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A New Limit on Planck Scale Lorentz Violation from Gamma-ray Burst Polarization

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arxiv 1102.2784 v6 pith:HX3WJORM submitted 2011-02-14 astro-ph.HE astro-ph.COgr-qchep-ph

A New Limit on Planck Scale Lorentz Violation from Gamma-ray Burst Polarization

classification astro-ph.HE astro-ph.COgr-qchep-ph
keywords constraintslorentzburstdimensioneffectivegammalimitparameter
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Constraints on possible Lorentz invariance violation (LIV) to first order in $E/M_{\rm Planck}$ for photons in the framework of effective field theory (EFT) are discussed, taking cosmological factors into account. Then, using the reported detection of polarized soft $\gamma$-ray emission from the $\gamma$-ray burst GRB041219a that is indicative of an absence of vacuum birefringence, together with a very recent improved method for estimating the redshift of the burst, we derive constraints on the dimension 5 Lorentz violating modification to the Lagrangian of an effective local QFT for QED. Our new constraints are more than five orders of magnitude better than recent constraints from observations of the Crab Nebula. We obtain the upper limit on the Lorentz violating dimension 5 EFT parameter $|\xi|$ of $2.4 \times 10^{-15}$, corresponding to a constraint on the dimension 5 standard model extension parameter, $k^{(5)}_{(V)00} \le 4.2 \times 10^{-34}$ GeV$^{-1}$.

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Cited by 2 Pith papers

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

  1. A winding number analysis of Schwarzschild black hole stability in light of Planck-scale modified kinematics

    gr-qc 2026-07 accept novelty 5.0

    Cubic entropy corrections from the MDR ηE³/E_P leave Schwarzschild black holes with a single physical branch of winding number W=−1; the would-be stable root is unphysical.

  2. A winding number analysis of Schwarzschild black hole stability in light of Planck-scale modified kinematics

    gr-qc 2026-07 conditional novelty 5.0

    For the cubic entropy correction S=πr_h²−αr_h³ arising from a Planck-scale modified dispersion relation, all physically allowed Schwarzschild-like branches have winding number w=−1, so no stable phase appears.