BBC - Future - Science & Environment - Bored? Hunt for dark matter in your spare time t is the next â€œbig huntâ€ in modern physics. Following confirmation of the existence of the Higgs Boson earlier this year, physicists now have their eyes on dark matter. With more than four times as much of the elusive stuff believed to be out there than visible matter, finding it would be of arguably even greater significance than the discovery that gained Peter Higgs and FranÃ§ois Englert the Nobel prize last month. Now more people than ever are joining the search party, even non-scientists in their spare time. Itâ€™s probably not worth turning out your cupboards to see if thereâ€™s any dark matter lurking at the back, but there is a way that you can contribute â€“ at least, if you have the right skills. Physicists believe dark matter exists because without its gravitational pull, galaxies would fly apart. Yet we can't actually see the stuff because it doesnâ€™t appear to absorb or emit light. There are several theories for what dark matter might be, but they all have to start from negative clues: what we donâ€™t know, or what it doesnâ€™t do. The current favourite invokes a new fundamental particle called a weakly interacting massive particle (Wimp). â€œWeakly interactingâ€ means Wimps can, in theory, pass straight through ordinary matter, but occasional collisions with it generate little bursts of light with no other discernible cause. Such flashes would be the telltale signs of dark matter. Several dark-matter detectors looking for these rare dark-matter flashes are underground, at the bottom of deep mineshafts. One such experiment called LUX looks for collisions of Wimps in a tank of liquid xenon 1.6km underground in a mine in South Dakota. The scientists running LUX recently reported that none had been identified during the first few months it has been in operation. This might not be such a big deal if it wasnâ€™t for the fact that some earlier experiments have reported a few unexplained events that could possibly have been caused by Wimps. As LUX is one of the most sensitive dark-matter experiments currently operating, the new results suggest that the earlier, enticing findings were a false alarm. At the same time, on board the International Space Station, the Alpha Magnetic Spectrometer (AMS) experiment is looking for signals from the mutual annihilation of colliding Wimps. And there are hopes that the Large Hadron Collider at Cern in Geneva might, once it resumes operations next year, be able to conduct particle smashes at the energies which might produce Wimps from scratch. In the meantime, the more information we can collect about dark matter in the cosmos, the better placed we are to figure out where and how to look for it. Thatâ€™s the motivation for making more detailed astronomical observations of galaxies where dark matter is thought to reside. Doing so could help to deduce basic properties of the mysterious particles, such as whether they are "cold" and easy slowed down by gravity, or hot and thus less easily retarded. Bent light One way of doing this is to look for dark matter via its â€œgravitational lensingâ€ effect. As Einsteinâ€™s theory of general relativity predicted, gravitational fields can bend light. This means that dark matter can act like a lens: the light coming from distant objects can be distorted when it passes by a dense clump of matter. David Harvey of the University of Edinburgh, Thomas Kitching of University College London, and their coworkers are using this lensing effect to find out how dark matter is distributed in galaxy clusters, where dark matter can outweigh ordinary matter by a factor of up to 100.