Robustness of entanglement in Hawking radiation for optical systems immersed in thermal baths
arXiv:2211.10306 · doi:10.1103/PhysRevD.107.085009
Abstract
Entanglement is the quantum signature of Hawking's particle pair-creation from causal horizons, for gravitational and analog systems alike. Ambient thermal fluctuations, ubiquitous in realistic situations, strongly affects the entanglement generated in the Hawking process, completely extinguishing it when the ambient temperature is comparable to the Hawking temperature. In this work, we show that optical analog systems have a built-in robustness to thermal fluctuations which are at rest in the laboratory. In such systems, horizons move relative to the laboratory frame at velocities close to the speed of light. We find that a subtle interplay between this relative velocity and dispersion protects the Hawking-generated entanglement -- allowing ambient temperatures several orders of magnitude larger than the Hawking temperature without significantly affecting entanglement.
13 + 3 pages, 5 figures. Comments and questions welcome
References in corpus (10)
- Fiber-optical analogue of the event horizon
- Black/White hole radiation from dispersive theories
- Cost of quantum entanglement simplified
- Probing the thermal character of analogue Hawking radiation for shallow water waves?
- Optical analogues of black-hole horizons
- Hawking radiation by Kerr black holes and conformal symmetry
- Stimulating the Quantum Aspects of an Optical Analog White-Black Hole
- Symplectic circuits, entanglement, and stimulated Hawking radiation in analog gravity
- Hawking radiation in optics and beyond
- Hawking temperature in dispersive media: Analytical and numerical study