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Journal article 988 views

Accelerating photons with gravitational radiation

Graham Shore

Nucl. Phys. B, Volume: 605, Issue: 1-3, Pages: 455 - 466

Swansea University Author: Graham Shore

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DOI (Published version): 10.1016/S0550-3213(01)00137-7

Abstract

The nature of superluminal photon propagation in the gravitational field describing radi- ation 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...

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Published in: Nucl. Phys. B
Published: 2001
Online Access: http://arxiv.org/abs/gr-qc/0012063
URI: https://cronfa.swan.ac.uk/Record/cronfa17521
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first_indexed 2014-03-22T02:30:09Z
last_indexed 2018-02-09T04:51:13Z
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spelling 2014-03-21T16:08:34.9121998 v2 17521 2014-03-21 Accelerating photons with gravitational radiation 28a24f55687c82d6f3ee378ead3cf234 Graham Shore Graham Shore true false 2014-03-21 FGSEN The nature of superluminal photon propagation in the gravitational field describing radi- ation 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. Journal Article Nucl. Phys. B 605 1-3 455 466 2 7 2001 2001-07-02 10.1016/S0550-3213(01)00137-7 http://arxiv.org/abs/gr-qc/0012063 COLLEGE NANME Science and Engineering - Faculty COLLEGE CODE FGSEN Swansea University 2014-03-21T16:08:34.9121998 2014-03-21T15:31:11.6029214 Faculty of Science and Engineering School of Biosciences, Geography and Physics - Physics Graham Shore 1
title Accelerating photons with gravitational radiation
spellingShingle Accelerating photons with gravitational radiation
Graham Shore
title_short 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_sort Accelerating photons with gravitational radiation
author_id_str_mv 28a24f55687c82d6f3ee378ead3cf234
author_id_fullname_str_mv 28a24f55687c82d6f3ee378ead3cf234_***_Graham Shore
author Graham Shore
author2 Graham Shore
format Journal article
container_title Nucl. Phys. B
container_volume 605
container_issue 1-3
container_start_page 455
publishDate 2001
institution Swansea University
doi_str_mv 10.1016/S0550-3213(01)00137-7
college_str Faculty of Science and Engineering
hierarchytype
hierarchy_top_id facultyofscienceandengineering
hierarchy_top_title Faculty of Science and Engineering
hierarchy_parent_id facultyofscienceandengineering
hierarchy_parent_title Faculty of Science and Engineering
department_str School of Biosciences, Geography and Physics - Physics{{{_:::_}}}Faculty of Science and Engineering{{{_:::_}}}School of Biosciences, Geography and Physics - Physics
url http://arxiv.org/abs/gr-qc/0012063
document_store_str 0
active_str 0
description The nature of superluminal photon propagation in the gravitational field describing radi- ation 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.
published_date 2001-07-02T03:20:14Z
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score 11.013148

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