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We have 136 PhD Projects, Programmes & Scholarships for Self-funded Students in Cardiff
PhD Projects, Programmes & Scholarships for Self-funded Students in Cardiff
We have 136 PhD Projects, Programmes & Scholarships for Self-funded Students in Cardiff
Cardiff University School of English, Communication and Philosophy - PhD Opportunities
With its unique mix of disciplines, Cardiff School of English, Communication and Philosophy offers an exciting range of specialised and innovative postgraduate programmes and a dynamic and highly successful research culture. Read more
Developing Large Arrays of Superconducting Microwave Kinetic Inductance Detectors for Future Astronomy Instrumentation
The Cardiff Astronomy Instrumentation Group (AIG) is one of the world leaders in Microwave Kinetic Inductance Detector (MKID) development. Read more
Advanced numerical methods for solving the forward problem in E/MEG
Electroencephalography (EEG) is a technique that measures the electric potential originating from the brain using electrodes located on the scalp. Read more
[STFC Studentship] Simons Observatory – Small aperture telescope build, testing and deployment
It is widely believed that very shortly after the Big Bang, the universe underwent a period of very rapid expansion, called inflation. Read more
[STFC Studentship] Developing Large Arrays of Superconducting Microwave Kinetic Inductance Detectors for Future Astronomy Instrumentation
The Cardiff Astronomy Instrumentation Group (AIG) is one of the world leaders in Microwave Kinetic Inductance Detector (MKID) development. Read more
Revealing the Hidden Light: Understanding the cosmic dust and cold gas in nearby galaxies.
Over half the light ever emitted by stars in the Universe having been absorbed by cosmic dust, and the situation is worse (>90%) when looking at regions where star-formation is occurring. Read more
Machine Learning for Multi-Messenger Astronomy with Gravitational Waves
Gravitational waves (GWs) are produced by some of the most violent events in the Universe, such as the mergers of black holes and the explosive deaths of massive stars. Read more
Characterisation of tissue microstructure from non-invasive MRI using Machine Learning
The characterisation of biological tissue microstructure in vivo and non-invasively is of outmost interest in science. If successful, it could reveal unique insights into biological processes, including aging and cancer. Read more
Why is the Universe getting cleaner by the day? Modelling dust, gas and metals in high redshift galaxies using BEDE
High redshift galaxies discovered using submillimetre surveys of the sky (so-called submillimetre galaxies) are likely ancestors of present-day massive early-type galaxies. Read more
Understanding carrier dynamics in CuInZnS3 quantum dots toward high-performance indoor photovoltaics
CuInZnS3 quantum dots (CIZS QDs) is a non-toxic and phosphide free material which has a significant potential to be used in wearable PVs and indoor PVs [1,2]. Read more
Towards a clinical MEG system: theoretical and practical insights into the use of optically pumped magnetometers
Magnetoencephalography (MEG) is a non-invasive medical imaging technique that allows characterisation of human brain electrophysiology by measuring magnetic fields generated by neural currents. Read more
The Sweet-Spot for Star Formation
CONTEXT. Star formation is one of the most fundamental processes regulating the evolution and appearance of the Universe, with implications for many diverse areas of astronomy. Read more
The Late Stages of Galaxy Evolution – a project with the Euclid Space Observatory
The Hubble Space Telescope (HST) and the James Webb Space Telescope (JWST) make it possible to obtain high-resolution images of tiny areas of sky. Read more
The formation and evolution of star-forming filaments
CONTEXT. Filaments play a critical role in star formation. Read more
Star Formation Triggered by Colliding Interstellar Clouds
CONTEXT. Much of the interstellar gas in a galaxy like the Milky Way is in dense molecular clouds. When these clouds enter a spiral arm, they merge to form larger clouds, and are compressed to higher densities. Read more