Schwinger Effect, Hawking Radiation, and Unruh Effect
arXiv:1602.05336 · doi:10.1142/S021827181645005X
Abstract
We revisit the Schwinger effect in de Sitter, anti-de Sitter spaces and charged black holes, and explore the interplay between quantum electrodynamics and the quantum gravity effect at one-loop level. We then advance a thermal interpretation of the Schwinger effect in curved spacetimes. Finally, we show that the Schwinger effect in a near-extremal black hole differs from Hawking radiation of charged particles in a non-extremal black hole and is factorized into those in an anti-de Sitter space and a Rindler space with the surface gravity for acceleration.
Latex 10 pages, no figure; Proceedings for LeCosPA Symposium, National Taiwan University, Dec. 14-18, 2015
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Cited by in corpus (9)
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- Astrophysics in Strong Electromagnetic Fields and Laboratory Astrophysics
- Induced energy-momentum tensor of Dirac field in 2D de Sitter QED
- From Schwinger Balls to Black Holes
- Pair creation in the early universe
- Energy-momentum tensor and effective Lagrangian of scalar QED with a nonminimal coupling in 2D de Sitter spacetime
- Canonical Quantization of the U(1) Gauge Field in the right Rindler-wedge in the Rindler Coordinates
- Canonical Quantization of the U(1) Gauge Field in the Rindler Coordinates