Dynamics of compact objects at the centre of galaxies and implications for gravitational wave detections

Outline

Under the supervision of Dr Fabio Antonini, the student will develop a theoretical framework to make predictions for the gravitational wave sources produced in the nuclei of galaxies where dense nuclear star clusters are often observed.

What is funded

This project will be funded by the STFC.

Applicants should apply to the Doctor of Philosophy in Physics and Astronomy with a start date of 1st October 2020.

https://www.cardiff.ac.uk/study/postgraduate/research/programmes/programme/physics-and-astronomy

Duration

3 years

Eligibility

You should have obtained, or be about to obtain a First or Upper Second Class UK Honours degree in Physics , or a related subject, Alternatively, applicants with equivalent qualifications gained outside the UK will also be considered. Applicants with a Lower Second Class degree will be considered if they also have a Master’s degree.

Applicants whose first language is not English are normally expected to meet the minimum University requirements (e.g. 6.5 IELTS)