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Research at CSPA

Research at CSPA is focussed in several groups as well as a range of individual research interests. The main research groups are listed below. Information about particular research topics can be found by following the links.

SINS: Stellar interiors and nucleosynthesis MonGRels: Monash General Relativists

The SINs group studies the structure and interior evolution of stars as well as the nuclear elements they produce.

Monash has a large group of researchers working in many areas of both Classical and Numerical General Relativity.
Clique du Soleil: Solar Physics SPH: Smoothed Particle Hydrodynamics

The Solar Physics group is mainly concerned with understanding magnetic activity in the sun using helioseismology.

SPH is a numerical technique for solving the equations of fluid dynamics, developed strongly here at Monash and being applied widely in astrophysics and geophysical fluid dynamics.
Gravitational dynamics High Energy Astrophysics
The dynamics group studies small-N systems, in particular extrasolar planetary systems including the effects of moons, tides, spin-orbit coupling and relativity, and the dynamics of small-N systems in dense stellar systems. Three-body stability is central to much of our work. High Energy Astrophysics involves understanding some of the most violent objects in the universe, such as supernovae and the neutron stars they leave behind.

Other research topics at CSPA include:

Galaxy Evolution Particle Cosmology
The Formation of the Solar System Star Formation
Active Galaxies Binary Stars and the Early Universe
Supernova Remnants Black Holes
Neutron Star Binaries Particle Astrophysics of the Galactic Centre