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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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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 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.
College: Faculty of Science and Engineering
Issue: 1-3
Start Page: 455
End Page: 466