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It has been long conjectured that a signature of Quantum Gravity will be Lorentz Invariance Violation (LIV) that could be observed at energies much lower than the Planck scale. One possible signature of LIV is an energy-dependent speed of…

High Energy Astrophysical Phenomena · Physics 2024-03-29 Tsvi Piran , Dmitry D. Ofengeim

After almost 4 years of operation, the two instruments onboard the Fermi Gamma-ray Space Telescope have shown that the number of gamma-ray bursts with high energy photon emission above 100 MeV cannot exceed roughly 9% of the total number of…

High Energy Astrophysical Phenomena · Physics 2015-06-05 Carl W. Akerlof , WeiKang Zheng

Intrinsic variability was searched for in arrival times of six gamma-ray bursts (GRBs) at high energies -- between 30 MeV and 2 GeV -- detected by the Fermi satellite's Large Area Telescope (LAT). The GRBs were selected from the Fermi LAT…

High Energy Astrophysical Phenomena · Physics 2024-07-31 E. Casey Aldrich , Robert J. Nemiroff

The Fermi Gamma-ray Space Telescope with its main instrument onboard, the Large Area Telescope (LAT), opened a new era in high-energy astrophysics and in particular for the study of Gamma-Ray Bursts (GRBs), which are short flashes of -rays…

High Energy Astrophysical Phenomena · Physics 2010-12-03 Aurelien Bouvier

Lorentz invariance violation in photons can be quantified by measuring the difference in arrival times between high- and low-energy photons originating from gamma-ray bursts (GRBs). When analyzing data, it is crucial to consider the…

High Energy Astrophysical Phenomena · Physics 2025-04-22 Hanlin Song , Bo-Qiang Ma

We examine 288 GRBs detected by the Fermi Gamma-ray Space Telescope's Gamma-ray Burst Monitor (GBM) that fell within the field-of-view of Fermi's Large Area Telescope (LAT) during the first 2.5 years of observations, which showed no…

High Energy Astrophysical Phenomena · Physics 2015-06-03 LAT Collaboration , GBM Collaboration

In quantum theory of gravity, we expect the Lorentz Invariance Violation (LIV) and the modification of the dispersion relation between energy and momentum for photons. The effect of the energy-dependent velocity due to the modified…

Cosmology and Nongalactic Astrophysics · Physics 2020-01-24 Yu Pan , Yungui Gong , Shuo Cao , He Gao , Zong-Hong Zhu

The recent detection of gamma-ray burst GRB~221009A has attracted attention due to its record brightness and first-ever detection of $\gtrsim 10$ TeV $\gamma$ rays from a GRB. Despite being the second-nearest GRB ever detected, at a…

High Energy Astrophysical Phenomena · Physics 2024-06-18 Hassan Abdalla , Soebur Razzaque , Markus Böttcher , Justin Finke , Alberto Domínguez

The variable activity of a gamma-ray burst (GRB) source is thought to be correlated with its absolute peak luminosity - a relation that, if confirmed, can be used to derive an independent estimate of the redshift of a GRB. We find that…

Astrophysics · Physics 2009-11-07 Nicole M. Lloyd-Ronning , Enrico Ramirez-Ruiz

Since the discovery of the cosmological origin of GRBs there has been growing interest in using these transient events to probe the quantum gravity energy scale in the range 10^16--10^19 GeV, up to the Planck mass scale. This energy scale…

Astrophysics · Physics 2009-11-10 Steven E. Boggs , Cornelia B. Wunderer , Kevin Hurley , Wayne Coburn

We present a complete analysis of Fermi Large Area Telescope (LAT) data of GRB 221009A, the brightest Gamma-Ray Burst (GRB) ever detected. The burst emission above 30 MeV detected by the LAT preceded by 1 s the low-energy (< 10 MeV) pulse…

High Energy Astrophysical Phenomena · Physics 2024-09-10 M. Axelsson , M. Ajello , M. Arimoto , L. Baldini , J. Ballet , M. G. Baring , C. Bartolini , D. Bastieri , J. Becerra Gonzalez , R. Bellazzini , B. Berenji , E. Bissaldi , R. D. Blandford , R. Bonino , P. Bruel , S. Buson , R. A. Cameron , R. Caputo , P. A. Caraveo , E. Cavazzuti , C. C. Cheung , G. Chiaro , N. Cibrario , S. Ciprini , G. Cozzolongo , P. Cristarella Orestano , M. Crnogorcevic , A. Cuoco , S. Cutini , F. D'Ammando , S. De Gaetano , N. Di Lalla , A. Dinesh , R. Di Tria , L. Di Venere , A. Domínguez , S. J. Fegan , E. C. Ferrara , A. Fiori , A. Franckowiak , Y. Fukazawa , S. Funk , P. Fusco , G. Galanti , F. Gargano , C. Gasbarra , S. Germani , F. Giacchino , N. Giglietto , M. Giliberti , R. Gill , F. Giordano , M. Giroletti , J. Granot , D. Green , I. A. Grenier , S. Guiriec , M. Gustafsson , M. Hashizume , E. Hays , J. W. Hewitt , D. Horan , T. Kayanoki , M. Kuss , A. Laviron , J. Li , I. Liodakis , F. Longo , F. Loparco , L. Lorusso , B. Lott , M. N. Lovellette , P. Lubrano , S. Maldera , D. Malyshev , A. Manfreda , G. Martí-Devesa , R. Martinelli , I. Martinez Castellanos , M. N. Mazziotta , J. E. McEnery , I. Mereu , M. Meyer , P. F. Michelson , N. Mirabal , W. Mitthumsiri , T. Mizuno , P. Monti-Guarnieri , M. E. Monzani , T. Morishita , A. Morselli , I. V. Moskalenko , M. Negro , R. Niwa , N. Omodei , M. Orienti , E. Orlando , D. Paneque , G. Panzarini , M. Persic , M. Pesce-Rollins , V. Petrosian , R. Pillera , F. Piron , T. A. Porter , G. Principe , J. L. Racusin , S. Rainò , R. Rando , B. Rani , M. Razzano , S. Razzaque , A. Reimer , O. Reimer , F. Ryde , M. Sánchez-Conde , P. M. Saz Parkinson , D. Serini , C. Sgrò , V. Sharma , E. J. Siskind , G. Spandre , P. Spinelli , D. J. Suson , H. Tajima , D. Tak , J. B. Thayer , D. F. Torres , J. Valverde , G. Zaharijas , S. Lesage , M. S. Briggs , E. Burns , S. Bala , P. N. Bhat , W. H. Cleveland , S. Dalessi , C. de Barra , M. Gibby , M. M. Giles , R. Hamburg , B. A. Hristov , C. M. Hui , D. Kocevski , B. Mailyan , C. Malacaria , S. McBreen , S. Poolakkil , O. J. Roberts , L. Scotton , P. Veres , A. von Kienlin , C. A. Wilson-Hodge , J. Wood

Gamma-ray bursts (GRBs) are the most powerful explosions in the universe and probe physics under extreme conditions. GRBs divide into two classes, of short and long duration, thought to originate from different types of progenitor systems.…

High Energy Astrophysical Phenomena · Physics 2014-11-20 LAT Collaboration

Explosive astrophysical events at high red shift can be used to place severe limits on the fractional variation in the speed of light ($\Delta c/c$), the photon mass ($m_{\gamma}$), and the energy scale of quantum gravity ($E_{QG}$). I find…

Astrophysics · Physics 2008-11-26 Bradley E. Schaefer

Astrophysical observations provide a unique opportunity to test possible signatures of Lorentz Invariance Violation (LIV), due to the high energies and long distances involved. In quantum theory of gravity, one may expect the modification…

Cosmology and Nongalactic Astrophysics · Physics 2020-03-04 Yu Pan , Jingzhao Qi , Shuo Cao , Tonghua Liu , Yuting Liu , Shuaibo Geng , Yujie Lian , Zong-Hong Zhu

Gamma ray bursts (GRBs) are short and intense pulses of $\gamma$-rays arriving from random directions in the sky. Several years ago Amelino-Camelia et al. pointed out that a comparison of time of arrival of photons at different energies…

Astrophysics · Physics 2009-11-10 Tsvi Piran

Some models for quantum gravity (QG) violate Lorentz invariance and predict an energy dependence of the speed of light, leading to a dispersion of high-energy gamma-ray signals that travel over cosmological distances. Limits on the…

High Energy Astrophysical Phenomena · Physics 2009-04-21 Robert Wagner

We discuss the prospects for bounding and perhaps even measuring quantum gravity effects on the dispersion of light using the highest energy photons produced in gamma ray bursts measured by the Fermi telescope. These prospects are brigher…

High Energy Astrophysical Phenomena · Physics 2009-10-29 Giovanni Amelino-Camelia , Lee Smolin

Various approaches to quantum gravity suggest the possibility of violation of Lorentz symmetry at very high energies. In these cases we expect a modification at low energies of the dispersion relation of photons that contains extra powers…

Astrophysics · Physics 2015-06-24 Maria Rodriguez Martinez , Tsvi Piran , Yonatan Oren

The Fermi Gamma-Ray Space Telescope has more than doubled the number of Gamma-Ray Bursts (GRBs) detected above 100 MeV within its first year of operation. Thanks to the very wide energy range covered by Fermi's Gamma-ray Burst Monitor (GBM;…

High Energy Astrophysical Phenomena · Physics 2019-08-13 Jonathan Granot

Observations of high energy emission from gamma-ray bursts (GRBs) constrain the extreme physical conditions associated with these energetic cosmic explosions. The Large Area Telescope (LAT) onboard the Fermi Gamma-ray Space Telescope, a…

High Energy Astrophysical Phenomena · Physics 2009-12-17 S. B. Pandey , Carl W. Akerlof , W. Zheng , F. Yuan