arXiv · 1712.09524
Soliton Diffusion as a Signature of Hawking Radiation in Bose-Einstein Condensates
Abstract
We propose a scheme to detect analog Hawking radiation (HR) in an atomic Bose-Einstein condensate (BEC) through measuring the diffusion of a dark soliton. The HR is generated by changing the transverse trapping potential of the BEC to obtain a background flow, which is subsonic in downstream and supersonic in upstream, satisfying the condition of black hole horizon. When the system is in thermal equilibrium at Hawking temperature, a dark soliton is created in the upstream. Due to the influence of the HR, the motion of the dark soliton is similar to a Brownian particle and hence exhibits an apparent diffusion, which can be measured and be taken as a signal of the HR. Since the dark soliton is much "heavier" than Hawking quanta, its diffusion is much easier detectable than the Hawking quanta themselves.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Chao Hang, Gregory Gabadadze, Guoxiang Huang. 2019-07-29. Soliton Diffusion as a Signature of Hawking Radiation in Bose-Einstein Condensates. https://doi.org/10.1016/j.physletb.2019.04.008
Cite the original work for its findings. Save a collection to share your selection of sources.