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Sensitivity of Astrophysical Observations to Gravity-Induced Wave Dispersion in Vacuo

We discuss possible signatures of quantum gravity for the propagation of light, including an energy-dependent velocity (refractive index), dispersion in velocity at a given energy, and birefringence. We also compare the sensitivities of different astrophysical observations, including BATSE data on G...

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Detalles Bibliográficos
Autores principales: Amelino-Camelia, G., Ellis, John R., Mavromatos, N.E., Nanopoulos, Dimitri V., Sarkar, Subir
Lenguaje:eng
Publicado: 1998
Materias:
Acceso en línea:http://cds.cern.ch/record/369506
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author Amelino-Camelia, G.
Ellis, John R.
Mavromatos, N.E.
Nanopoulos, Dimitri V.
Sarkar, Subir
author_facet Amelino-Camelia, G.
Ellis, John R.
Mavromatos, N.E.
Nanopoulos, Dimitri V.
Sarkar, Subir
author_sort Amelino-Camelia, G.
collection CERN
description We discuss possible signatures of quantum gravity for the propagation of light, including an energy-dependent velocity (refractive index), dispersion in velocity at a given energy, and birefringence. We also compare the sensitivities of different astrophysical observations, including BATSE data on GRB 920229, BeppoSAX data on GRB 980425, the possible HEGRA observation of GRB 920925c, and Whipple observations of the active galaxy Mrk 421. Finally, we discuss the prospective sensitivities of AMS and GLAST.
id cern-369506
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 1998
record_format invenio
spelling cern-3695062023-03-14T18:07:59Zhttp://cds.cern.ch/record/369506engAmelino-Camelia, G.Ellis, John R.Mavromatos, N.E.Nanopoulos, Dimitri V.Sarkar, SubirSensitivity of Astrophysical Observations to Gravity-Induced Wave Dispersion in VacuoAstrophysics and AstronomyWe discuss possible signatures of quantum gravity for the propagation of light, including an energy-dependent velocity (refractive index), dispersion in velocity at a given energy, and birefringence. We also compare the sensitivities of different astrophysical observations, including BATSE data on GRB 920229, BeppoSAX data on GRB 980425, the possible HEGRA observation of GRB 920925c, and Whipple observations of the active galaxy Mrk 421. Finally, we discuss the prospective sensitivities of AMS and GLAST.We discuss possible signatures of quantum gravity for the propagation of light, including an energy-dependent velocity (refractive index), dispersion in velocity at a given energy, and birefringence. We also compare the sensitivities of different astrophysical observations, including BATSE data on GRB 920229, BeppoSAX data on GRB 980425, the possible HEGRA observation of GRB 920925c, and Whipple observations of the active galaxy Mrk 421. Finally, we discuss the prospective sensitivities of AMS and GLAST.astro-ph/9810483ACT-10-98CTP-TAMU-40-98NEIP-98-014CERN-TH-98-342ACT-1998-10CTP-TAMU-98-40NEIP-98-014oai:cds.cern.ch:3695061998-10-30
spellingShingle Astrophysics and Astronomy
Amelino-Camelia, G.
Ellis, John R.
Mavromatos, N.E.
Nanopoulos, Dimitri V.
Sarkar, Subir
Sensitivity of Astrophysical Observations to Gravity-Induced Wave Dispersion in Vacuo
title Sensitivity of Astrophysical Observations to Gravity-Induced Wave Dispersion in Vacuo
title_full Sensitivity of Astrophysical Observations to Gravity-Induced Wave Dispersion in Vacuo
title_fullStr Sensitivity of Astrophysical Observations to Gravity-Induced Wave Dispersion in Vacuo
title_full_unstemmed Sensitivity of Astrophysical Observations to Gravity-Induced Wave Dispersion in Vacuo
title_short Sensitivity of Astrophysical Observations to Gravity-Induced Wave Dispersion in Vacuo
title_sort sensitivity of astrophysical observations to gravity-induced wave dispersion in vacuo
topic Astrophysics and Astronomy
url http://cds.cern.ch/record/369506
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