How to count single photons at room temperature, and how to keep a quantum key secret in open air.
Those are the two questions. This is a programme, not a body of results: we have
reviewed the literature, written a test plan, and proposed an architecture. Nothing
has been fabricated or measured yet, and we will publish results when there are some.
Literature reviews
3
internal, not peer-reviewed
Experiments planned
1
48 conditions, not yet run
Architectures proposed
1
source, circuit, detector
Results published
0
we will say when that changes
§ 01
Counting photons without cooling
Quantum communication sends information one photon at a time, mostly at telecom
wavelengths where optical fibre loses least. The best single-photon detectors work
there only when cooled. A detector is blind to light past its material's cutoff, so
the choice of material decides what it can count at all.
Fig. 1.1 What each material can see Literature
A semiconductor absorbs only photons with more energy than its band gap, so it is
blind beyond λc = hc / Eg ≈ 1240 nm·eV / Eg.
Band gaps are approximate room-temperature values. Silicon stops near 1107 nm and
cannot see either telecom band; germanium's line uses its indirect gap, and its
absorption fades well before that (its direct gap, about 0.80 eV, sits near
1550 nm). The two perovskites absorb in the visible, which is why our proposal
uses them as a photon source and pairs them with plasmonic structures to
detect.
Fig. 1.2 Interference is the computation LiteratureI(x) ∝ cos²(πdx/λL) · sinc²(πax/λL), two-slit
interference after Young (1807), computed for d ≈ 4.4a. On a photonic chip the same
effect, inside a Mach–Zehnder interferometer, is what turns paths of light into
logic.
What the reviews concluded
Our reviews looked at room-temperature options: silicon and germanium–silicon
avalanche photodiodes, perovskite quantum dots, plasmonic enhancement, and
two-dimensional materials.
One finding shaped everything after it: for graphene and twisted two-dimensional
materials, single-photon detection has so far been shown only at cryogenic
temperatures. Room temperature is the open part of the problem, and the reason
for the experiment below.
§ 02
Keys made of light, in weather
Quantum key distribution lets two parties agree a secret key whose security rests on
physics: measuring a photon disturbs it, so an eavesdropper leaves errors behind.
Over a free-space link the enemy is also the sky. Fog, haze and rain scatter the
photons the key is made of.
Fig. 2.1 BB84, ten photons Conceptual
The protocol of Bennett and Brassard (1984). Alice encodes each bit as a polarisation
in one of two bases, + or ×; Bob measures in a basis of his own. Afterwards they
compare bases, never bits, in public, and keep only the positions where they matched.
They then check a sample for errors; too many, and they assume someone was listening
and throw the key away. An example sequence, not a run.
Fig. 2.2 What fog does to a free-space link Literature
The Kim model (Kim, McArthur and Korevaar, 2001):
α = (3.91 / V) · (λ / 550 nm)−q per km for visibility
V, with q falling to zero in dense fog. Computed here for 1550 nm and
850 nm. In clear air a link loses well under 1 dB per kilometre; in dense fog it
loses hundreds, and choosing a longer wavelength no longer helps. Simulations of
BB84 over such channels have been published, for example Atieh, Raytchev and
Buhari (2023); that work is theirs, not ours.
§ 03
The experiment we have planned
Perovskites detect light well and degrade quickly: heat, moisture and light itself
break them down. Before any perovskite detector is worth building, we want to know
which combination survives. The plan is written; none of it has been run.
Fig. 3.1 48 conditions, all empty Planned
A full factorial design: three perovskites, four surface passivations and four
encapsulations. With six device and three glass replicates per condition, 432
samples. Results will be analysed by three-way ANOVA. Every cell is empty because
none has been made.
How each sample would be stressed
Damp heat at 85 °C and 85% relative humidity
Light soaking at 1 sun and 5 suns
Thermal cycling between −40 °C and 85 °C
Up to 1,000 hours under test
What counts as passing
At least 70% of responsivity kept after 168 hours of damp heat
T80 beyond 1,000 hours at 1 sun and 65 °C
At least 85% kept after 200 thermal cycles
Dark current rising less than tenfold
Gates set in advance, so the result cannot choose its own bar.
§ 04
An architecture we have proposed
If the materials hold up, the long aim is one chip that makes single photons,
processes them by interference, and counts them, all at room temperature. It is a
design with targets, not a device.
Fig. 4.1 Source, circuit, detector Planned
A perovskite quantum-dot source of single photons, a silicon-photonic circuit of
Mach–Zehnder interferometers, and a perovskite–plasmonic detector. Proposed in our
own strategy report; not fabricated.
Phase 1 Planned
Targets, not results · 1–2 years
A single-photon source with g(2)(0) below 0.1
Gate fidelity above 95%
Detector dark counts below 100 per second per mm²
Phase 2 Planned
Targets, not results · 3–5 years
A small processor of 4 to 8 photonic qubits
Elsewhere at Heliosync Research
Where this meets the digital human
A photonic reservoir to process timing-sensitive signals such as voice prosody, proposed for Shanaya
Reading
Young, T. A Course of Lectures on Natural Philosophy and the Mechanical Arts. London, 1807.
Bennett, C. H. and Brassard, G. Quantum cryptography: public key distribution and coin tossing. Proceedings of the IEEE International Conference on Computers, Systems and Signal Processing, Bangalore, 1984.
Kim, I. I., McArthur, B. and Korevaar, E. Comparison of laser beam propagation at 785 nm and 1550 nm in fog and haze for optical wireless communications. Proc. SPIE 4214, 2001.
Atieh, A., Raytchev, M. and Buhari, A. QKD over FSO under different weather conditions using OptiSystem software. Photonics North, IEEE, 2023. doi:10.1109/PN58661.2023.10223140
Our own reviews, test plan and proposal are internal working documents and are not published here.
Have a lab, a fab or a better idea?
The experiment needs one. We would like to hear from you.