PRESENTS

in physics, the temperature at which molecular movement virtually ceases and the lowest level of energy is reached; measures ?273.15o on the Celsius scale, ?459.67o on the Fahrenheit scale; temperature scales having absolute zero as their starting point, such as the Kelvin and Rankine scales, are called absolute temperature scales; idea of absolute zero originated with study of gas contraction at decreased temperatures

This lowest possible temperature is the same for all substances. Called absolute zero, it occurs at ?273.16o C, or ?459.69o F. The Kelvin and Rankine temperature scales use it as their zero point. Degrees on the Kelvin scale, commonly used in cryogenics, have the same range as degrees of the Celsius, or centigrade, scale. Degrees on the Rankine scale, used in the aerospace industry, have the same range as degrees of the Fahrenheit scale.

On an extremely cold Alaskan winter night, temperatures might drop to ?70o F (around 252 K). The cryogenic temperature range begins at an indefinite point much lower than this. The boiling point of oxygen?90 K?is in the high end of the range. Since even liquid hydrogen and helium are now produced commercially, scientists can begin cryogenic experiments with liquid helium, which has a boiling point of 4.2 K. Temperatures below 0.001 K have already been achieved. The theoretical limit for one method is five ten-millionths of a degree above absolute zero (0.0000005 K).

Although such temperatures appear to be very close to absolute zero, that temperature can never be reached. The third law of thermodynamics states this to be impossible. Just as there is no largest number?since no matter how large a number is written, another digit can be added to make it even larger?so too there is no smallest number. No matter how low a temperature is reached as 0.001 K shrinks to 0.0000001 K and below, temperatures even lower will always exist.

Under natural conditions a substance is cooled by placing it next to something colder. However, if the substance is to be made colder than anything in nature, work must be done to remove heat, and insulation must be provided to keep the substance cold.

Cryogenic cooling techniques use similar energy-transfer principles. Energy must first be introduced into a system (by compressing a gas, for example). This raises the temperature of the system. The excess heat energy flows out to the surrounding area, which cools the system to its original temperature. Then the system is insulated and made to do work (by allowing the gas to expand, for example). This step uses up some of the remaining heat energy and cools the system below the temperature of its surroundings.

Special techniques are used to reach temperatures around the millidegree (0.001 K) level. These techniques make use of the relationship, described by the second law of thermodynamics, between the amount of energy and the amount of disorder, or entropy, in a system. According to the second law, disorderly atoms within a system may be made more orderly (the entropy may be decreased) only if energy from outside the system is applied to the system.

Cooling by demagnetization depends on this relationship. A strong magnetic field provides the outside energy to line up the molecules of a paramagnetic crystal (see Magnet and Magnetism). This also raises the temperature. When the crystal cools back to the starting temperature, the field is removed and the molecules swing back to a disorderly arrangement. The energy they use to move comes from the heat energy of the crystal, so the temperature drops.

Unusual properties of helium at low temperatures make other cooling methods possible. For example, at certain temperatures liquid helium is more ordered (has less entropy) than solid helium, which can be formed only under pressure. If liquid helium is compressed at one of those temperatures, it solidifies. Unlike normal substances, helium at these special temperatures must absorb heat (increase its entropy), causing the temperature to drop when it solidifies. This technique does not require a magnetic field, which could interfere with some kinds of experiments.

Above 2.2 K liquid helium acts like a normal cryogenic fluid. But below that temperature helium-4, the most abundant isotope, acquires superfluidity. Superfluid helium runs quickly through tiny holes that would slow normal liquids, defies the laws of gravity by creeping up the sides of a container, and conducts heat a thousand times more efficiently than copper.

At varying low temperatures, some metals and metal alloys become superconductors. When the transition temperature for a given metal is reached, its electrical resistance completely disappears. Presumably, an electric current could run forever through an aluminum ring cooled to a temperature of about 1 K or through a lead ring cooled to about 7 K. The transition temperatures of some alloys are even higher.

Superconductors have been of limited use because they must be cooled with liquid helium, which is a rare and expensive substance. In the 1980s, however, a new class of high-temperature superconductive materials was discovered. These ceramic compounds of copper oxide with rare earth elements made the commercial application of high-temperature superconductivity more feasible. Many materials can superconduct at temperatures exceeding 90 K, which can be achieved at a low cost using liquid nitrogen.

High-temperature superconductors may reduce the costs of running particle accelerators, which currently use conventional superconductive electromagnets and require expensive cryogenic cooling techniques. Other possible applications include power transmission lines and magnetically levitated superfast trains. Superconducting computer elements, another industrial application of cryogenics, may also be improved with high-temperature superconductors.

The use of cryogenics in experiments in food preservation and the production of liquid natural gas for automobiles has increased. In medicine, cryogenics produces banks of tissues and organs for future surgical grafting and implantation; some embryos have been frozen and stored for later implantation as ?test-tube babies.?