PhD Studentship in Computational Astrophysics - Magnetic Fields and Superconductivity in Neutron Star Cores

Soon after the discovery of first neutron stars, it was suggested that the inner part of the star (its core) is a gigantic superconductor. Over the last twenty years researchers made extraordinary progress in understanding of different types of neutron stars and their X-ray emission by modelling crust-confined magnetic field evolution, but completely ignoring the core. It is time now to start disentangling the core mystery and to probe different scenarios for magnetic field evolution in the core while considering superconductivity.

In this project, the PhD student will solve various MHD systems of equations describing fluid motion and magnetic field evolution using Dedalus code. This project involves performing simulations on supercomputer. You will receive training and gain skills in running a computer code on HPC facilities, development and analysis of complicated MHD simulations., You must have, or expect to gain, a minimum 2:1 Honours degree or international equivalent in a subject relevant to the proposed PhD project (Physics or Applied Mathematics). Enthusiasm for research, the ability to think and work independently, excellent analytical skills and strong verbal and written communication skills are essential requirements.
Home and international applicants (inc. EU) are welcome to apply but only home fees are covered. Applicants whose first language is not English require an IELTS score of 6.5 overall with a minimum of 5.5 in all sub-skills.
International applicants may require an ATAS ( ) clearance certificate prior to obtaining their visa and to study on this programme.