Printer Friendly

Unworldy pressures: scientists put the supersqueeze on gases, metals and minerals.

Unwordly Pressures

By squishing materials in the clenched jaws of a diamond vise, scientists are striving to achieve the ultimate tight squeeze. In so doing, at least one team may have pinched a new record for the largest pressures ever sustained in a laboratory -- super-squeezes soiintense that they apparently exceed even the colossal pressures exerted at the center of the Earth.

Attaining these exotically high pressures intthe lab enables geophysicists to mimic conditions deep within the Earth and other planets, and provides physicists with valuable experimental checks onttheories about atomic and molecular behavior.

In the December 1990 REVIEW OF SCIENTIFC INSTRUMENTS, researchers at Cornell University report squeezing a microscopic sample of molybdenum powder to a pressure of 4.16 million bars (megabars). Earth's atmosphere exerts approximately 1 bar; the planet's center exerts an estimated 3.61 megabars. The Cornell team, led by materials scientist Arthur L. Ruoff, also reports squeezing tungsten and other samples to somewhat lower pressures.

The 4.16-megabar squeeze probably represents a world record, Ruoff told SCIENCE NEWS. Then again, it may only approach record status. The answer depends on which big-squeeze researchers you talk to and how they choose to calibrate such huge pressures.

In 1986, a research team headed by Hokwang Mao at the Carnegie Institution of Washington (D.C.) and a separate group led by William C. Moss at Lawrence Livermore (Calif.) National Laboratory reported measuing 5.5- and 4.6-megabar pressures in their diamond vises, also known as diamond anvil cells. Those values depend on a calibration method involving the laser-induced fluorescence emitted by tiny ruby crystals squeezed within the anvil, a method Ruoff considers suspect at pressures above 1.8 megabars.

Mao readily acknowledges that the ruby fluorescence technique harbors uncertainties, but he points out that Ruoff's calibration method has limitations of its own. "To claim that their pressures are definitely higher than anybody else's, or that the ruby fluorescence technique is inadequate, is premature," Mao says.

To be sure, no simple barometer exists for ultrahigh pressures. Researchers instead must rely on physical inferences and mathematical extrapolations that are based on more readily measurable properties of the materials under pressure. Debates about the merits and pitfalls of different clibration methods are endemic to high-pressure research.

Technical uncertainties notwithstanding, high-pressure scientists are observing gases, metals and minerals under conditions never before produced in laboratories, or perhaps anywhere else on the planet. For instance, Mao and his co-workers have been squeezing hydrogen gas so tightly that it reorganizes into a solid and displays hints that it might even become a metal -- maybe even a superconducting metal, according to calculations by others. At last December's meeting of the American Geophysical Union in San Francisco, Mao reported data from several studies on iron hydride, which he says may be the most abundant material in Earth's core. He also described experiments in which his team pressed graphite into a new molecular arrangement -- one apparently strong enough to break the anvil. Each diamond jaw can cost as much as $1,500, Ruoff notes.

The Cornell researchers, too, have uncovered strange material effects in their supersqueeze experiments. They find, for example, that extreme pressures dramatically distort the normal cubic arrangement of carbon atoms in the anvil's diamond, squashing the atoms into a highly strained structure. This "surprising" distortion, says Ruoff, shows up as a colorful effect called birefringence, in which light bends at different angles as it passes through the stressed material.

The Cornell team has also pulled off an offbeat sort of alchemy. Under megabar pressures, samples of zirconium and hafnium -- so-called rare earth or transition mettal elements -- show substantial changes in shape and chemical character. Their crystal structures and the arrangement of their valence electrons (the ones that participate in chemical bonds) reshuffle, Ruoff says, to match those of the unstressed elements in the column to the right on the periodic table -- namely, niobium and tantalum.

CWhen you press things really hard, you change the distances between their atoms," he explains. Since the Cornell researchers can maintain multimegabar pressures for weeks in their diamond anvil cells, they can precisely determine these interatomic distances with X-ray crystallography. But since their samples are small -- about the size of a mist particle -- they need an especially bright source of X-rays. The Cornell High-Energy Synchrotron Source fills the bill, shining an intense X-ray beam through the anvil's diamond jaws, which conveniently double as observation windows.

Crystallography alone cannot furnish a quantitative measure of pressure. Researchers must also apply some physical chemistry and mathematics in the form of "equations of state" -- formulas expressing the relationship among a material's temperature, pressure and volume. Only the volume data come directly from crystallography studies.

The Cornell crew uses a specific equation derived by other investigators who performed "shock experiments," in which explosions or high-speed impacts squeeze targets such as tungsten pellets to enormous pressures (up to tens of megabars or more), but only for a few millionths of a second. The velocity of sound waves emerging from these shocks provides information about the target's properties, such as stiffness. This, in turn, serves as an indicator of the pressure on the shocked target material.

Mao warns that minute geometric irregularities in these targets might easily yield complex acoustic signals that could introduce an error of as much as 0.5 megabar into subsequent pressure calculations based on the shock experiments.

Ruoff acknowledges this possibility, but he claims that at higher pressures, the ruby fluorescence calibration used by the Carnegie and Livermore groups suffers from more troublesome uncertainties. Above 1.8 megabars, he says, the ruby fluorescence signal fades and disappears, and a second fluorescence signal then appears. Mao and others interpret that signal as coming from the ruby at higher pressures, but Ruoff remains unconvinced.

"A lot of things could have happened" during the ruby fluorescence "blackout," he says. Thus, the assumption that the same fluorescence-pressure relation holds both before the ruby fluorescence dims and after the second fluorescence appears is shaky at best, Ruoff contends. The tiny ruby crystals may have undergone a change in crystal structures, or the increased pressure may have induced unanticipated fluorescence from the diamond, he suggests.

Mao counters that the ruby's fluorescence never completely disappears, but instead becomes very faint as a stronger fluorescence from the diamond temporarily competes with it.

That's still not enough for Ruoff. In August 1988, he and colleagues reported observing diamond fluorescence at about 2.5 megabars, which he thinks could have misled Mao's group to calculate a 5.5-megabar pressure. Similar subtleties may have led Moss team at Livermore to measure 4.6 megabars in their vise, he adds. If Ruoff is right, then the recent 4.16-megabar reading at Cornell might indeed mark a record high.

The potential pitfalls of both calibration methods place pressure investigators between a rock and a hard place. "The high-pressure business is very tough," Ruoff says, and he gets no argument from Mao on that. But with much to learn about how materials cope in the big squeeze, the researchers intend to press on.
COPYRIGHT 1991 Science Service, Inc.
No portion of this article can be reproduced without the express written permission from the copyright holder.
Copyright 1991, Gale Group. All rights reserved. Gale Group is a Thomson Corporation Company.

Article Details
Printer friendly Cite/link Email Feedback
Author:Amato, Ivan
Publication:Science News
Date:Feb 2, 1991
Words:1176
Previous Article:Starbirth may guide galactic chemistry.
Next Article:Pediatric pain: helping sick children cope with medical pokes and probes.
Topics:


Related Articles
Squeezed hydrogen turns semi-metallic.
Diamond fever: new ways of coating just about anything with diamond may spawn a sparkling new industry.
Journey to the center of the earth.
The lightest metal in the universe; scientists make a fleeting metal from hydrogen.
Diamonds from outer space.
Radiation helps break down toxic waste.
Undersea Riches.
In a squeeze, nitrogen gets chunky.
Rocks in Earth's mantle could hold five oceans. (Earth Science).
Deep seas, dark worlds: deep-sea vents create cozy homes for some of Earth's weirdest life forms.

Terms of use | Copyright © 2016 Farlex, Inc. | Feedback | For webmasters