Gravitational waves, predicted by Einstein's theory of general relativity,
are ripples in the curvature of spacetime which propagate at the speed of light.
They are emitted in the most violent events in the universe such as supernovae,
coalescence of neutron stars and black hole collisions. The ideal instrument
to detect them is a giant laser interferometer with suspended mirrors. It must
be able to detect a length change of at least 10-20m in 1 km.
To reach this level of sensitivity much research and development into ways to
build these instruments is needed. Projects will develop skills in a number
of highly employable areas such as: optics, electro-optics, electronics, control
systems, isolation systems and modelling.
We also have research projects which aim to develop spin-off technology into
commercial products, for example high sensitivity trace gas analysis, laser
intensity and frequency stabilization techniques, high-sensitivity low-power
alternatives to LiDaR and more.
All honours projects will be undertaken in the Gravitational Wave Facility
in the Department of Physics. For further information contact Prof.
David McClelland or just come and visit us in the Gravitational Wave Building
in the Department of Physics.