Computational Modelling Group

Astrophysics

Astrophysics is broadly characterized as the physics of non-terrestrial objects. This could include small objects in our solar system or, through cosmology, the study of the entire universe. At present most projects here study extreme astronomical objects such as black holes, neutron stars and accretion disks.

For queries about this topic, contact Ian Hawke.

View the calendar of events relating to this topic.

Projects

Cosmological evolution of supermassive black holes in the centres of galaxies

Anna Kapinska (Investigator)

Radio galaxies and quasars are among the largest and most powerful single objects known and are believed to have had a significant impact on the evolving Universe and its large-scale structure. Their jets inject a significant amount of energy into the surrounding medium, hence they can provide useful information in the study of the density and evolution of the intergalactic and intracluster medium. The jet activity is also believed to regulate the growth of massive galaxies via the AGN feedback. In this project, through the use of numerical simulations, I explore the intrinsic and extrinsic physical properties of the population of Fanaroff-Riley II (FR II) objects, i.e. their kinetic luminosities, lifetimes, and central densities of their environments. This allows one to investigate evolution of these radio sources across cosmic time, and to discuss the significance of the impact of these sources on the evolving Universe.

Gravitational waves from neutron stars

Ian Hawke (Investigator)

Gravitational waves, once detected, will give information about the extremes of space and time. Compact objects such as neutron stars are perfect locations for generating such waves.

Numerical Elastic Neutron Stars

Ian Hawke, Ian Jones (Investigators), Andrew Penner

We study the gravitational wave forms that radiate from an asymmetric neutron star using an elasto-hydrodynamic model.

Relativistic multifluids

Ian Hawke (Investigator)

Multiphase flow is a central model in fluid dynamics. Its extension to relativity is crucial for tackling many astrophysics problems, and has fascinating mathematical features.

Self-Force and Black Hole Inspirals

Sam Dolan (Investigator)

We use IRIDIS to compute the self-force acting on a solar-mass black hole orbiting a supermassive black hole.

Whisky Code

Ian Hawke (Investigator)

A 3D finite volume code for simulating compact relativistic hydrodynamics.

People

Carsten Gundlach
Professor, Mathematics (FSHS)
Gwenael Gabard
Lecturer, Institute of Sound & Vibration Research (FEE)
Ian Hawke
Lecturer, Mathematics (FSHS)
Ian Jones
Lecturer, Mathematics (FSHS)
Sam Dolan
Research Fellow, Mathematics (FSHS)
Tim Lemon
Postgraduate Research Student, Mathematics (FSHS)
Justin Lovegrove
Postgraduate Research Student, Mathematics (FSHS)
John Muddle
Postgraduate Research Student, Mathematics (FSHS)
Elena Vataga
Technical Staff, iSolutions
Petrina Butler
Administrative Staff, Research and Innovation Services
Anna Kapinska
Alumnus, ICG, University of Portsmouth
Andrew Penner
Alumnus, Mathematics (FSHS)