A list of papers can be found at here. The following portfolio is a summary of some of my favourite projects, it is certainly not an exhaustive list. It is split into the following sections for ease.
- Experimental & Instrumentation
- Computational Modeling & Programming
- Public Talks, Engagement & Outreach
Last Updated: 26th March 2019 - Added TEDx talk.
Experimental & Instrumentation
Since lasers are beams of light, very far from the centre of the
beam the intensity of the field goes to zero (no light).
Previous research tells us that far from any scattering
source (air molecules, edges, etc), this intensity must vary
smoothly. As a result, only certain spatial patterns of laser
are possible, these are called
spatial modes and some are shown right. The typical image of a
laser (known as the TEM00, HG00 or fundamental mode) is shown
For a given laser, there are unique sets of spatial modes that the laser can support. If there is light present in several of these modes, new patterns can emerge from interference.
Unfortunately, from a given intensity pattern, it is difficult to work out which modes are present. In this project, I am working to improve sensors that can directly read out the modal content of a given laser.
In cold atom instruments such as,
very stable lasers are used to move electrons in the cold
sample of atoms between different
atomic energy levels.
The frequency of these lasers is stabilized with an
As the temperature of this cavity rises, it will expand due to
and so the frequency of light which resonates in this cavity
will change, causing the laser to drift away from the resonances
in the atoms.
Usually an analogue temperature control system is used, however, very sensitive devices require multiple layers of temperature control. I designed a digital temperature controller using an Arduino and some additional custom electronics. This allowed each layer to communicate, achieving more stable control. An Arduino was chosen because it is a friendly system for future users to work with. Stability of (3 ± 1)mK was obtained for an open system, with breadboard design.
See my report and code.
Computational Modeling & Programming
In an Atomic interferometer, a cloud of atoms is prepared in a common electronic state. Lasers are then used to put the atoms in a 50:50 quantum superposition of states. By interfering these states with each other, it is possible to make statements about the fields encountered by the atoms on their paths. Unfortunately, the lasers carry some noise. Optical cavities have been proposed to address some of these noise issues. This could promise significant advances for both gravitational wave detectors and portable atom interferometers.
In this work, I developed a computational model of atoms interacting with a generic time domain laser field. I developed the model for Raman interactions and verified it against known test cases, chose a suitable integration routine and characterized the errors. We found that for reasonable choices of parameters, cavity-assisted Raman interferometry was not viable. We further developed the routine for multi-photon Bragg transitions and explored the limits. The results are published in Physical Review A, ArXiv and Proceedings of Science.
I built the Birmingham Environment for Software Testing (BEST) shortly after my work verifying numerical models for the cavity assisted atom interferometry paper. I found that each time I modified part of the model, to introduce a new feature or speed up the execution time, I would need to re-run lots of detailed simulations to ensure I hadn't introduced a bug. These simulations could take hours and so I wanted to automate the process.
The solution I was looking for was not unlike Continuous integration in software engineering. Unfortunately, unlike software engineering my builds were not fast and my tests were very slow and computationally expensive. I found common tools like Jenkins and GitLab were not suitable for my tests.
I built BEST to alleviate these problems, it can be used standalone or it can hook into GitLabs CI system. It supports grouping of errors by return codes, so you can separate programming errors from numerical/science errors. It supports invoking multiple interacting languages (e.g. C++, Python, Bash) all in one test, so you can have a script (e.g. python) that tests your program (e.g. C) in some large parameter space.
If you are interested in using BEST, or setting up your own server please do let me know.
- BEST FAQ
- BEST Preview
16th February 2018
TEDx - The Gravity Synth (Invited Talk)
21st November 2018
Astronomy In the City (Invited Talk)
- Instruments Gravitational Wave Detectors and Musical Instruments Alike.
- 27th July 2018 Lunar Festival (Invited Talk) - Gravitational Waves.
- 16th May 2018, The Botanist, Birmingham. Pint of Science (Invited Talk) - How Improvements To Gravitational Wave Observatories Enabled GW-Multi-Messenger Astronomy. LIGO Document Link (login required).
- 16th May 2018, 1000 Trades, Birmingham. Maker Monday (Invited Talk) - Audio Synthesis Using Miniature Model Gravitational Wave Detectors.
- 21st March 2018, Whitworth Art Gallery. Future Sessions Launch Party (Invited Talk) - I presented for 10 minuets on the significance of Gravitational Wave Instrumentation to contextualize a Gravity Synth performance. This was a real opportunity to artists about science.
- 26th-30th September 2018 Gravity Fields Festival I won £500 funding plus accommodation to run a three day Gravitational Waves themed science exhibit including the Gravity Synth and planetarium.
- 27th-29th July 2018 Lunar Festival I built and installed a 3 day day art installation centered on Gravitational Wave technology. I also gave a talk (see above) alongside a Gravity Synth performance later in the evening.
- 10th March 2018 Seventh Wave Festival of Electronic Music I presented the Gravity Synth as a preliminary trial using this performance to engage with music enthusiasts and artists about science.
- 3rd October 2017, Malvern Malvern Festival of Innovation. I organized the groups attendance at the Malvern Festival of Innovation. We developed a new interactive planetarium exhibit for this event on cosmological distance scales.
- Summer 2017 Procured a 5.5m planetarium for the research group, trained fellow postgraduates and the student astronomical society to use it and built a website for it.
- 1st-9th July 2017 Royal Society Summer Science Exhibition (see above).
- 15-17th May 2017 Co-organized Pint of Science Atoms to Galaxies event. Larger than a usual Pint of Science, our event was held at Millennium Point and sold around 200 tickets each night. I built two new exhibits including a Rubins Tube and a Michelson Interferometer. We won funding from IoP to support the venue hire costs.
- Spring 2017 Built Gravity Synth! initial prototype.
- 25th Feb 2017 Organized visit to Big Bang Fair at Leicester Grammar School about Gravitational Waves.
- 1st Nov 2016 Organised visit to William Brookes Sixth Form about Gravitational Waves and Quantum Technology.
- 21st - 22nd September 2016, Grantham, UK Gravity Fields Festival. Presented Gravitational Waves exhibit.
- 16-19th March 2016, Birmingham NEC, UK Nuclear Institute Big Bang Fair. I organized my attendance at the event and drafted a business case to my employer to allow me to attend and cover my costs. I was awarded a Certificate of Appreciation in return. This was the first STEM outreach I had done and I immediately recognized the importance, both outside the university sector and within. Big Band Fair Marketing Video.
Note: You will need to accept a self signed certificate.
I developed a Newtonian model of the solar system as part of
my undergraduate studies. The aim was to predict the trajectory
of a satellite undergoing a
gravity assist (e.g. voyager), but the program models all of
the gravitational interactions between the planets with an
adaptive step size routine written in C++.
See my report and code.
Public Talks, Engagement & Outreach
The Gravity Synth is a musical performance that is formed by the fusion of a Miniaturized Gravitational Wave Detector and a modular synthesizer.
The project explores a new way of engaging both artists and the general public. I built a working, portable, robust Michelson Interferometer, that was capable of interfacing with a modular synthesizer. Together with the modular synthesizer, the device is an entirely new musical instrument.
The device provides an immediate source of engagement to artists who can become inspired by Gravitational Waves and can incorporate this into their work.
I have been leading this project for a number of years now, right from the initial build, through the first prototypes to the final build. I give regular talks about the project to artists, scientists and the general public.
The Royal Society Summer Science Exhibition is a week-long public engagement event held at the Royal Societies London headquarters. I joined as part of the Birmingham group, alongside a number of other UK universities working in Gravitational wave research. Considered by some to be the premier public engagement event, attended by media, politicians as well as the general public.
The Birmingham group presented a large interactive tabletop Michelson interferometer . The interferometer was previously part of an exhibit in the Thinktank Futures gallery and needed to be upgraded with a real-time signal readout and large plastic buttons to modulate the length of the arms, mimicking the effect of a Gravitational Wave passing though detector.
There were 4 buttons, each mimicking the effect of a different Gravitational Wave source on the detector. They worked by moving one of the mirrors a small amount to represent a changing space-time interval. The light would then interfere as it does in a gravitational wave detector (e.g. LIGO/Virgo). The interference pattern would be visible (as in the original exhibit), but also read by a photo diode and plotted real time on the screen.
This presented a number of technical challenges, for safety reasons we restricted ourselves to 1mW of light (same as a laser pointer), this was enough to produce a visible pattern. The photo-diode was placed behind the screen with a small pinhole providing light to it. However, after accounting for losses only a few hundred microwatts of power (which is comparable to a bright room) reached the photo-diode and so the signal was noisy.
Alongside two other PhD students, we solved the problem by only allowing certain frequencies of light to pass through and be amplified. Then averaging was applied in software.
I also developed the internal electronics for the button box, reading the signal and relaying over USB. Mounting this into the box with reliable joints that could be fixed away from the lab presented its own set of technical problems.
Development of a 2nd Year Undergraduate Python Course
In the first year of my PhD I co-developed a new second year python module, teaching students how to do simple numerical modeling in a Jupyter notebook. The module is automatically marked. I continued to work as a PGTA for the following two years while the course was in its infancy.
Post Graduate Teaching Assistant (PGTA)
I worked as a PGTA for three years at the University of Birmingham. I marked reports and helped students develop skills to solve the problems they had been set.