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Constraints on Lorentz invariance violation from gamma-ray burst GRB090510

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arxiv 0909.4927 v6 pith:ODHO2XXW submitted 2009-09-27 hep-ph astro-ph.COastro-ph.HEgr-qchep-th

classification hep-phastro-ph.COastro-ph.HEgr-qchep-th
keywords dispersionburstconstraintsgamma-raygrb090510invariancelorentzmass
verification ladder T0 review T1 audit T2 compute T3 formal

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abstract

We obtain modified dispersion relations by requiring the vanishing of determinant of inverse of modified photon propagators in Lorentz invariance violation (LIV) theory. Inspired by these dispersion relations, we give a more general dispersion relation with less assumption and apply it to the recent observed gamma-ray burst GRB090510 to extract various constraints on LIV parameters. We find that the constraint on quantum gravity mass is slightly larger than the Planck mass but is consistent with the other recent observations, so the corresponding LIV coefficient $\xi_1$ has reached the natural order ($o(1)$) as one expects. From our analysis, the linear LIV corrections to photon group velocity might be not excluded yet.

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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. Monte Carlo simulation of GRB data to test Lorentz-invariance violation

    hep-ph 2025-04 conditional novelty 5.0 of 10

    A combined model with both Lorentz-violation and energy-dependent intrinsic delays recovers simulated parameters across all mock datasets and fits multi-GeV and TeV GRB photons, yielding a subluminal LV scale of about...

  2. Examining Lorentz invariance violation with three remarkable GRB photons

    astro-ph.HE 2025-04 conditional novelty 4.0 of 10

    Adding three extreme GRB photons preserves the fitted Lorentz-violation scale E_LV ~ 3e17 GeV, but only when an energy-dependent intrinsic delay term, itself a fitting construct, absorbs the new TeV photons.

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