Abstract
By etching a hole in the mirrors or by placing a scatterer in the center of a cavity, we can create a sink for light. In a Bose-Einstein condensate of photons this sink results in the creation of a so-called radial vortex, which is a two-dimensional analog of a Schwarzschild black hole. We theoretically investigate the Hawking radiation and the associated graybody factor of this Schwarzschild black hole. In particular, we determine the density-density and velocity-velocity correlation functions of the Hawking radiation, which can be measured by observing the spatial correlations in the fluctuations in the light emitted by the cavity.
| Original language | English |
|---|---|
| Article number | 023850 |
| Number of pages | 6 |
| Journal | Physical Review A |
| Volume | 99 |
| Issue number | 2 |
| DOIs | |
| Publication status | Published - 25 Feb 2019 |
Funding
We thank Govert Nijs, Nick Plantz, and Stefan Vandoren for helpful discussions. This work is supported by the China Scholarship Council (CSC), the Stichting voor Fundamenteel Onderzoek der Materie (FOM), and is part of the D-ITP consortium, a program of the Netherlands Organization for Scientific Research (NWO) that is funded by the Dutch Ministry of Education, Culture and Science (OCW).
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