The link between the deep Earth and its dynamic surface. Modelling the two-way interaction of plate tectonics with the actions of erosion and sedimentation gives a fundamentally new view of the dynamics of our planet and the importance of the surface on the deep interior. It will improve our understanding of the formation of sedimentary basins, their evolution and their preservation over geological time.
The formation of stars and planets. This project will identify the mechanisms that create stars and planets, providing a sound basis for studying the birth of planetary systems with next-generation telescopes. It will maintain Australia's position at the forefront of astronomy and the advanced computational methods we shall develop will have applications in many other fields.
How do sediments become magnetised? Construction of an empirical-numerical framework. The magnetism of sediments provides information on the past behaviour of the Earth's magnetic field. This project will study sediments from the oceans around Australia to understand how the field was recorded and use this information to construct a new generation of computer models that will provide insights into the physics of the recording process.
The key role of black holes in galaxy evolution. This project will determine the effect of black holes on galaxy formation using sophisticated supercomputer simulations of radiation, jets and winds interacting with multi-phase interstellar gas in the host galaxy. The results of these simulations will be calibrated against radio and optical observations and incorporated into larger scale simulations describing the growth of structure in the Universe and the evolution of galaxies. This research is ....The key role of black holes in galaxy evolution. This project will determine the effect of black holes on galaxy formation using sophisticated supercomputer simulations of radiation, jets and winds interacting with multi-phase interstellar gas in the host galaxy. The results of these simulations will be calibrated against radio and optical observations and incorporated into larger scale simulations describing the growth of structure in the Universe and the evolution of galaxies. This research is highly relevant to the future science programs of the Giant Magellan Telescope and the Square Kilometre Array.Read moreRead less