds by fourteen orders of magnitude.

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Cited by 1 Pith paper

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  1. Spectra for Reactions in Astrophysical Electromagnetic Cascades with Lorentz Invariance Violation: The Vacuum Cherenkov Effect

    astro-ph.HE 2024-12 conditional novelty 4.0 of 10

    The authors provide closed-form total rates and simulated photon and electron spectra for vacuum Cherenkov radiation under second-order Lorentz invariance violation.

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