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.)