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A particularly simple Lorentz-violating modification of the Maxwell theory of photons maintains gauge invariance, CPT, and renormalization. This modified-Maxwell theory, coupled to standard Dirac particles, involves nineteen dimensionless…

High Energy Physics - Phenomenology · Physics 2008-11-26 F. R. Klinkhamer , M. Risse

The aim of this brief review is to present a case study of how astrophysics data can be used to get bounds on Lorentz-violating parameters. For this purpose, a particularly simple Lorentz-violating modification of the Maxwell theory of…

High Energy Physics - Phenomenology · Physics 2008-10-14 F. R. Klinkhamer

Present and future ultra-high-energy-cosmic-ray facilities (e.g., the South and North components of the Pierre Auger Observatory) and TeV-gamma-ray telescope arrays (e.g., HESS and CTA) have the potential to set stringent bounds on the nine…

High Energy Physics - Phenomenology · Physics 2010-12-23 F. R. Klinkhamer

This article reviews the methods used to obtain a two-sided bound on isotropic modified Maxwell theory from experimental data of ultra high-energy cosmic rays in 2008. The bound is updated with results from the HEGRA experiment.

High Energy Physics - Phenomenology · Physics 2017-08-23 M. Schreck

Present and future ultra-high-energy-cosmic-ray facilities (e.g., the Pierre Auger Observatory with South and North components) and TeV-gamma-ray telescope arrays (e.g., HESS or VERITAS and CTA) have the potential to set stringent indirect…

High Energy Physics - Phenomenology · Physics 2011-06-30 F. R. Klinkhamer

Up to date, there is no consensus regarding the origin of ultra-high energy cosmic rays (UHECR) beyond the Greisen--Zatsepin--Kuzmin (GZK) limit. In order for these UHECRs to reach the Earth, an extremely suppressed interaction between them…

High Energy Astrophysical Phenomena · Physics 2017-10-12 Oscar Castillo-Felisola , Cristobal Corral , Piotr Homola , Jilberto Zamora-Saa

A detailed analysis of vacuum Cherenkov radiation in spacelike Maxwell-Chern-Simons (MCS) theory is presented. A semiclassical treatment reproduces the leading terms of the tree-level result from quantum field theory. Moreover, certain…

High Energy Physics - Theory · Physics 2008-11-26 C. Kaufhold , F. R. Klinkhamer

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

Cosmic-rays with energies exceeding 10^{19} eV are referred to as Ultra High Energy Cosmic Rays (UHECRs). The sources of these particles and their acceleration mechanism are unknown, and for many years have been the issue of much debate.…

High Energy Astrophysical Phenomena · Physics 2015-03-17 E. Waxman

There is a unique Lorentz-violating modification of the Maxwell theory of photons, which maintains gauge invariance, CPT, and renormalizability. Restricting the modified-Maxwell theory to the isotropic sector and adding a standard…

High Energy Physics - Phenomenology · Physics 2010-04-21 F. R. Klinkhamer , M. Schreck

Ultra-high cosmic rays (UHECRs) with energies >10^19 eV emitted at cosmological distances will be attenuated by cosmic microwave and infrared background radiation through photohadronic processes. Lower energy extra-galactic cosmic rays…

High Energy Astrophysical Phenomena · Physics 2011-07-25 Xiang-Yu Wang , Ruo-Yu Liu , Felix Aharonian

The Lorentz-violating isotropic modified Maxwell theory minimally coupled to standard Dirac theory is characterized by a single real dimensionless parameter which is taken to vanish for the case of the standard (Lorentz-invariant) theory. A…

High Energy Physics - Theory · Physics 2011-04-05 F. R. Klinkhamer , M. Schreck

While several arguments can be proposed against the existence of particles with energy in excess of $(3-5)\times 10^{19}$ eV in the cosmic ray spectrum, these particles are actually observed and their origin seeks for an explanation. After…

Astrophysics · Physics 2007-05-23 Pasquale Blasi

We consider the astrophysical implications of the diffusion equation solution for Ultra-High Energy Cosmic Rays (UHECR) in the expanding universe, obtained in paper I (V.Berezinsky & A.Gazizov, ApJ 643 (2006) 8). The UHECR spectra are…

Astrophysics · Physics 2009-03-19 V. Berezinsky , A. Z. Gazizov

Ultra High Energy Cosmic Rays, UHECR, are charged particles with energies between $\sim10^{18}\,{\rm eV}$ and $\sim3\times10^{20}\,{\rm eV}\sim50\,{\rm J}$. They exhibit fundamental physics at energies inaccessible to terrestrial…

High Energy Astrophysical Phenomena · Physics 2025-05-29 Noémie Globus , Roger Blandford

Ultra-High-Energy Cosmic Rays (UHECRs), particles characterized by energies exceeding $10^{18}$ eV, are generally believed to be accelerated electromagnetically in high-energy astrophysical sources. One promising mechanism of UHECR…

High Energy Astrophysical Phenomena · Physics 2024-12-10 Luca Comisso , Glennys R. Farrar , Marco S. Muzio

Using the propagation of ultra high energy nucleons, photons and electrons in the universal radiation backgrounds, we obtain limits on the luminosity of topological defects scenarios for the origin of the highest energy cosmic rays. The…

Astrophysics · Physics 2011-05-12 R. J. Protheroe , Todor Stanev

In this paper, upper limits on the total luminosity of ultra-high-energy cosmic rays (UHECR) (E > $10^{18}$ eV) are determined for five individual sources. The upper limit on the integral flux of GeV-TeV gamma-rays of a given source is used…

High Energy Astrophysical Phenomena · Physics 2014-07-25 R. C. Anjos , V. de Souza , D. A. Supanitsky

Cosmic rays and air showers at ultra-high energy are unique tools to test the validity of Lorentz invariance. A brief overview is given on such tests focusing on isotropic, non-birefringent Lorentz violation (LV) in the photon sector. Based…

High Energy Physics - Phenomenology · Physics 2022-08-19 Markus Risse

Ultra high energy cosmic rays (UHECRs) probably originate in extreme conditions in which extra dimension effects might be important. In this paper we calculate the correction in black hole accretion mechanisms due to extra dimension effects…

High Energy Physics - Theory · Physics 2016-03-16 Rita C. Anjos , Carlos H. Coimbra-Araújo , Roldao da Rocha , Vitor de Souza
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