Intrinsic instability of sonic white holes
U. Leonhardt, T. Kiss, P. Ohberg

TL;DR
This paper demonstrates that sonic white holes in Bose-Einstein condensates inherently possess a discrete spectrum of instabilities, unaffected by high-energy physics analogues, challenging their stability and potential as black hole models.
Contribution
It reveals the intrinsic instability spectrum of sonic white holes, independent of trans-Planckian physics, providing new insights into analogue gravity systems.
Findings
Sonic white holes exhibit a discrete instability spectrum.
Instability spectrum is insensitive to trans-Planckian physics.
Implications for the stability of analogue black hole models.
Abstract
Artificial black holes, such as sonic holes in Bose-Einstein condensates, may give insights into the role of the physics at the event horizon beyond the Planck scale. We show that sonic white holes give rise to a discrete spectrum of instabilities that is insensitive to the analogue of trans-Planckian physics for Bose-Einstein condensates.
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Taxonomy
TopicsFluid Dynamics and Turbulent Flows · Fluid Dynamics and Thin Films
