Gamma Ray Burst Constraints on Ultraviolet Lorentz Invariance Violation

dc.creatorKahniashvili, Tina
dc.creatorGogoberidze, Grigol
dc.creatorRatra, Bharat
dc.date2006-07-04
dc.date2006-10-20
dc.date.accessioned2026-07-07T10:23:17Z
dc.date.available2026-07-07T10:23:17Z
dc.descriptionWe present a unified general formalism for ultraviolet Lorentz invariance violation (LV) testing through electromagnetic wave propagation, based on both dispersion and rotation measure data. This allows for a direct comparison of the efficacy of different data to constrain LV. As an example we study the signature of LV on the rotation of the polarization plane of $γ$-rays from gamma ray bursts in a LV model. Here $γ$-ray polarization data can provide a strong constraint on LV, 13 orders of magnitude more restrictive than a potential constraint from the rotation of the cosmic microwave background polarization proposed by Gamboa, López-Sarrión, and Polychronakos (2006).
dc.description5 pages, references added, accepted for publication in Phys. Lett. B
dc.identifierhttps://arxiv.org/abs/astro-ph/0607055
dc.identifierhttp://arxiv.org/abs/astro-ph/0607055
dc.identifierPhys.Lett.B643:81-85,2006
dc.identifierdoi:10.1016/j.physletb.2006.10.041
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/175771
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectHigh Energy Physics - Theory
dc.titleGamma Ray Burst Constraints on Ultraviolet Lorentz Invariance Violation
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