We deliver real-world solutions to the football community. Our areas of interest within football include: fitness and nutrition, psychology, match analysis, physical activity, skill acquistion and coaching, and performance analysis.
Our research is applied in nature and is focused on physical activity, sedentary behaviour, fitness and health in laboratory and various real world settings.
Find out more about Nineteenth-century writing and print culture research within the Research Institute for Literature and Cultural History.
ART LABS offers contemporary and innovative approaches to professional research, art practice and advanced study.
The General Engineering Research Institute (GERI) conduct a wide range of projects. Find out more about some of these research case studies here, including the phase unwrapping project, the laser doppler anemometry project, the PiE laser project and the icroelectronic packages project.
Find out more about possible PhD projects for 2026 in the Astrophysics Research Institute. If your favourite topic is not in the list, we highly encourage you to contact staff in your fields of interest to discuss PhD projects.
The Astrophysics Research Institute specialist subject areas include theoretical galaxy formation, time domain astrophysics, stellar populations and astronomical instrumentation. Discover more about each of these areas.
The Galaxy Formation and Evolution Research Group looks at population studies of dwarf galaxies up to the most massive clusters of galaxies, supermassive black holes and detailed modelling of the internal structure of galaxies. Discover more about our expertise, who we work with and meet the researchers.
Within the time domain astrophysics research group, we are involved in major observational survey projects. We work on a variety of explosive transients, including galactic and extragalactic novae, type la supernovae, core collapse supernovae, and gamma rays bursts. The Liverpool Telescope is the workhorse of the group. Find out more about our research.
By studying the gas and stars that shape the Milky Way as well as other galaxies in the local Universe, we can understand the life cycles of stars like our Sun, unravel the chemical enrichment history of the universe, and probe the existence of black holes across a wide mass spectrum.