Gravitational waves are yet to be directly detected and physicists from the University of Glasgow have been awarded a 4.2 million pounds Science & Technology Funding Council (STFC) grant to develop new technologies to test for their existence.
This research will be important for a worldwide network of detectors, including the German-UK GEO 600, the French-Italian Virgo, and the American Laser Interferometer Gravitational-Wave Observatory (LIGO) which are currently being upgraded to start hunting for these most elusive signals emanating from the deepest reaches of the Universe.
Gravitational wave astronomy provides unique tools for studying the destructive and creative forces at work in the Universe that are unobservable by other means and promise to lead to further breakthroughs in fields of astrophysics and cosmology.
In order to find evidence of gravitational waves, a team of researchers from the University of Glasgow are studying new materials and optical techniques to enhance the sensitivity of gravitational wave detectors.
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As gravitational waves from astronomical events ripple out across the universe they greatly decrease in amplitude and are tremendously difficult to measure by the time they reach and travel through the Earth.
The detectors which contain instrumentation developed the University of Glasgow will be capable of measuring with a sensitivity of around 1/1000th of the diameter of a proton.
Sheila Rowan, Professor of Physics and Astronomy at the University of Glasgow, said: "We are entering a very exciting time in the search for gravitational waves. Experiments aimed at detecting gravitational waves have been in development for several decades and we are now reaching sensitivity levels where detection is expected in the next few years."
In particular, space and time can dilate. Space and time should be considered together and in relation to each other and the speed of light is nonetheless invariant, the same for all observers.