Entanglement-based Free Space Quantum Cryptography in Daylight Antía Lamas-Linares, Matthew P. Peloso, Ilja Gerhardt, Caleb Ho and Christian Kurtsiefer.

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Presentation transcript:

Entanglement-based Free Space Quantum Cryptography in Daylight Antía Lamas-Linares, Matthew P. Peloso, Ilja Gerhardt, Caleb Ho and Christian Kurtsiefer DAMOP 2009, Charlottesville, VA

Why free space? Why entanglement? Ad hoc setups (travel: 23C3, BlackHat and DEFCON) Does not need preexisting fiber infrastructure Satellites Does not need a high bandwidth source of random numbers (*) Can be used for “device independent” protocols where security does not rely on a trusted measuring box (*) transmitter receiver BBM92 Results APL 89, (2006) raw coincidences sifted coincidences final key

Basic Setup source for photon pairs

Entanglement source “classic” type-II crossed ring configuration, 2 mm BBO, 30mW 71k s -1 and 78k s -1 singles per arm into single mode fibers 12k s -1 detected pairs from 30 mW 407nm into single mode fibers polarization visibility in H/V and 45° basis: 97% and 92% optical bandwidth 8.7 nm FWHM small footprint, works in outdoor conditions (30 degrees, 90% humidity) 19’’ 10’’ Now there are better PDC sources for this purpose. PPKTP sources exhibit much higher rates and narrower spectral features. [Fedrizzi et al, Opt. Express 15, (2007)].

Bright light effects For all detector types -> saturation For actively quenched detectors -> death Passively quenched detectors can survive but relatively quickly saturate Saturation reduces the probability of detecting the “true” pairs Accidental coincidences increase the QBER and can prevent key production Given the dead time of the detectors (1μs) and a coincidence time window essentially fixed by the jitter (~1ns), our only option is to reduce the background seen by the detectors

Spectral filtering: filters matched to PDC source 72% Background reduced by a factor ~100 Signal transmission 57% T=57%

Spatial filtering: pinhole at focus position + baffles + shading and blackout material Φ=30 μm pinhole+shading ~12 dB reduction in background. Signal unaffected. tapered apertures ~3-4 dB reduction in background. Signal unaffected.

Where: Across the sports field at NUS A few more things to note are the antennas (classical comms) and the tripods (passive stability)

Synchronization and time filtering Both sides are synchronized using the intrinsic correlations of the PDC process. An atomic clock is used for ~5 s to get the initial synchronization. Subsequently a feedback loop adjusts the coincidence window to follow the clock drift. Coincidence time window adjusted to the intrinsic jitter of the detectors. Background diminishes linearly with size of coincidence window. Do we NEED atomic clocks? NO, enough information within the PDC signal. Use better algorithms -> We should be able to use standard “bad” computer clocks [NJP 11, (2009)]

Daylight crypto 2 day run singles rate, remote side singles rate, local side raw coincidences sifted coincidences error corrected, privacy amplified key QBER accidental coincidences [NJP 11, (2009)]

Effects of detector saturation raw coincidences QBER

Summary A combination of spectral, spatial and temporal filtering is sufficient to suppress background from sunlight Demonstrated a continuous run of an entanglement based QKD system over several days Atomic clocks should be eliminated by taking full advantage of intrinsic timing info in PDC

Christian KurtsieferAntia Lamas-LinaresValerio ScaraniGleb MaslennikovIlja GerhardtHou Shun Poh Matt Peloso Caleb HoDarwin GosalBrenda ChngTien Tjuen NgSyed Abdullah AljunidJianwei Lee Thanks!