Lorentz invariance violation and γ-ray propagation: Detectability by very-high-energy γ-detectors

Nick E. Mavromatos*

*Corresponding author for this work

Research output: Chapter in Book/Report/Conference proceedingConference paperpeer-review

Abstract

Several models of (quantum) gravity predict tiny violations of Lorentz Invariance (LI) at microscopic (Planckian) scales, which increase with the energy of the probe and amplified with the distance of the source. Thus, astrophysical/cosmological energetic probes provide the best test grounds of LI. The talk reviews the status and prospects of such tests, using high-energy cosmic γ detectors. The Čerenkov Telescope Array (CTA) is an excellent experimental tool for making such tests with sensitivities exceeding those possible using other detectors.

Original languageEnglish
Title of host publication14th Marcel Grossman Meeting On Recent Developments in Theoretical and Experimental General Relativity, Astrophysics and Relativistic Field Theories, Proceedings
EditorsRemo Ruffini, Massimo Bianchi, Remo Ruffini, Robert T Jantzen
PublisherWorld Scientific Publishing Co. Pte Ltd
Pages3219-3227
Number of pages9
ISBN (Electronic)9789813226593
Publication statusPublished - 1 Jan 2018
Event14th Marcel Grossman Meeting On Recent Developments in Theoretical and Experimental General Relativity, Astrophysics and Relativistic Field Theories - Rome, Italy
Duration: 12 Jul 201518 Jul 2015

Conference

Conference14th Marcel Grossman Meeting On Recent Developments in Theoretical and Experimental General Relativity, Astrophysics and Relativistic Field Theories
Country/TerritoryItaly
CityRome
Period12/07/201518/07/2015

Keywords

  • Gamma-ray detectors
  • High energy astrophysics
  • Lorentz invariance violation

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