Possible astrophysical probes of quantum gravity

dc.creatorSarkar, Subir
dc.date2002-04-30
dc.date2002-05-03
dc.date.accessioned2026-07-07T10:31:55Z
dc.date.available2026-07-07T10:31:55Z
dc.descriptionA satisfactory theory of quantum gravity will very likely require modification of our classical perception of space-time, perhaps by giving it a 'foamy' structure at scales of order the Planck length. This is expected to modify the propagation of photons and other relativistic particles such as neutrinos, such that they will experience a non-trivial refractive index even in vacuo. The implied spontaneous violation of Lorentz invariance may also result in alterations of kinematical thresholds for key astrophysical processes involving high energy cosmic radiation. We discuss experimental probes of these possible manifestations of the fundamental quantum nature of space-time using observations of distant astrophysical sources such as gamma-ray bursts and active galactic nuclei.
dc.description11 pages, 3 figures (MPL LaTeX style); Invited talk at the ``First IUCAA Meeting on the Interface of Gravitational and Quantum Realms'', Pune, 17-21 December 2001; Changes: Fig.3 now correctly attibuted to Liberati, Jacobson & Mattigly
dc.identifierhttps://arxiv.org/abs/gr-qc/0204092
dc.identifierhttp://arxiv.org/abs/gr-qc/0204092
dc.identifierMod.Phys.Lett.A17:1025-1036,2002
dc.identifierdoi:10.1142/S0217732302007521
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/178585
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectHigh Energy Physics - Theory
dc.titlePossible astrophysical probes of quantum gravity
dc.typetext

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