Accelerating Photons with Gravitational Radiation

The nature of superluminal photon propagation in the gravitational field describing radiation from a time-dependent, isolated source (the Bondi-Sachs metric) is considered in an effective theory which includes interactions which violate the strong equivalence principle. Such interactions are, for ex...

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Detalles Bibliográficos
Autor principal: Shore, G.M.
Lenguaje:eng
Publicado: 2000
Materias:
General Relativity and Cosmology
Acceso en línea:https://dx.doi.org/10.1016/S0550-3213(01)00137-7
http://cds.cern.ch/record/481261
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author Shore, G.M.
author_facet Shore, G.M.
author_sort Shore, G.M.
collection CERN
description The nature of superluminal photon propagation in the gravitational field describing radiation from a time-dependent, isolated source (the Bondi-Sachs metric) is considered in an effective theory which includes interactions which violate the strong equivalence principle. Such interactions are, for example, generated by vacuum polarisation in conventional QED in curved spacetime. The relation of the resulting light-cone modifications to the Peeling Theorem for the Bondi-Sachs spacetime is explained.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2000
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spelling cern-4812612023-03-14T17:09:24Zdoi:10.1016/S0550-3213(01)00137-7http://cds.cern.ch/record/481261engShore, G.M.Accelerating Photons with Gravitational RadiationGeneral Relativity and CosmologyThe nature of superluminal photon propagation in the gravitational field describing radiation from a time-dependent, isolated source (the Bondi-Sachs metric) is considered in an effective theory which includes interactions which violate the strong equivalence principle. Such interactions are, for example, generated by vacuum polarisation in conventional QED in curved spacetime. The relation of the resulting light-cone modifications to the Peeling Theorem for the Bondi-Sachs spacetime is explained.The nature of superluminal photon propagation in the gravitational field describing radiation from a time-dependent, isolated source (the Bondi–Sachs metric) is considered in an effective theory which includes interactions which violate the strong equivalence principle. Such interactions are, for example, generated by vacuum polarisation in conventional QED in curved spacetime. The relation of the resulting light-cone modifications to the Peeling Theorem for the Bondi–Sachs spacetime is explained.The nature of superluminal photon propagation in the gravitational field describing radiation from a time-dependent, isolated source (the Bondi-Sachs metric) is considered in an effective theory which includes interactions which violate the strong equivalence principle. Such interactions are, for example, generated by vacuum polarisation in conventional QED in curved spacetime. The relation of the resulting light-cone modifications to the Peeling Theorem for the Bondi-Sachs spacetime is explained.gr-qc/0012063CERN-TH-2000-285SWAT-266UGVA-DPT-00-9-1088CERN-TH-2000-285SWAT-266UGVA-DPT-1088oai:cds.cern.ch:4812612000-12-17
spellingShingle General Relativity and Cosmology
Shore, G.M.
Accelerating Photons with Gravitational Radiation
title Accelerating Photons with Gravitational Radiation
title_full Accelerating Photons with Gravitational Radiation
title_fullStr Accelerating Photons with Gravitational Radiation
title_full_unstemmed Accelerating Photons with Gravitational Radiation
title_short Accelerating Photons with Gravitational Radiation
title_sort accelerating photons with gravitational radiation
topic General Relativity and Cosmology
url https://dx.doi.org/10.1016/S0550-3213(01)00137-7
http://cds.cern.ch/record/481261
work_keys_str_mv AT shoregm acceleratingphotonswithgravitationalradiation

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