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We analyze the MeV/GeV emission from four bright Gamma-Ray Bursts (GRBs) observed by the Fermi-Large Area Telescope to produce robust, stringent constraints on a dependence of the speed of light in vacuo on the photon energy (vacuum…

High Energy Astrophysical Phenomena · Physics 2013-06-06 V. Vasileiou , A. Jacholkowska , F. Piron , J. Bolmont , C. Couturier , J. Granot , F. W. Stecker , J. Cohen-Tanugi , F. Longo

Some Quantum Gravity (QG) theories allow for a violation of Lorentz invariance (LIV), manifesting as a dependence of the velocity of light in vacuum on its energy. If such a dependence exists, then photons of different energies emitted…

We examine what the absorbed spectra of extra-galactic TeV gamma-ray sources, such as blazars, would look like in the presence of Lorentz invariance violation (LIV). Pair-production with the extra-galactic background light modifies the…

Astrophysics · Physics 2008-12-30 Uri Jacob , Tsvi Piran

We use the recent reanalysis of multi-TeV gamma-ray observations of Mrk 501 to constrain the Lorentz invariance breaking parameter involving the maximum electron velocity. Our limit is two orders of magnitude better than that obtained from…

Astrophysics · Physics 2011-06-09 F. W. Stecker , Sheldon L. Glashow

Modern ideas in quantum gravity predict the possibility of Lorenz Invariance Violation (LIV) manifested e.g. by energy dependent modification of standard relativistic dispersion relation. In a recent paper Jacob and Piran proposed that time…

Astrophysics · Physics 2009-06-30 Marek Biesiada , Aleksandra Piórkowska

GRB 221009A has posed a significant challenge to our current understanding of the mechanisms that produce TeV photons in gamma-ray bursts (GRB). On one hand, the Klein-Nishina (KN) effect of the inverse Compton scattering leads to less…

High Energy Astrophysical Phenomena · Physics 2025-06-23 D. Avila Rojas , S. Hernández-Cadena , M. M. González , A. Pratts , R. Alfaro , J. Serna-Franco

I discuss some theoretical ideas concerning the representation of quantum gravity as a Lorentz-symmetry-violating `medium' with non-trivial optical properties, which include a refractive index in `vacuo' and stochastic effects associated…

Astrophysics · Physics 2017-08-23 N. E. Mavromatos

The Crab Nebula was detected with the Milagro experiment at a statistical significance of 17 standard deviations over the lifetime of the experiment. The experiment was sensitive to approximately 100 GeV - 100 TeV gamma ray air showers by…

Relativistic jets from blazars are known to be sources of very-high-energy gamma rays (VHEGRs). During their propagation in the intergalactic space, VHEGRs interact with pervasive cosmological photon fields such as the extragalactic…

High Energy Astrophysical Phenomena · Physics 2019-10-01 Rafael Alves Batista , Andrey Saveliev , Elisabete M. de Gouveia Dal Pino

Fast variations of gamma-ray flux from Active Galactic Nuclei and Gamma-Ray Bursts can constrain Lorentz Invariance Violation (LIV) because of the delayed (or advanced) arrival of photons with higher energies: this approach has lead to the…

High Energy Astrophysical Phenomena · Physics 2019-08-13 Markus Gaug , Daniel Garrido

Gamma-ray bursts (GRBs) have been considered as potential very high-energy photon emitters due to the large amount of energy released as well as the strong magnetic fields involved in their jets. However, the detection of TeV photons is not…

High Energy Astrophysical Phenomena · Physics 2023-03-01 M. M. González , D. Avila Rojas , A. Pratts , S Hernández-Cadena , N. Fraija , R. Alfaro , Y. Pérez Araujo , J. A. Montes

(ABRIDGED) The Gamma-ray Large Area Space Telescope (GLAST) will measure the spectra of distant extragalactic sources of high energy gamma-rays. GLAST can look for energy dependent propagation effects from such sources as a signal of…

Astrophysics · Physics 2008-11-26 F. W. Stecker

Energy spectra of gamma-ray blazars may contain an imprint from the cosmic infrared background radiation due to gamma-ray absorption (pair-production) by soft photons constituting the extragalactic background light (EBL). The signature of…

Astrophysics · Physics 2009-09-29 F. Krennrich , E. Dwek

Gamma rays with energies greater than 7 TeV from the Crab pulsar/nebula have been observed at large zenith angles, using the Imaging Atmospheric Technique from Woomera, South Australia. CANGAROO data taken in 1992, 1993 and 1995 indicate…

We spectrally fit the GeV gamma-ray flares recently-observed in the Crab Nebula by considering a small blob Lorentz-boosted towards us. We point out that the corresponding inverse-Compton flare at TeV--PeV region is more enhanced than…

High Energy Astrophysical Phenomena · Physics 2015-06-04 Kazunori Kohri , Yutaka Ohira , Kunihito Ioka

The modelling of gamma-ray burst (GRB) spectra has considerable potential for increasing the understanding of these enigmatic sources. A diversity of ideas and analyses has been generated over the last two decades to explain line features…

Astrophysics · Physics 2009-10-28 M. G. Baring

During the observation period 1997, the nearby Blazar Mkn 501 showed extremely strong emission and high variability. We examine multiwavelength aspects of this event using radio, optical, soft and hard X-ray and TeV data. We concentrate on…

The delay in the arrival times between high and low energy photons from cosmic sources can be used to test the violation of the Lorentz invariance (LIV), predicted by some quantum gravity theories, and to constrain its characteristic energy…

High Energy Astrophysical Phenomena · Physics 2017-11-29 M. G. Bernardini , G. Ghirlanda , S. Campana , P. D'Avanzo , J. -L. Atteia , S. Covino , G. Ghisellini , A. Melandri , F. Piron , R. Salvaterra , G. Tagliaferri

Quantum gravity arguments and the entropy bound for effective field theories proposed in PRL 82, 4971 (1999) lead to consider two correlated scales which parametrize departures from relativistic quantum field theory at low and high…

High Energy Physics - Theory · Physics 2012-03-15 J. M. Carmona , J. L. Cortes

Due to their higher concentrations and small internal velocities, Milky Way subhalos can be at least as important as the smooth halo in accounting for the GeV positron excess via dark matter annihilation. After showing how this can be…

High Energy Astrophysical Phenomena · Physics 2010-08-13 Matthew D. Kistler , Jennifer M. Siegal-Gaskins