Hawking radiation on a falling lattice
Ted Jacobson, David Mattingly

TL;DR
This paper investigates Hawking radiation using a falling lattice model in 1+1 dimensions, demonstrating that the effect can be accurately simulated with a discretized scalar field theory through both analytical and numerical methods.
Contribution
It introduces a lattice falling into a black hole to model Hawking radiation, showing the effect arises from mode mixing analogous to Bloch oscillations, with high accuracy.
Findings
Hawking radiation is reproduced within 0.5% accuracy on a properly spaced lattice.
Outgoing modes originate from incoming modes via a process similar to Bloch oscillations.
Numerical results confirm the theoretical predictions of mode mixing and Hawking radiation emergence.
Abstract
Scalar field theory on a lattice falling freely into a 1+1 dimensional black hole is studied using both WKB and numerical approaches. The outgoing modes are shown to arise from incoming modes by a process analogous to a Bloch oscillation, with an admixture of negative frequency modes corresponding to the Hawking radiation. Numerical calculations show that the Hawking effect is reproduced to within 0.5% on a lattice whose proper spacing where the wavepacket turns around at the horizon is in units where the surface gravity is 1.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
