2010
DOI: 10.1016/j.astropartphys.2010.03.003
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Lorentz violation from cosmological objects with very high energy photon emissions

Abstract: Lorentz violation (LV) is predicted by some quantum gravity theories, where photon dispersion relation is modified, and the speed of light becomes energydependent. Consequently, it results in a tiny time delay between high energy photons and low energy ones. Very high energy (VHE) photon emissions from cosmological distance can amplify these tiny LV effects into observable quantities. Here we analyze four VHE γ-ray bursts (GRBs) from Fermi observations, and briefly review the constraints from three TeV flares … Show more

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Cited by 90 publications
(130 citation statements)
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“…[76][77][78] for recent attempts of addressing anomalies in 2 + 1 dimensions), and to be in violation with current observations such as tests of Lorentz Invariance (LI). Stringent constraints on LI violation have been placed via observations of Gamma-Ray Bursts (GRB) by the FERMI Large Area Telescope, LAT [79], which is sensitive to MeV-to-GeV GRBs, and the Gamma-Ray Burst Monitor collaborations that use GRB 080916C [80] and GRB 090510 [81]. In addition, competitive results can be achieved by observations of flares of Active Galactive Nuclei by MAGIC, or the H.E.S.S.…”
Section: Loop Quantum Cosmologymentioning
confidence: 99%
“…[76][77][78] for recent attempts of addressing anomalies in 2 + 1 dimensions), and to be in violation with current observations such as tests of Lorentz Invariance (LI). Stringent constraints on LI violation have been placed via observations of Gamma-Ray Bursts (GRB) by the FERMI Large Area Telescope, LAT [79], which is sensitive to MeV-to-GeV GRBs, and the Gamma-Ray Burst Monitor collaborations that use GRB 080916C [80] and GRB 090510 [81]. In addition, competitive results can be achieved by observations of flares of Active Galactive Nuclei by MAGIC, or the H.E.S.S.…”
Section: Loop Quantum Cosmologymentioning
confidence: 99%
“…The motivation of DSR theories is also derived from the observation of interesting effects such as deformation of dispersion relation etc. at very high energy scales [1,[4][5][6][7]. The introduction of an observer independent energy scale in DSR formulation, say κ, leads to such a modification in the dispersion relation of a free particle [1,2,8,9].…”
Section: Introductionmentioning
confidence: 99%
“…In the past, various limits on LIV have been obtained from the spectral time lags of individual GRB or a large sample of GRBs (e.g., Amelino-Camelia et al 1998;Coleman & Glashow 1999;Schaefer 1999;Ellis et al 2003Ellis et al , 2006Boggs et al 2004;Kahniashvili et al 2006;Jacob & Piran 2008;Abdo et al 2009a,b;Biesiada & Piórkowska 2009;Xiao & Ma 2009;Shao et al 2010;Chang et al 2012Chang et al , 2016Nemiroff et al 2012;Ellis & Mavromatos 2013;Kostelecký & Mewes 2013;Vasileiou et al 2013Vasileiou et al , 2015Pan et al 2015;Zhang & Ma 2015;Wei et al 2016). In particular, Abdo et al (2009a) used the time lag of the highest energy (13.2 GeV) photon from GRB 080916C to constrain the linear LIV energy scale (E QG,1 ) and presented a stringent limit of 1.3 × 10 18 GeV, improving the previous limits by at least one order of magnitude.…”
Section: Introductionmentioning
confidence: 99%