lower ones, this will not constitute proof for Hogan's hypothesis. It would, however, provide a strong motivation for further study. The sensitivity of GEO600 will then be significantly improved by using 'squeezed vacuum' and by the installation of a mode filter in a new vacuum chamber. The technology of 'squeezed vacuum' was particularly refined in Hannover and would be used in a gravitational wave detector for the first time. "We are very eager to find out what we can learn about the possible holographic noise over the course of the coming year", says Prof. Dr. Karsten Danzmann, director of the Hannover Albert-Einstein-Institute. "GEO600 is the only experiment in the world able to test this controversial theory at this time. Unlike the other large laser interferometers, GEO600 reacts particularly sensitively to lateral movement of the beam splitter because it is constructed using the principle of signal recycling. Normally this is inconvenient, but we need the signal recycling to compensate for the shorter arm lengths compared to other detectors. The holographic noise, however, produces exactly such a lateral signal and so the disadvantage becomes an advantage in this case. You could say that this has placed us in the very centre of a tornado in fundamental research!" "Scientists at Fermilab have decided that it's high time they build a 'holometer' to test the smoothness of space-time. Theoretical physicists like Stephen Hawking have proposed that space-time is not smooth but it's been a lot of math and no actual data. The Fermilab team