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Stretched matter goes to unusual extremes.


Like a stretched rubber band, most materials become narrower in cross section when extended. A few materials, however, unexpectedly get fatter when stretched.

Researchers have now discovered an unusual combination of these effects. Certain stretched materials expand in one direction of their cross sections and contract in the other, while maintaining a constant volume. Theory and experimental observation suggest that such behavior could occur naturally in several forms of matter with extremely high or low densities.

Ray H. Baughman of the Honeywell Technology Center in Morristown, N.J., and his coworkers describe their findings in the June 16 SCIENCE.

This research provides "an intriguing glimpse into the strange properties of some unusual materials," comments Roderic Lakes of the University of Wisconsin-Madison “University of Wisconsin” redirects here. For other uses, see University of Wisconsin (disambiguation).
A public, land-grant institution, UW-Madison offers a wide spectrum of liberal arts studies, professional programs, and student activities.
. The results may prove important both in fundamental studies of matter under extreme conditions and for applications in sensors or devices for controlling light, he adds.

Poisson's ratio When a sample of material is stretched in one direction, it tends to get thinner in the other two directions. Poisson's ratio (ν, ), named after Simeon Poisson, is a measure of this tendency.  measures how much a stretched material's cross section decreases for a given increase in length. If a material's cross section expands upon stretching, its Poisson's ratio is negative (SN: 3/14/87).

Uniform materials with a negative Poisson's ratio increase in volume when stretched. But if a material has nonuniform properties, its Poisson's ratio might be negative in one direction and positive in another. In some instances, the effects would balance, leaving the stretched material's volume unchanged.

Astrophysicists An astrophysicist is a person who professionally studies and conducts research in astrophysics. Famous astrophysicists
  • Hannes Olof Gösta Alfvén (Sweden, 1908 – 1995)
  • Subrahmanyan Chandrasekhar (India, USA, 1910 – 1995)
 have proposed that the crusts of neutron stars neutron star, extremely small, extremely dense star, about double the sun's mass but only a few kilometers in radius, in the final stage of stellar evolution. Astronomers Baade and Zwicky predicted the existence of neutron stars in 1933.  and the cores of white dwarfs white dwarf, in astronomy, a type of star that is abnormally faint for its white-hot temperature (see mass-luminosity relation). Typically, a white dwarf star has the mass of the sun and the radius of the earth but does not emit enough light or other radiation to be  consist of ultradense metallic crystals Metallic crystal structure is that of metal atoms surrounded by a sea of valence electrons. Electrons are given by the metal atoms and belong to the crystal as a whole. The ability of outer-structure electrons to move throughout the crystal explains its high electric conductivity. . At high pressures, such a solid consists of well-separated atomic nuclei surrounded by a sea of free electrons. Such a material would be highly resistant to changes in volume.

Calculations by Baughman and his colleagues predict that these solids would have a large negative Poisson's ratio in certain directions balanced by a large positive ratio in others. They note that these properties might be used to determine the structure of neutron stars and white dwarfs from their vibrations.

Baughman and his colleagues suggest that similar behavior can occur in colloidal crystals Colloidal crystals

Periodic arrays of suspended colloidal particles. Common colloidal suspensions (colloids) such as milk, blood, or latex are polydisperse; that is, the suspended particles have a distribution of sizes and shapes.
, which consist of widely separated, regularly spaced microscopic particles suspended in a liquid; in assemblages of dust particles in electrically charged gases (SN: 8/6/94); and in laser-cooled ion crystals (SN: 1/31/98).

The researchers measured changes in the spacing of beryllium beryllium (bərĭl`ēəm) [from beryl ], metallic chemical element; symbol Be; at. no. 4; at. wt. 9.01218; m.p. about 1,278°C;; b.p. 2,970°C; (estimated); sp. gr. 1.85 at 20°C;; valence +2.  ions confined in a laser trap laser trap
n.
A device made of magnetic coils and tuned lasers in which atoms or particles are slowed and then confined to a small region of space. A laser trap is used to form a Bose-Einstein condensate. Also called atom trap.
 at millikelvin temperatures. They found that applying a force in the appropriate direction increased the distance between ion layers in a different direction, confirming that an ion crystal can exhibit a negative Poisson's ratio without a change in volume. By adjusting the setup, the researchers could also alter the value of Poisson's ratio.

The ability to adjust Poisson's ratio is potentially useful for employing sparse crystals as diffraction gratings for optical devices, Baughman notes.
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Author:Peterson, I.
Publication:Science News
Article Type:Brief Article
Geographic Code:1USA
Date:Jun 17, 2000
Words:461
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