Severe Limits on Variations of the Speed of Light with Frequency

dc.creatorSchaefer, Bradley E.
dc.date1998-10-29
dc.date.accessioned2026-07-07T12:01:08Z
dc.date.available2026-07-07T12:01:08Z
dc.descriptionExplosive astrophysical events at high red shift can be used to place severe limits on the fractional variation in the speed of light ($Δc/c$), the photon mass ($m_γ$), and the energy scale of quantum gravity ($E_{QG}$). I find $Δc/c < 6.3 \times 10^{-21}$ based on the simultaneous arrival of a flare in GRB 930229 with a rise time of $220 \pm 30 μs$ for photons of 30 keV and 200 keV. The limit on $m_γ$ is $4.2 \times 10^{-44} g$ for GRB 980703 from radio to gamma ray observations. The limit on $E_{QG}$ is $8.3 \times 10^{16}$ GeV for GRB 930131 from 30 keV to 80 MeV photons.
dc.description7 pages, Submitted to PRL
dc.identifierhttps://arxiv.org/abs/astro-ph/9810479
dc.identifierhttp://arxiv.org/abs/astro-ph/9810479
dc.identifierPhys.Rev.Lett.82:4964-4966,1999
dc.identifierdoi:10.1103/PhysRevLett.82.4964
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/207004
dc.subjectAstrophysics
dc.titleSevere Limits on Variations of the Speed of Light with Frequency
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