Loading…
Loading grant details…
| Funder | UK Research and Innovation Future Leaders Fellowship |
|---|---|
| Recipient Organization | Imperial College London |
| Country | United Kingdom |
| Start Date | Jan 25, 2021 |
| End Date | Jan 31, 2026 |
| Duration | 1,832 days |
| Number of Grantees | 2 |
| Roles | Fellow; Award Holder |
| Data Source | UKRI Gateway to Research |
| Grant ID | MR/T041323/1 |
Our current understanding of physics does not explain why the universe around us is made overwhelmingly of matter and not antimatter. My work on the T2K experiment, which studies the oscillations of a type of particle called the neutrino as it travels long distances, has seen hints of a new type of matter-antimatter difference which has the potential to provide an explanation for the matter dominated universe.
Larger datasets and smaller uncertainties are necessary to confirm these differences. My fellowship will address both of these issues.
During the fellowship, the currently running long distance neutrino oscillation experiments, T2K and NOvA, will collect their largest neutrino-oscillation datasets to date. I will lead the analysis of T2K's data, which will, for the first time, be sensitive enough to provide highly significant evidence for matter-antimatter differences in neutrinos.
As well as using the larger dataset, I will add new samples of neutrino events to the analysis, increasing the number of neutrino interactions that can be studied by approximately 30%. Not only will these new samples further increase the size of the available data, they will also give us a better understanding of how neutrinos interact with our detectors, allowing us to reduce the uncertainties in our analyses due to our knowledge of neutrino interactions.
The resulting analysis will be the most precise constraint on matter-antimatter differences in neutrinos from any single experiment.
Currently T2K and NOvA analyse their data separately. This separation means that information that each experiment has that would improve the other's analysis is ignored. During this fellowship I would work with collaborators in the NOvA experiment to analyse T2K and NOvA data together for the first time.
The result will be a more precise constraint on matter-antimatter differences in the neutrino sector than either experiment could produce alone, maximising the impact of these UK government funded experiments.
The billion-dollar scale DUNE experiment, which is scheduled to start taking data in the mid 2020s, promises even larger neutrino oscillation datasets than those from T2K and NOvA. However, our current understanding of neutrino interactions with our detector materials is not good enough to take advantage of these datasets. I will develop part of a High-Pressure gas Time Projection Chamber (HPgTPC) for DUNE that will measure neutrino interactions of a type inaccessible to previous detectors.
The resulting reduction in our uncertainties on neutrino-matter interactions will give DUNE the capability to definitively observe and fully characterise the neutrino matter-antimatter asymmetry. In the long term there are potential medical applications of this type of detector in better understanding how radiation is deposited in materials, such as those used in radiotherapy.
The subsystem that this fellowship will allow me to lead the construction of is the HPgTPC's data acquisition (DAQ) electronics. DAQ electronics allow the HPgTPC to record the neutrino interactions of interest. To do this, I will use high-speed FPGA electronics which have wide applicability both within STFC's science area and more widely including the medical sector, fintech and national security.
Furthermore, UK companies will be able to manufacture parts of the system, furthering the UK's high-tech sector. I will also lead a program of prototype tests of the HPgTPC in beams of low energy particles. These tests will allow the detector to be accurately calibrated and improve our knowledge of the interaction of these low energy particles with a variety of different materials.
A reduction of DUNE's analysis uncertainties from 3% to 2% will correspond to a 33% reduction in the running time necessary to achieve definitive observation of matter-antimatter asymmetry in the neutrino sector, allowing us to do more physics with the same amount of funding.
Imperial College London
Complete our application form to express your interest and we'll guide you through the process.
Apply for This Grant