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Physics News Update
Number 784, July 7, 2006 by Phil Schewe and Ben Stein

Red Oxygen

A new evolutionary crystallography algorithm predicts the structure of crystals under a range of extreme pressure and temperature conditions on the basis of the chemical composition alone. One of these crystals would be a form of red-colored oxygen. Predicting crystal structures is difficult even for simple solids, partly because of the task of sorting among the astronomical number of possible ways given atoms can compose a basic repeatable unit cell.

Artem Oganov, a scientist at the Swiss Federal Institute of Technology (ETH) in Zurich, in Switzerland, and Colin Glass, a Ph.D. student, approach the problem by combining electronic structure calculations and a specifically developed evolutionary algorithm. In exploring the myriad atomic arrangements, they proceed in a step-by-step, continual-optimization fashion that avoids configurations less likely to succeed. This makes the algorithm very efficient and allows the researchers to make certain specific predictions.

One example is calcium carbonate (CaCO3) at very high pressures. Oganov's team for the first time predicted two new stable structures for this mineral. By now, both structures have been confirmed in experiments by Japanese colleagues. Oganov and Glass have also solved the structures crystalline oxygen at high pressure.

Oxygen is unique from the chemical point of view. The only magnetic molecular element known, under pressure it loses its magnetism and turns red. The structure of red oxygen, which remained unknown for a long time, seems to be finally solved and turns out to be unique; that is, it does not manifest itself in any other element. At even higher pressure oxygen is known to turn black in color and become superconducting, which happens because of the increased interactions between the O2 molecules. The ETH researchers also predict a new stable phase of sulphur and several new metastable forms of carbon.

Oganov and Glass, Journal of Chemical Physics, 28 June 2006
Contact Artem Oganov, ETH Laboratory of Crystallography
+41-(0)44-632-37-52, a.oganov@mat.ethz.ch
Artem Oganov's Web page

Squeezed Light and Gravity Waves

A proven method for reducing the noise in high-precision optical measurements will soon be applied to the search for gravitational waves. The most likely way such waves will be detected is by observing their subtle effects on suspended mirrors in detectors such as the Laser Interferometer Gravitational-wave Observatory (LIGO).

At LIGO, laser light is split into two beams which reflect many times from mirrors suspended at the ends of two long pipes positioned at right angles. The two beams are brought back together to form an interference pattern. This procedure is adjusted so that a photodetector is positioned at a null in the pattern; that is, it normally sees no photons coming its way. The plan is that a passing gravity wave would ever so slightly move the suspended mirrors in the two pipes (which are otherwise insulated from ordinary kinds of vibration) relative to each other, which in turn would disturb the interference pattern. Suddenly the photodetector would record photons, heralding a gravity wave.

One problem with this scheme is "shot noise," the quantum-based uncertainty in our knowledge of how many photons are present in a laser beam at any moment. Fluctuations in photon number could trigger a false positive reading.

Physicists at the Max Planck Institute for Gravitational Physics in Hannover, Germany, and the University of Hannover are hoping to reduce the quantum noise inherent in this interferometric approach to gravity wave detection by squeezing light. Squeezed light is produced when quantum noise in one or the other of two complementary variables describing a light beam (such as phase and amplitude) is greatly reduced at the expense of the other by sending the light through (a series of) special optical crystals.

The use of squeezed light reduces quantum noise in a number of optoelectronic applications. Usually the squeezed light approach is applied at megahertz frequencies, but the Hannover researchers have for the first time gotten it to work at all the detection frequencies pertinent for LIGO including frequencies below a hundred hertz, the expected frequency range of gravitational waves arriving from some distant coalescing black holes in the universe. According to Henning Vahlbruch (henning.vahlbruch@aei.mpg.de) a squeezed-light control scheme would help reduce noise and raise the sensitivity of gravity wave detectors.

Vahlbruch et al., Physical Review Letters, 7 July 2006
Contact Henning Vahlbruch, Max Planck Institute for Gravitational Physics
henning.vahlbruch@aei.mpg.de
Web site of Roman Schnabel's lab

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