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PhD Thesis Prize

PhD/MSc Thesis Prize 2023

Many congratulations to Matthew Pearce, Ross Hunter, Sahl Rowther and Cait Cullen for their success in the 2023 Thesis Prize competition!

PhD Thesis Prize 2022

Many congratulations to Samuel Holt, Arnau Brossa Gonzalo and Benjamin Cooke, for their success in the 2022 PhD Thesis Prize competition!

SamDr Sam Holt was awarded the Faculty of Science Thesis Prize for an outstanding Physics PhD. Sam worked on exotic magnetic states known as skyrmions. He writes " I started at the University of Warwick in 2013 where I completed my undergraduate degree and continued at Warwick for my PhD under the supervision of Geetha Balakrishnan. My PhD research was undertaken as part of the UK Skyrmion project, a collaboration between the universities of Warwick, Oxford, Cambridge, Durham, and Southampton which investigates the physics of topological magnetic textures known as magnetic skyrmions. These skyrmion systems have been of great interest since their recent discovery in 2009 due to the interesting physics they present and their potential uses in spintronic devices. My thesis focused on studying skyrmions in Néel systems, Bloch skyrmions in confined geometries, and creating Python software to simulate the results of various experimental techniques on arbitrary magnetic states. I have since been working as a research fellow at the University of Southampton specialising in computational magnetism. "

Congratulations on the Faculty thesis prize, Sam!

ArnauDr Arnau Brossa Gonzalo was awarded the Springer Thesis Prize, for his doctoral thesis "First observation of B0→Dbar*(2007)0K+π− and B0s→Dbar*(2007)0K−π+ decays in LHCb". Arnau explains: "The Standard Model of particle physics is extremely successful at describing matter interaction at the most fundamental level. However, it is not perfect and while it provides several predictions up to an impressive level of precision it fails to answer some questions such as the difference between matter and antimatter in the early stages of the universe, which predictions are in direct disagreement with cosmic background radiation observations.

My work is yet another step towards answering this question, focusing on the search of B hadron decays to a D* meson, a Kaon and a Pion. These decays exhibit CP-violating properties, i.e. this decay behaves slightly differently than the conjugate anti-B hadron decay. This makes its understanding crucial for the finding of possible discrepancies with respect to the Standard Model predictions. As these decays are extremely rare and can only occur at very high energies, my work is based on the data recorded by the LHCb experiment during the years 2016 to 2018. The data sample consists in proton proton collisions at energies at the TeV scale. These collisions generate a very rich hadronic environment with a small probability for these decays to occur among hundreds of other processes.

In order to be able to measure these processes, we require a detector capable of tracking and identifying all the different particles involved in the decay. Since the probability for these decays to occur, and more importantly, to be detected is so small, a high number of events (of the order of millions!) is required. From all these events only the events which include the decay under study are selected. Using that process we can measure not only the probabilities for the B-hadron and anti B-hadron decays to happen but also to measure the momentum distribution of the final state particles which is crucial for the complete understanding of this and similar CP-violating processes."

Well done to Arnau on his prize!

BenDr Ben Cooke was awarded the Winton Thesis Prize for an outstanding Astronomy PhD. Ben's studies were on extra-solar planets. He explains " My PhD focussed on monotransiting exoplanets – these are planets which orbit stars other than the sun that are only seen to transit once during our observations of them. The majority of well characterised exoplanets have short orbits, allowing us to see them transit multiple times and making it easier to constrain their periods. Those on longer orbits, planets more similar to our own, are more likely to be monotransits and their periods are harder to constrain. In my thesis I predict the abundance of these type of signals in the data from a current transit mission, TESS (Transiting Exoplanet Survey satellite), as well as simulate the optimal way to follow them up to better characterise them with the minimum expenditure of telescope time. I found that, for exoplanets with periods greater than 30 days, monotransits well outnumber multitransits and are thus vital to better explore this region of parameter space. The work in this thesis has helped influence the direction of NGTS (Next-Generation Transit Survey) and led to the discovery and characterisation of some of the first monotransiting exoplanet systems from the TESS mission.

The figure shows the predicted distribution of multi and monotransiting systems found by TESS, multitransit systems are in red with monotransit systems in blue. It is clear that to properly explore the parameter space for orbits over 30 days one must effectively utilise monotransits."

Many congratulations to Ben on the fantastic work.


PhD Thesis Prize 2021

Many congratulations to Elena Cukanovaite, James Gott and Samuele Ferracin, for their success in the 2021 PhD Thesis Prize competition. Read on for more information about their research and its importance.

ElenaDr Elena Cukanovaite was awarded the Winton Prize for Astrophysics, for her doctoral thesis on "3D atmospheric models of helium-dominated atmosphere white dwarfs". Elena, who is currently working as a postdoc in the Astrophysics & Astronomy groupLink opens in a new window at Warwick, writes: "During my PhD I used powerful computers to recreate the atmospheres of dead stars. These remnant stars are known as white dwarfs, and they are the leftover cores of stars that have died after exhausting their life fuel. Roughly 97% of all stars in the Milky Way galaxy are destined to become white dwarfs, including our own Sun. Therefore, white dwarfs are incredibly important objects when trying to understand the evolution of stars, and planetary systems like our own solar system. Recent discoveries of planets and planetesimals around several white dwarfs have shown that planetary systems can in fact survive the death of their host star.

To be able to extract all this information from white dwarfs, we need to understand the observations we obtain for white dwarfs. Most of the information we can get from stars comes in the form of light, which has been generated in their atmospheres and travelled to us through the fabric of space. Thus, for us to be able to interpret this data, we need to be able to model stellar atmospheres correctly. By comparing our models with observed data, we can extract fundamental parameters of white dwarfs.

The astronomical community have had atmospheric models of white dwarfs for many decades, but with faster and better computers, we have been able to create more realistic models. The major improvements of the models I have created is in terms of their dimensionality. Before 2011, only 1D models were used for white dwarfs. However, we all know that we live in a 3D world, and thus using 1D models is simply not very realistic. During my PhD, I have modelled the atmospheres of a specific type of a white dwarf for the first time in 3D. This has allowed me to collect more accurate information on white dwarfs and thus improve studies of exoplanets, galactic evolution and beyond."

These two animations show the light leaving the top of my 3D simulations. They both have very different temperatures and surface gravities. On the left, the model is relatively cool and is not as dense as the model on the right. The model on the right is also much hotter. The animations shown here define the two extremes of the models I have created.
Left Right

samDr Samuele Ferracin was awarded the Faculty of Science and Department of Physics Thesis Prize, for his doctoral thesis "Devising accreditation protocols for near-term quantum computing devices". Sam explained: "The past few years have seen unprecedented advances in the development of quantum computers. These fascinating devices promise to boost our computational capabilities well beyond their current limits. However, due to the quantum nature of their internal components, they suffer non-negligible levels of noise and their outputs are unreliable. As the available quantum computers rapidly grow in size and become harder to simulate on “classical” computers, finding methods to characterize their performance is a task of timely importance.

During my PhD I focused on finding schemes to verify the correctness of the outputs of noisy quantum computers. Together with my supervisor and some colleagues I developed a protocol to assess how close the “noisy” outputs are to the correct ones. Importantly, our protocol does not require classical simulation of quantum computations and is fully scalable for the long term. In collaboration with a research team at IBM we have tested this protocol on two experimental devices, demonstrating the effectiveness of our method as well as its practicality."

Many congratulations to Sam on this prize! Sam is currently a postdoctoral researcher at the University of WaterlooLink opens in a new window, Canada.

Dr James Gott is this year's winner of the Springer Thesis Prize for his doctoral study on "Defects in Self-Catalysed III-V Nanowires". James, who is currently a postdoc in the Condensed Matter cluster, explains:

"Semiconductor nanowires are a candidate for next generation technology due to superior properties enabled by their geometry. Current semiconductor devices are limited in choice of material combinations due to the unavoidable formation of imperfections during growth. The size and shape of nanowires allows growth of perfect crystals using a wider range of material combinations due to more efficient strain relaxation. However, perfectly optimised growth is rare and imperfections can, and do, still occur in nanowires. Imperfections, such as planar defects or diffuse interfaces, diminish device performance and need to be understood.

In my thesis I present an in-depth study into imperfections that can be found in self-catalysed III-V semiconductor nanowires. By utilising the advanced electron microscopy facilities at Warwick, I analysed interface sharpness and defects at the atomic and macroscopic scale. I discovered that a surprising variety and quantity of defect structures can exist in nanowire systems, and they can in fact host some never-before-seen defect configurations. To probe how these defects are formed, conditions during nanowire growth can be emulated inside the microscope using the latest generation of in-situ heating holder. This allowed me to examine defect formation, dynamics, and removal, revealing that many of the defects can in fact be removed. This information is critical for attaining perfect nanowire growth and presents annealing strategies to improve crystal quality, and therefore device performance.

The work in my thesis helps us to understand how we can better engineer nanowires for improved device performance in current and future applications. This helps boost the pursuit of increasing transistor density beyond the limit set by Moore’s law."

(a) Scanning electron microscope image of nanowires attached to substrate. (b) A scanning transmission electron microscope (STEM) image of a single nanowire with a defective tip. (c) Colourised atomic resolution STEM image of some defect structures found in a nanowire.
James Gott research James Gott

PhD Thesis Prize 2020

Many congratulations to George King, Ben Chapman and Connor Mosley, for their success in the 2020 PhD Thesis Prize competition. A full list of recent thesis prize winners, and other accolades earned by the Department's PhD students, can be found here.

George King

George King was awarded the Winton Prize for Astrophysics, for his doctoral work on "Observations of Exoplanetary Systems at X-ray Wavelengths". George explained:

My work focused on exoplanets - planets around other stars - orbiting much closer to their star than Mercury orbits the Sun. At such close distances the output of high-energy X-rays from a star can remove material from the atmospheres of planets. I investigated the rate and energy of X-rays hitting a range of nearby exoplanets, to assess both current ongoing changes these are causing and how it has influenced the planets' evolution in the past. I also worked on the first detailed observation of a exoplanet transit (the short drop in the light from the star due to a planet passing in front of it) in X-rays. Observing this in X-rays could allow us to directly investigate gas being stripped from the planet.


Connor Mosley was a joint winner of the Faculty of Science Thesis Prize, and also won the Springer Thesis Prize. His thesis on terahertz spectroscopy of anisotropic materials will be published in book form by Springer. In Connor's work he created a new source of terahertz (far infrared) radiation with excellent polarisation control, which he used to study exotic magnetic materials. Connor writes:

The work presented in this thesis may have immediate impact on the study of anisotropic media at THz frequencies, with photoconductive emitters and detectors being the most commonly used components for commercially available terahertz spectroscopy and imaging systems, and by providing a new way to study the nature of magnetic phase transitions in multiferroics. In the longer term the increased understanding of multiferroics yielded by ultrafast spectroscopic methods, including terahertz time-domain spectroscopy, may help develop new magnetoelectric and multiferroic materials for applications such as spintronics.

BenBen Chapman was a joint winner of the Faculty of Science Thesis Prize, for his thesis titled "Ion cyclotron emission from energetic ion populations in fusion plasmasLink opens in a new window". Ben writes:
Future fusion reactors, such as ITER, will fuse deuterium-tritium to produce 3.5 MeV alpha-particles. It is crucial we understand the underlying physics of these fast ions if they are to be exploited to sustain thermonuclear burn. These fast ions are able to excite Ion cyclotron emission (ICE) waves, which, in fusion reactors, are in the radio frequency range. The detection of ICE is non-invasive, making it an attractive way forward for energetic ion measurements in future tokamaks such as ITER.

Ion cyclotron emission (ICE) comprises suprathermal radiation whose spectrum peaks at successive local cyclotron harmonics of the emitting energetic ion population. The driving mechanism behind ICE is the magnetoacoustic cyclotron instability (MCI). In this thesis, we simulate the MCI using the EPOCH particle-in-cell (PIC) code to solve the self-consistent Maxwell-Lorentz system of equations for fully kinetic electrons, thermal background ions, and the minority energetic ion distribution that drives the primary ICE.

By comparing PIC simulation results with experimental data from the KSTAR tokamak, we examine the nature of ICE excited by different energetic ion driving populations during edge localised mode (ELM) events. Simulations of ICE observed in the JET and ASDEX-Upgrade (AUG) tokamaks are then discussed. Motivated by recent observations of ICE in the core region of several tokamaks, we then compare MCI simulations that use two types of energetic ion distribution function, a spherical shell of varying thickness, and a ring-beam of varying width. We build on this work by demonstrating that observations of core ICE in AUG can be explained in terms of a driving population of fusion-born protons relaxing via the MCI. Bicoherence analysis shows that this is made possible through nonlinear wave-wave interactions between linearly unstable cyclotron harmonics.