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Physics News Update
Number 780, June 9, 2006 by Phil Schewe and Ben Stein

A Hint of Negative Electrical Resistance

A hint of negative electrical resistance emerges from a new experiment in which microwaves of two different frequencies are directed at a 2-dimensional electron gas. The electrons, moving at the interface between two semiconductor crystals, are subjected to an electric field in the forward (longitudinal) direction and a faint magnetic field in the direction perpendicular to the plane. In such conditions the electrons execute closed-loop trajectories which will, in addition, drift forward depending on the strength of the applied voltage.

A few years ago, two experimental groups observed that when, furthermore, the electrons were exposed to microwaves, the overall longitudinal resistance could vary widely -- for example, increasing by an order of magnitude or extending down to zero, forming a zero-resistance state, depending on the relation between microwave frequency and the strength of the applied magnetic field (for background, see Physics Today, April 2003).

Some theorists proposed that in such zero-resistance state, the resistance would actually have been less than zero: the swirling electrons would have drifted backwards against the applied voltage. However, this rearwards motion would be difficult to observe because of an instability in the current flow -- that is, the current distribution becomes inhomogeneous so as to yield a vanishing voltage drop.

A Utah/Minnesota/Rice/Bell Labs group has now tested this hypothesis in a clever bichromatic experiment using microwaves at the two frequencies. Michael Zudov (now at the University of Minnesota, zudov@physics.umn.edu, 612-626-0364) and Rui-Rui Du (now at Rice University) sent microwaves of two different frequencies at the electrons, observing that for nonzero-resistance states the resultant resistance was the average of the values corresponding to the two frequencies separately. On the other hand, when the measurements included frequencies that had yielded a zero resistance, the researchers observed a dramatic reduction of the signal.

Judging from the average resistance observed for non-zero measurements, they deduce that whenever zero resistance was detected, the true microscopic resistance had actually been less than zero. In other words, an observed zero resistance was masking what was in fact an unstable negative- resistance state.

Zudov et al., Physical Review Letters, 16 June 2006
Contact Michael Zudov, University of Minnesota
zudov@physics.umn.edu, 612-626-0364

Your Neighbors Would Love You on Mars

On Mars, no one could hear a lawn mower's sound farther than a couple of hundred feet -- compared to the several miles it can travel on Earth -- according to a new computer simulation of sound propagation on our next-door planetary neighbor.

In general, what do things sound like on Mars? At this week's meeting of the Acoustical Society of America in Providence, R.I., Amanda Hanford (ald227@psu.edu) and Lyle Long of Pennsylvania State University presented detailed computer calculations that simulate how sound travels through the Martian atmosphere, which is much thinner than Earth's (exerting only 0.7 percent of the pressure of our atmosphere on the surface) and has a very different composition (containing 95.3 percent carbon dioxide, compared to about 0.33 percent on our planet).

The loss of 1999's Mars Polar Lander, which was to record sounds directly on the planet, has compelled researchers to find other means to study how sound travels there. To determine the behavior of sound on Mars, the researchers analyzed how gas molecules move and collide in its atmosphere. The researchers took into account the gas molecules' mean free path, the average distance a molecule travels before it collides with a neighbor (6 microns, compared to 50 nanometer on Earth). They also considered the different ways in which gas molecules could exchange energy when colliding with each other.

In their computational approach, known as direct simulation Monte Carlo, collisions occurred randomly, though at a statistically accurate rate. Accounting for the different combinations of molecule species that could collide along with the many different ways in which they could lose or gain energy required a huge amount of computation -- over 60 hours -- even for simulating a small patch of atmosphere for every sound frequency they considered, using a 32-processor "Beowulf" computer cluster that was one of the most powerful computers in the world. With their approach, the researchers could determine all physical properties of interest in the propagation of sound on Mars.

The researchers' results show that the absorption of sound on Mars is 100 times greater than it is on Earth, because of the differences in molecular composition and lower atmospheric pressure. Owing to computational considerations (they could only analyze collisions over a relatively small region of space), the researchers only simulated the propagation of lower-wavelength sounds (with frequencies in the ultrasound regime) but extrapolated the results down to audible frequencies.

Paper 2aPA3 at the American Acoustical Society meeting
Also see Computer Simulations of the Propagation of Sound on Mars, a lay-language paper on the ASA meeting's Web site
Contact Amanda Hanford, Pennsylvania State University
ald227@psu.edu

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