2009
DOI: 10.1088/1126-6708/2009/08/089
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The refractive index of curved spacetime II: QED, Penrose limits and black holes

Abstract: This work considers the way that quantum loop effects modify the propagation of light in curved space. The calculation of the refractive index for scalar QED is reviewed and then extended for the first time to QED with spinor particles in the loop. It is shown how, in both cases, the low frequency phase velocity can be greater than c, as found originally by Drummond and Hathrell, but causality is respected in the sense that retarded Green functions vanish outside the lightcone. A "phenomenology" of the refract… Show more

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Cited by 39 publications
(85 citation statements)
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“…As demonstrated in our previous investigations of the realisation of causality in curved spacetime [5][6][7][8][9][10], in order to verify that causality is respected we need to demonstrate that the phase velocity, which may be superluminal for low frequencies, is equal to 1 in the high-frequency limit [5,[11][12][13]. This implies constraints on the phase shift of the photon modes as they scatter from the shockwave.…”
Section: Jhep03(2016)129mentioning
confidence: 99%
See 3 more Smart Citations
“…As demonstrated in our previous investigations of the realisation of causality in curved spacetime [5][6][7][8][9][10], in order to verify that causality is respected we need to demonstrate that the phase velocity, which may be superluminal for low frequencies, is equal to 1 in the high-frequency limit [5,[11][12][13]. This implies constraints on the phase shift of the photon modes as they scatter from the shockwave.…”
Section: Jhep03(2016)129mentioning
confidence: 99%
“…This is technically simpler than its spinor counterpart, although the necessary formalism for the latter is established in [8]. In section 8, we also discuss a super-renormalizable scalar theory, which exhibits interesting differences from QED in its UV behaviour.…”
Section: Jhep03(2016)129mentioning
confidence: 99%
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“…The breakthrough made in a series of papers [8][9][10][11] was to extend the DrummondHathrell result by relaxing the requirement that ω 2 R/m 4 ≪ 1. The result is obtained by calculating the one-loop vacuum polarization due to the Feynman graphs illustrated in Figure 1 in the appropriate limits.…”
Section: Introductionmentioning
confidence: 99%