Superconductivity

related topics
{math, energy, light}
{acid, form, water}
{system, computer, user}
{work, book, publish}
{son, year, death}
{car, race, vehicle}
{style, bgcolor, rowspan}

Superconductivity is an electrical resistance of exactly zero which occurs in certain materials below a characteristic temperature. It was discovered by Heike Kamerlingh Onnes in 1911. Like ferromagnetism and atomic spectral lines, superconductivity is a quantum mechanical phenomenon. It is also characterized by a phenomenon called the Meissner effect, the ejection of any sufficiently weak magnetic field from the interior of the superconductor as it transitions into the superconducting state. The occurrence of the Meissner effect indicates that superconductivity cannot be understood simply as the idealization of perfect conductivity in classical physics.

The electrical resistivity of a metallic conductor decreases gradually as the temperature is lowered. However, in ordinary conductors such as copper and silver, this decrease is limited by impurities and other defects. Even near absolute zero, a real sample of copper shows some resistance. Despite these imperfections, in a superconductor the resistance drops abruptly to zero when the material is cooled below its critical temperature. An electric current flowing in a loop of superconducting wire can persist indefinitely with no power source.[1]

In 1986, it was discovered that some cuprate-perovskite ceramic materials have critical temperatures above 90 K (−183 °C). These high-temperature superconductors renewed interest in the topic because of the prospects for improvement and potential room-temperature superconductivity. From a practical perspective, even 90 kelvins is relatively easy to reach with the readily available liquid nitrogen (boiling point 77 kelvins), resulting in more experiments and applications.

See also the history of superconductivity.

Contents

Full article ▸

related documents
Pressure measurement
Electromagnetic radiation
Modified Newtonian dynamics
Lorentz force
Kinematics
Lagrangian point
Magnet
Magnetohydrodynamics
Thermodynamic temperature
Cosmic ray
Black body
Gravitational lens
Standard Model
Fluid dynamics
Atomic orbital
Bose–Einstein condensate
Casimir effect
Lens (optics)
Kilogram
Polar coordinate system
Mercury (planet)
Sundial
Nuclear magnetic resonance
Angular momentum
Langmuir probe
Photoelectric effect
Light pollution
Ohm's law
Roche limit
Navier–Stokes equations