Compact Relativistic Objects (Astrophysical and Geophysical Fluid Dynamics)

The most dramatic cosmic phenomena like Supernova Explosions, Active Galactic Nuclei, or Gamma-ray Bursts involve formation of compact relativistic objects like neutron stars and black holes. Their interaction with surrounding plasma can only be understood within the framework of Einstein's theory of relativity. Our research in this area is focused on numerical simulations of various phenomena that can be described using relativistic gas dynamics, electrodynamics, or MHD. These include jets from active galactic nuclei, electromagnetic and MHD winds from neutron stars and black holes, accretion onto black holes.

keywords: applied mathematics, astrophysics, relativistic gas dynamics, electrodynamics, MHD

Astrophysical and Geophysical Fluid Dynamics
The group in Leeds is one of the leading groups in the field of Astrophysical and Geophysical Fluid Dynamics, with international reputation in dynamo theory, astrophysical MHD and convection. The strength of the group is recognised by the award of several prizes and special fellowships. The group also holds one of the largest grants ever awarded to the University of Leeds. The nine permanent members of staff work with eighteen postdocs and postgraduate students.

The group is actively engaged in research in a wide-range of areas of astrophysical and geophysical fluid dynamics: from planetary dynamics (the geodynamo and planetary dynamos) through solar, stellar and galactic dynamics to highly compressible and relativistic dynamics on the largest scales. Magnetic fields are a strong theme, and the group is interested in how planets (like the Earth), stars (like the Sun), neutron stars, black holes and galaxies generate their magnetic fields through dynamo action. On the Sun, the well-known eleven-year sunspot cycle is a manifestation of the solar dynamo; indeed the solar magnetic field underlies all solar magnetic phenomena such as solar flares, coronal mass ejections and the solar wind. In the Earth, magnetic fields are generated by convection in the molten iron core, and it has recently become possible to solve the fundamental equations that govern the motion of fluids and the generation of magnetic fields, and successfully reproduce many of the observed features of the geomagnetic field. At the other end of the scale, magnetic fields are implicated in the formation of spectacular jets coming from neutron stars, black holes and galaxies. Without magnetic fields, the group has interests in waves and hydrodynamic instabilities in rotating stratified fluids, with applications to the Earth's atmosphere and ocean (and with application to other planets).