Sub-ns timing accuracy for satellite quantum communications
arXiv:1902.07126 · doi:10.1364/JOSAB.36.000B59
Abstract
Satellite quantum communications have rapidly evolved in the past few years, culminating in the proposal, development, and deployment of satellite missions dedicated to quantum key distribution and the realization of fundamental tests of quantum mechanics in space. However, in comparison with the more mature technology based on fiber optics, several challenges are still open, such as the capability of detecting, with high temporal accuracy, single photons coming from orbiting terminals. Satellite laser ranging, commonly used to estimate satellite distance, could also be exploited to overcome this challenge. For example, high repetition rates and a low background noise can be obtained by determining the time-of-flight of faint laser pulses that are retro-reflected by geodynamics satellites and then detected on Earth at the single-photon level. Here we report an experiment with regard to achieving a temporal accuracy of approximately 230 ps in the detection of an optical signal of few photons per pulse reflected by satellites in medium Earth orbit, at a distance exceeding 7500 km, by using commercially available detectors. Lastly, the performance of the Matera Laser Ranging Observatory is evaluated in terms of the detection rate and the signal-to-noise ratio for satellite quantum communications.
7 pages, 4 figures, part of the "QUANTUM KEY DISTRIBUTION AND BEYOND" featured issue of the Journal of the Optical Society of America B
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Cited by in corpus (7)
- Advances in Space Quantum Communications
- The Deep Space Quantum Link: Prospective Fundamental Physics Experiments using Long-Baseline Quantum Optics
- Simulation of Silicon Waveguide Single-Photon Avalanche Detectors for Integrated Quantum Photonics
- Spacetime effects on wavepackets of coherent light
- Synchronization of quantum communication over an optical classical communication channel
- Introduction to gravitational redshift of quantum photons propagating in curved spacetime
- Proposal for an optical interferometric measurement of the gravitational red-shift with satellite systems