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Tunnelling amplitudes and Hawking radiation from worldline QFT

2025/08/01 by Anton Ilderton, Ilderton, Anton, Karthik Rajeev +1 · 9 citations
Physics and Astronomy · #Amplitude #Black Holes and Theoretical Physics #FOS: Physical sciences #General Relativity and Quantum Cosmology (gr-qc) #Hawking #Hawking radiation #High Energy Physics - Theory (hep-th) #Horizon #Noncommutative and Quantum Gravity Theories #Path integral formulation #Quantum Electrodynamics and Casimir Effect #Quantum field theory in curved spacetime #Quantum tunnelling #Saddle #Spacetime

paper · pdf · doi:10.48550/arxiv.2508.00997

published in arXiv (Cornell University) (Cornell University)

openalex publication_date 2025/08/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

We compare Hawking radiation in a collapse background with Schwinger pair creation in an electric field. The comparison is driven by the presence of an analogue horizon in the Schwinger case, which causally divides spacetime for classical particles, but through which quantum fields can tunnel. Amplitudes for tunnelling processes are encoded in the asymptotic behaviour of solutions to the appropriate background-coupled wave equation. We construct these solutions, in both gravity and QED, using the worldline approach, where tunnelling and particle creation manifest as complex saddle points of a real-time path integral. For the Schwinger effect, these saddles correspond to complex worldlines, while for Hawking radiation, the corresponding worldlines are real, but appear complex when extended beyond a certain coordinate patch.

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