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Physics News Update
Number 682, April 21, 2004 by Phil Schewe and Ben Stein

Exoplanet Detected Using Microlensing

The presence of a planet orbiting a distant star has been deduced not by the customary method of observing a slight change in the star's spectrum when tugged by the planet but rather by the way in which a foreground star (17,000 light years away) and its attendant planet distort the image of a background star (some 24,000 light years away) through the process of gravitational lensing. Several detector groups are set up to monitor the passage of stars in the Milky Way passing behind or near foreground objects (dark matter? brown dwarfs? other stars?) and to make sense of changes in the light curve for the background objects.

Ian Bond of the Institute for Astronomy in Edinburgh, Scotland and his colleagues at two detector groups, the Microlensing Observations in Astrophysics (MOA) and Optical Gravitational Lensing Experiment (OGLE) report that in the case of one distant star the characteristic brightening light curve (heralding a lensing event) bore some extra spikes indicative of a lensing object consisting of two parts. Further analysis showed that the one object was only 0.4% as massive as the other, suggesting a star-planet pairing. The presumed planet has a mass of 1.5 Jupiters. (Bond et al., Astrophysical Journal Letters, 10 May 2004.)

Parity Violation in Electron-Electron Scattering

Parity violation in electron-electron scattering has been seen for the first time, adding to physicists' understanding of the elusive weak force. Parity is name for the proposition that if one viewed an interaction among particles in a special mirror that reflected in all three dimensions then physics would be the same in the ordinary and in the mirror world. Three of the four known physical forces---gravity, electromagnetic, and strong---respect (or "conserve") parity. The fourth force, the weak force, does not conserve parity, a fact established in the 1950s by watching the decays of cobalt nuclei. Since then parity violation has also been observed in other reactions, such as transitions between energy levels within atoms and electron-positron annihilations, but never before in low-angle, relatively low-energy electron-electron scattering.

Electrons are non-nuclear particles; so why do they scatter via any kind of nuclear force, much less the weak nuclear force? Because the weak and electromagnetic forces, though normally very different in their attributes (the electromagnetic force keeps atoms together and governs light, while the weak force exerts itself only at very short range, within about the size of a proton, and is responsible for some kinds of radioactivity) the two forces are still, properly speaking, parts of a single underlying "electroweak" force. Therefore even though electrons interact chiefly through the electromagnetic force, there is enough admixture of weak-force to make itself felt, albeit only in an experiment of great delicacy.

Researchers at SLAC scattered a high-energy beam of polarized electrons off electrons in a liquid hydrogen target and measured the fractional difference in scattering rates when the intrinsic spin of the beam electrons were lined up with or against the direction of the beam. The observed asymmetry not only demonstrated that a bit of parity-violating force was present (in keeping with theoretical ideas about the weak force) but also provided a measure---in fact, the first quantitative measure---of the electrons' "weak charge," a commodity, analogous to electric charge, and indicative of the strength of the weak interaction between two electrons.

One of the team members, Krishna Kumar of the University of Massachusetts (kkumar@physics.umass.edu), asserts that the statistical error of 30 parts per billion (ppb) is the most precise measurement of an asymmetry (the measured effect was 175 parts per billion) in a lepton scattering experiment (that is, one involving electrons, muons, or neutrinos). (Anthony et al., Physical Review Letters, upcoming article.)

A Land Speed Record for Data Flow

A land speed record for data flow, 6.25 gigabits per second (average rate) moving over an 11,000-km course, has been set a consortium of scientists form the CERN lab in Geneva and Caltech in Pasadena. This new result was announced at the Spring 2004 Internet2 Member Meeting in Arlington, Virginia. The World Wide Web got its start at CERN, where particle physicists had to find ways of sending huge loads of data to collaborators. CERN will again need huge flow rates, perhaps at the 10-gigabit-per-second level, when they begin physics experiments at the Large Hadron Collider (LHC) now under construction. (More information at Caltech website.)

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