Numerics and theory of relativistic astrophysical transients

The University of Bath invites applications from outstanding candidates for a 3.5-year funded studentship in numerical and theoretical high-energy astrophysics within the Bath Astrophysics Group in the Department of Physics.

The successful applicant will work with Dr Van Eerten on theoretical and numerical modeling of high-energy astrophysical transients, in particular relativistic outflows from gamma-ray bursts and related phenomena such as supernovae, blazars and tidal disruption of stars. Over the course of the PhD, the applicant will both adapt existing software and develop from scratch solvers for applications in relativistic magnetohydrodynamics and radiative transfer. The applicant will work directly with other group members at Bath and with UK & international collaborators in applying numerical methods to interpretation of broadband data from transients.

The group has premium access to Bath’s newly commissioned 3000-core HPC Balena cluster. Bath group members are involved in major international projects including next generation X-ray satellites, LSST and the CTA and are well connected to other Research Institutes in the UK and abroad.

The University of Bath offers a comprehensive programme of postgraduate skills training; advice is readily available for careers in industry or academia. The Bath Doctoral College ensures a strong support network for students across disciplines and regular student-led astrophysics symposia are held with partner Universities through the Bristol-Bath-Exeter-Cardiff student symposia (BBECss) initiative.

Applicants should have a background in the physical sciences and have or expect to gain a First or Upper Second Class UK Honours degree, or the equivalent from an overseas University. A strong affinity with numerical modelling and programming is preferred.

Anticipated start date: 2 October 2017.