Low-energy electromagnetic radiation as an indirect probe of black-hole evaporation
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Publication:347563
DOI10.1016/j.nuclphysb.2016.09.011zbMath1349.83045arXiv1602.01475OpenAlexW2279451812MaRDI QIDQ347563
Publication date: 30 November 2016
Published in: Nuclear Physics. B (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1602.01475
Black holes (83C57) Feynman diagrams (81T18) Methods of quantum field theory in general relativity and gravitational theory (83C47) Lasers, masers, optical bistability, nonlinear optics (78A60)
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Cites Work
- Effective photon mass from black-hole formation
- Faster-than-\(c\) signals, special relativity, and causality
- The refractive index of curved spacetime: The fate of causality in QED
- Faster than light photons in gravitational fields. II: Dispersion and vacuum polarisation
- A local effective action for photon-gravity interactions
- ``Faster than light photons in gravitational fields - causality, anomalies and horizons
- Superluminality and UV completion
- Physical Foundations of Cosmology
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