This is a Masters by Research project.
Primary supervisor - Dr Sam Lander
Magnetars are extreme objects for two reasons. They are a kind of neutron star, compressed nuclear-density remnants of a supernova explosion and the densest objects in the Universe, but additionally harbour the strongest known magnetic fields in the Universe. Magnetars lose rotational energy relatively quickly, in a way usually attributed to their strong magnetic dipole radiation, but theoretical models of this process cannot fully explain observations. In particular, irregularities in their rotation, known as glitches, are commonplace, and indicate a coupling between the star's crust and its interior superfluid of neutrons. This project will seek to model this irregular rotation through local heating that destroys regions of superfluid temporarily.
Entry requirement
Minimum entry requirement is 2:1 in Mathematics, Physics.
Mode of study
Full-time
Start date
1 February 2026
Deadline
30 November 2025. Project is open to Home applicants only.
