Homodyne detection

Introduction

Optical homodyne detection is a method for detecting messages transmitted in optical signals, where a frequency or phase modulated signal is compared to what is misleadingly called the "local oscillator" (LO) signal, which is generated from the same source but not modulated with the message. In order to probe quantum effects, it is important to bring the noise of the detector down to the shot-noise limit, where the only fluctuations observed arise from the discrete nature of photons, which can be theoretically modelled as the vacuum-state fluctuations of the quantised electromagnetic field. This project's first objective is to build a homodyne detector from scratch.

Lab Location: S11-02-04 (Optics Lab)

Application: Continuous-variable QKD with Gaussian modulation and coherent states

While the first protocols for quantum key distribution (QKD) involved discrete variables (DV) in finite, small dimensions, QKD can also be done using continuous variables (CV) in infinite dimensions, i.e. the state of an electromagnetic field. Using Gaussian modulation and coherent states makes the QKD system relatively easy to implement and analyse, although getting positive key rates is a different matter. The homodyne detector is an essential component of this setup, but if we have the capacity, we can try to develop other parts of the system, such as the implementation of the QKD protocol itself in software. We want to pay particular attention to the design of the amplifier for the homodyne detector, for which there are stringent requirements and difficult tradeoffs to make.

Reality

What we actually ended up working towards is a simple version of the system proposed above. Instead of building a system capable of sending useful information, we aimed for the simpler objective of just being able to produce some kind of phase modulation. This is a stepping stone towards a full-blown optical communication system, where digital data is modulated onto the laser by a computer and read off from the results of the homodyne detection.

Background Reading

Our primary source of background information is Lasers and Electro-Optics, available for download via NUS Library. The relevant chapters are:

• Chapter 5 Laser Radiation, discussing the basic background on lasers
• Chapter 18 The Electro-optic and Acousto-optic Effects and Modulation of Light Beams, discussing how modulation can be achieved
• Chapter 21 Detection of Optical Radiation, discusses noise in detectors and the process of homodyne detection

For DV-QKD theorists who stumbled into this (like me), here's some background reading on CV-QKD:

• Review of Gaussian quantum-information processing
• Self-contained tutorial on theory of Gaussian-modulated CV-QKD

Tragically, we were nowhere close to being able to use the material on CV-QKD, but we leave the references here for posterity.

Theory

Phase Modulation

The next question is how to vary $\delta$ in an easily controllable manner. TODO

Talk about LiNbO3 structure, birefringence, electro-optic effect

Noise

Finally, we have to control for the effect of noise in our experiment. There are four primary sources of noise in semiconductor photodetectors:

• Shot noise, or quantum noise, arising from the quantisation of light: because the light must arrive at the detector one photon at a time, there will be some fluctuation in the signal read at any point in time.
• Nyquist-Johnson noise or thermal noise, arising from thermal fluctuations in the electronics.
• $1/f$ noise, which is apparently a very mysterious and universal phenomenon caused by various different factors, but has a power spectral density proportional to $1/f$, hence the name.
• Generation-recombination (GR) noise, caused by holes and electrons randomly being generated and recombining in the semiconductor.

$\Delta f$ is the sampling bandwidth, related to how often we take electrical measurements. By Nyquist's theorem, we must have a sampling period $T=1/\Delta f\leq 1/2f$ to reconstruct a modulated signal of maximum frequency component $f$: that is, we must have $\Delta f\geq 2f$.

Setup & Methodology

Full setup of Michelson interferometer with ${\ce {LiNbO3}}$ crystal.

Homodyne Detection Setup

The overview for the initially intended experiment is:

1. Split the laser beam into two, one component will be LO and another will be the signal
2. Frequency-shift the signal beam using an acousto-optical modulator (AOM)
3. Phase-modulate the signal beam using an electro-optical modulator (EOM). This is typically a ${\ce {LiNbO3}}$ crystal, whose birefringence is controlled by the voltage applied to it. For more advanced applications, we can use a transformer to amplify a small change in voltage into a large difference, producing a large change in the birefringence.
4. Recombine the signal and the LO in a 50:50 beam splitter
5. Send the two output beams to two reverse-biased photodiodes, and connect the junction between the photodiodes to a current detector to convert it to a voltage. The signal will be modulated according to the beat frequency.

The noise in the photodiodes tends to be low frequency, so aiming for a signal of frequency $10~\mathrm {MHz}$ or so will make it easier to remove the noise without affecting the signal.

Actual Setup

As the theory section indicates, we are constructing a Michelson interferometer with a ${\ce {LiNbO3}}$ crystal on one arm, serving as a voltage-controlled phase modulator. The voltage across the crystal controls the refractive index, which changes the path difference $\delta$ and therefore the phase difference. If the fringes are circular, the total intensity on the photodiode will vary significantly as the phase changes. This can be read off by using the photodiode as a current source and measuring the voltage it induces across a resistor.

A high-level overview is as follows:

1. Modify and wire up all battery-powered equipment (detectors and laser pointer) to use benchtop power supplies instead, and mount them on optical posts
2. Align the laser to ensure it is parallel to the table and its grid
3. Align the beam splitter to the grid of the table and the laser
4. Align the mirrors to produce circular fringes
5. Place and align the crystal so the beam passes through it
6. Align the lens to magnify the interference pattern, and align the photodiode so that it coincides with the pattern

Mounting and Wiring Components

In order to provide a consistent voltage throughout, and to avoid the hassle of changing batteries when they are depleted, it is advantageous to power devices using benchtop power supplies instead of batteries, whose output voltage will vary over the course of the experiment. We converted a laser pointer, powered by 3 1.5V batteries in series, and a photodiode, powered by a 9V battery, to do so.

The photodiode was easy to convert, since the terminals of the photodiode were connected to screw terminals. It was a simple matter to open the terminals, remove the wires connected to the battery, and insert new wires that were connected via crocodile clips to a benchtop power supply.

TODO insert photo of converted photodiode

The laser pointer was much more difficult to work with. When using batteries, the negative terminal of the batteries would be connected to the spring inside the laser pointer, while the positive terminal would be in electrical contact with the inside of the body of the laser pointer. A insulating sheath prevents short circuits.

TODO insert labelled photo of inside of laser pointer

To connect the laser pointer to the benchtop power supply, the two contacts had to be replaced with crocodile clips, connected to the benchtop power supply. However, most clips were too large to fit inside the laser pointer body, and those that did fit were very difficult to manipulate due to taking up most of the volume of the body. Additionally, the clips had to be insulated to prevent them from forming a short circuit, since they were placed very close to each other.

The correctly-sized crocodile clips and rubber sleeves were found scattered throughout the lab, and we had to perform a simple improvised crimp to attach wires to the clips. Lastly, we used a pair of cutters to cut the body of the laser pointer to expose the coil within, so the crocodile clips could be attached. We were careful to preserve the insulating sheath, to ensure the circuit could be formed properly.

TODO insert photo of final laser setup

The EOM Board

TODO talk about repairing it, soldering issues etc.

The EOM board is difficult to align properly. The solder mounds on the underside of the board make it difficult to seat the board firmly on the optical mount, while the tension in the coaxial cable used to supply the voltage also makes the system very unstable. Initial attempts to fix the position of the board by pressing it down with a wedge met some success, but it was still too prone to being misaligned while the setup was being adjusted.

Fortunately, the holes in the board are, by coincidence, mostly aligned with the holes in the mount. Although the mount uses imperial-sized screws, we were able to find the screws and components necessary to fix the board in place securely, producing the rather ugly assemblage pictured below.

TODO insert picture

We have also elected to place the board on a mount permitting the pitch and roll of the board to be adjusted, because it is difficult to guarantee its alignment otherwise, and since the crystal is birefringent, we want to ensure it is aligned with the polarisation of the laser, so that the whole beam will experience the same phase difference, and the fringe visibility can be maximised.

Results & Discussion

Equipment Parameters

We are using a Hamamatsu S5106 Si PIN photodiode as our detector, with a resistive load of $1~\mathrm {M\Omega }$. Measurements are taken with a Kenwood CS-5270 oscilloscope with $\Delta f=100~\mathrm {MHz}$.