Funded PhD studentships

We are currently accepting applications for STFC and University funded studentships in our group for a September 2025 start. Interviews for shortlisted candidates are expected to be held in February and March initially and will continue until the positions are filled. Please apply using the online application form.

Some examples of funded projects:

PhD Studentship on the NOvA Neutrino Experiment

A studentship is available to join the Sussex group working on the NOvA experiment under the supervision of Dr Lily Asquith. The NOvA experiment uses the world’s most powerful neutrino beam provided by Fermilab in Chicago, USA to measure the oscillation of muon-type to electron-type neutrinos using a pair of detectors separated by 800 km. NOvA will continue with more than a decade of data-taking until around 2027, and so is entering the most important era in terms of data analysis. Exploitation of the huge final data set will require creative thinking in addition to the development of machine learning techniques and novel approaches to the treatment of systematic uncertainties. The Sussex NOvA group comprises two faculty, two postdocs, and three PhD students. We are leading the effort to use thousands of “test beam” particles to improve the measurements of the oscillation parameters, including the Charge-Parity violation parameter that could reveal the secret of our matter-dominated universe. (supervisor: Dr Lily Asquith)

ATLAS: measuring the properties of the top quark and the Higgs boson  

Probing the Higgs boson, the most recently discovered fundamental particle, and one unlike anything else in the SM, is a critical priority in the search for new physics at the LHC. The Higgs boson is responsible for giving fundamental particles their mass and has the strongest interaction with the largest mass particles. The top quark is the heaviest fundamental particle in the SM and therefore has the strongest coupling to the Higgs. This makes LHC collisions where a Higgs is produced with a top-quark pair (ttH) one of the most exciting places to look for signs of new physics. The candidate will play a leading role in new measurements of ttH in the H->leptons decay mode using Run 3 data. This will provide fresh sensitivity to the top quark-Higgs interaction and the Higgs boson’s interaction with itself that will lead to world-leading sensitivity to new physics. The importance of this work goes beyond understanding the Higgs boson. The interplay between the strength of the top-Higgs interaction and the Higgs self-interaction is directly related to the stability of the Universe at a quantum level and the exact (CP) nature of the top-Higgs interaction could hold the answer to why we exist at all - why the Universe is matter-dominated. Efforts are ongoing to combine measurements of ttH with those of ttW, ttZ and more which all share a similar final state. The candidate will also be involved in such efforts including searching for new physics via effective field theory (EFT) techniques. The ATLAS-Sussex group has made significant contributions to measurements of ttH, ttW and ttll production in multi-lepton final states performed so far in ATLAS: profiting from this experience in the group, the candidate will be ideally positioned to make large impact in this sector, also through close contact with CERN-based experts. (Supervisor: Dr Josh McFayden)

PhD Studentship on the SNO+ Neutrino Experiment

A studentship is available to work on the SNO+ experiment under the supervision of Dr Elisabeth Falk. SNO+ offers a rich programme of neutrino physics, which includes neutrinoless double beta decay, antineutrinos from reactors and geothermal activity, solar neutrinos and a supernova watch. It is located at SNOLAB, 2 km underground in the Creighton mine in Canada. The experiment is taking physics data with the liquid-scintillator detector, with preparations for the introduction of the double beta decay isotope underway. You will join the Sussex group in working on the analysis of antineutrinos from nearby nuclear reactors. The focus will be on an oscillation measurement that is expected to surpass the current world-leading result for the so-called solar mass splitting within the duration of the studentship. You will also contribute to the calibration of the experiment and to data quality assurance, as well as participating in SNO+ experimental operations. You will have the opportunity to spend an extended period of time at SNOLAB. (Supervisor: Dr Elisabeth Falk)

FASER(2): Looking forward to new physics

FASER stands for “ForwArd Search ExpeRiment” and is one the newest experiments based at the Large Hadron Collider (LHC) at CERN. It is a novel experiment searching for exotic long-lived and weakly-interacting new particles. Such particles are excellent candidates to explain the existence of Dark Matter. If they exist, these exotic particles would be produced in collisions inside the ATLAS detector and detected nearly 500m away in FASER. 
The Sussex Experimental Particle Physics group has had involvement in the construction and commissioning of the FASER detector that is now installed underground at CERN. FASER is currently taking data during LHC Run 3 and the candidate will make major contributions to the analysis of this data with a view to probing brand new areas of phase-space that have until now been experimentally out of reach. The analysis of the data will involve understanding the performance of the detector and backgrounds to be then be able to search for possible signs of new particles. In addition, R&D studies are underway for a significantly upgraded detector to FASER, known as FASER2. This detector would be housed in the Forward Physics Facility and would be installed in next, high-luminosity (HL), phase of running for the LHC (Run 4) and would take data until the end of HL-LHC. It has a strong neutrino physics measurement programme in addition to the searches for new physics. The candidate will investigate different designs of FASER2 to determine what layouts and detector technologies will be required to get the best sensitivity to neutrinos and long-lived new particles. The Sussex Collider physics group has made significant contributions to the construction, commissioning and operation of FASER and is leading R&D efforts on FASER2: profiting from this experience in the group, the candidate will be ideally positioned to make large impact in this sector, also through close contact with CERN-based experts. (Supervisor: Dr Josh McFayden)

Novel Opaque Scintillator Detector R&D and Neutrino Physics

A  studentship is available to join the Sussex group working on novel opaque scintillator detector R&D and neutrino physics under the supervision of Prof Jeff Hartnell. You will have the opportunity to work on the exciting and counter-intuitive idea of using opaque scintillators as particle detectors. Traditionally, light travels through a transparent scintillator to a photosensor. Our approach, called LiquidO, embeds a lattice of optical fibres in an opaque scintillator with a short scattering length. The scintillation photons are stochastically confined close to the point of production via scattering and extracted by the fibres, removing the need for manual segmentation to create high-resolution imaging detectors. There are many applications in particle physics and beyond. Further information can be found here. You will join one of the largest groups developing this technology world-wide. Prof Jeff Hartnell co-leads the CLOUD neutrino experiment, which will deploy a 10-ton LiquidO detector 35 metres from Europe’s most powerful nuclear reactor cores at Chooz in France on the timescale of this studentship. The Sussex group also has a strong programme of in-house prototype development, construction, operation and analysis as well as characterisation of different scintillators and fibres. This project also includes the opportunity to spend an extended period working overseas. (Supervisor: Prof Jeff Hartnell)