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The high frequency peaked BL Lac object PG 1553+113 underwent a flaring event in 2012. The High Energy Stereoscopic System (H.E.S.S.) observed this source for two consecutive nights at very high energies (VHE, $E>$100~GeV). The data show an…

High Energy Astrophysical Phenomena · Physics 2019-08-14 D. A. Sanchez , F. Brun , C Couturier , A Jacholkowska , J. -P. Lenain

Very-high-energy (0.1-100 TeV) gamma-ray emission was observed in HAWC data from the lobes of the microquasar SS 433, making them the first set of astrophysical jets that were resolved at TeV energies. In this work, we update the analysis…

Direct laboratory bounds on the 9 nonbirefringent Lorentz-violating dimensionless parameters of modified-Maxwell theory range from the 10^{-7} level to the 10^{-16} level. The detection of air showers initiated by charged primaries…

High Energy Physics - Phenomenology · Physics 2008-10-28 F. R. Klinkhamer

Very-high-energy (VHE; $E \gtrsim 100$ GeV) gamma rays are expected to experience strong attenuation during cosmological propagation due to electron-positron pair production on the extragalactic background light (EBL). Recent observations…

High Energy Astrophysical Phenomena · Physics 2026-03-03 Longhua Qin , Jiancheng Wang , Chuyuan Yang , Huaizhen Li , Quangui Gao , Ju Ma , Ao Wang , Weiwei Na , Ming Zhou , Zunli Yuan , Chunxia Gu , Guangbo Long

The High-Altitude Water Cherenkov Observatory (HAWC) is a large field of view ($\sim$2sr) instrument sensitive to very-high energy gamma rays ($\sim$0.5-100TeV). It is located in central Mexico (19$^\circ$N) and has a high duty cycle…

High Energy Astrophysical Phenomena · Physics 2019-08-13 Israel Martinez-Castellanos

Lorentz invariance violation is a feature of several quantum gravity models in which Lorentz symmetry is broken at high energies, possibly leading to changes in particle behavior and interactions. In this work, we investigate vacuum…

High Energy Astrophysical Phenomena · Physics 2025-11-06 Andrey Saveliev , Rafael Alves Batista , Feodor Mishin

We present the first catalogs of the highest-energy (above 56 TeV and 100 TeV) gamma-ray sources seen by the High Altitude Water Cherenkov (HAWC) Observatory. The wide field-of-view of HAWC naturally lends itself to unbiased all-sky surveys…

High Energy Astrophysical Phenomena · Physics 2019-08-21 Kelly Malone

Despite the fact that quantum gravity theory still remains elusive, it is generally expected that it will bring the picture of a space-time foam at short distances leading to Lorenz Invariance Violation (LIV) manifested e.g. by energy…

Astrophysics · Physics 2015-05-13 Marek Biesiada , Aleksandra Piórkowska

The free photon dispersion relation is a reference quantity for high precision tests of Lorentz Invariance. We first outline theoretical approaches to a conceivable Lorentz Invariance Violation (LIV). Next we address phenomenological tests…

High Energy Physics - Theory · Physics 2010-01-16 Wolfgang Bietenholz

One of the experimental tests of Lorentz invariance violation is to measure the helicity dependence of the propagation velocity of photons originating in distant cosmological obejcts. Using a recent determination of the distance of the…

High Energy Astrophysical Phenomena · Physics 2015-05-28 P. Laurent , D. Gotz , P. Binetruy , S. Covino , A. Fernandez-Soto

The observation of cosmic neutrinos up to 2 PeV is used to put bounds on the energy scale of Lorentz invariance violation through the loss of energy due to the production of $e^+e^-$ pairs in the propagation of superluminal neutrinos. A…

High Energy Physics - Phenomenology · Physics 2019-12-02 J. M. Carmona , J. L. Cortes , J. J. Relancio , M. A. Reyes

The recent observation of high-energy astrophysical neutrinos can be used to constrain violations of Lorentz invariance emerging from a quantum theory of gravity. We perform threshold and Cherenkov analyses that improve existing bounds by…

High Energy Astrophysical Phenomena · Physics 2015-06-17 Jorge S. Diaz , Alan Kostelecky , Matthew Mewes

Although Lorentz symmetry has been tested at low energy with extremely good accuracy, its validity at very high energy is much less well established. If Lorentz symmetry violation (LSV) is energy-dependent (e.g. $\propto E^2$), it can be of…

General Physics · Physics 2016-10-26 Luis Gonzalez-Mestres

Recent observations of ultra high energy cosmic rays and gamma rays suggest that there are small violations of Lorentz symmetry. If there were no such violations, then the GZK cut off would hold and cosmic rays with energy $\sim 10^{20}eV$…

General Physics · Physics 2007-05-23 B. G. Sidharth

The positive-to-negative transition of spectral lag is an uncommon feature reported in a small number of GRBs. An application of such a feature has been made to constrain the critical quantum gravity energy ($E_{\rm QG}$) of the light…

High Energy Astrophysical Phenomena · Physics 2022-08-30 Zi-Ke Liu , Bin-Bin Zhang , Yan-Zhi Meng

Some of the best bounds on possible Lorentz violation in the electron sector come from observations of high-energy astrophysical phenomena. Using measurements of TeV inverse Compton radiation from a number of sources, we place the first…

High Energy Physics - Phenomenology · Physics 2008-11-26 Brett Altschul

High energy photons from astrophysical sources are unique probes for some predictions of candidate theories of Quantum Gravty (QG). In particular, imaging atmospheric Cherenkov telescopes (IACTs) are instruments optimised for astronomical…

High Energy Astrophysical Phenomena · Physics 2021-09-21 Tomislav Terzić , Daniel Kerszberg , Jelena Strišković

Searches for Lorentz invariance violation (LIV) in the neutrino sector have traditionally focused on non-standard neutrino oscillations induced by LIV in vacuum. In this work, however, we study anisotropic LIV in matter. First, we review…

High Energy Physics - Phenomenology · Physics 2026-02-10 Simon Hilding-Nørkjær , Johann Ioannou-Nikolaides , D. Jason Koskinen , Thomas Stuttard

Constraints on possible Lorentz invariance violation (LIV) to first order in $E/M_{\rm Planck}$ for photons in the framework of effective field theory (EFT) are discussed, taking cosmological factors into account. Then, using the reported…

High Energy Astrophysical Phenomena · Physics 2015-05-27 Floyd W. Stecker

The High Altitude Water Cherenkov (HAWC) observatory is a wide field-of-view detector sensitive to gamma rays of 100 GeV to a few hundred TeV. Located in central Mexico at 19 degrees North latitude and 4100 m above sea level, HAWC will…

High Energy Astrophysical Phenomena · Physics 2014-12-17 A. U. Abeysekara , R. Alfaro , C. Alvarez , J. D. Alvarez , R. Arceo , J. C. Arteaga-Velazquez , H. A. Ayala Solares , A. S. Barber , B. M. Baughman , N. Bautista-Elivar , J. Becerra Gonzalez , E. Belmont , S. Y. BenZvi , D. Berley , M. Bonilla Rosales , J. Braun , R. A. Caballero-Lopez , K. S. Caballero-Mora , A. Carraminana , M. Castillo , U. Cotti , J. Cotzomi , E. de la Fuente , C. De Leon , T. DeYoung , R. Diaz Hernandez , L. Diaz-Cruz , J. C. Diaz-Velez , B. L. Dingus , M. A. DuVernois , R. W. Ellsworth , S. F. E. , D. W. Fiorino , N. Fraija , A. Galindo , F. Garfias , M. M. Gonzalez , J. A. Goodman , V. Grabski , M. Gussert , Z. Hampel-Arias , J. P. Harding , C. M. Hui , P. Huentemeyer , A. Imran , A. Iriarte , P. Karn , D. Kieda , G. J. Kunde , A. Lara , R. J. Lauer , W. H. Lee , D. Lennarz , H. Leon Vargas , E. C. Linares , J. T. Linnemann , M. Longo , R. Luna-Garcia , A. Marinelli , H. Martinez , O. Martinez , J. Martinez-Castro , J. A. J. Matthews , J. McEnery , E. Mendoza Torres , P. Miranda-Romagnoli , E. Moreno , M. Mostafa , L. Nellen , M. Newbold , R. Noriega-Papaqui , T. Oceguera-Becerra , B. Patricelli , R. Pelayo , E. G. Perez-Perez , J. Pretz , C. Riviere , D. Rosa-Gonzalez , J. Ryan , H. Salazar , F. Salesa , A. Sandoval , M. Schneider , S. Silich , G. Sinnis , A. J. Smith , K. Sparks Woodle , R. W. Springer , I. Taboada , P. A. Toale , K. Tollefson , I. Torres , T. N. Ukwatta , L. Villasenor , T. Weisgarber , S. Westerhoff , I. G. Wisher , J. Wood , G. B. Yodh , P. W. Younk , D. Zaborov , A. Zepeda , H. Zhou , K. N. Abazajian
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