The word "cryogenic" is Greek and roughly translates to mean "to generate cold." At a recent in-house technology lecture, David Grillot, head of ITER's Cryogenic Project Team and introduced as the "coolest guy" at ITER, took his audience on a journey into the world of the ultra-chilled.
In common household refrigerators
temperatures are normally around 5 °C. In a freezer they go down to -18 °C. Cryogenics begins at temperatures lower than -153 °C (120 K) because it is below this point that the first of the cryogenic fluids begin to liquefy. The bottom limit is of course absolute zero: 0 K or -273 °C—the point at which all particle motion stops.
The age of cryogenics began toward the end of the 19th century, when scientists managed to liquefy air for the first time. Following the successful liquefaction of oxygen, nitrogen, hydrogen and argon, helium entered the stage in 1908 as the last of the cryogenic gases. The first droplets were produced at a temperature of 4 K, establishing helium as the coldest liquid in existence.
Since the middle of the 20th century, the field of cryogenics has advanced to such an extent that its applications today can be found everywhere—in the energy, food, health and space industries, and throughout science research.
What makes cryogenics so interesting for scientists and engineers is the effect of cryogenic temperatures on the thermal, mechanical and electrical properties of materials. Grillot's team members Marie Cursan and Denis Henry demonstrated, for example, the loss of ductility in a length of rubber, breaking a newly rigid section with relative ease after they had dunked it in liquid nitrogen.