
The process of reducing the temperature of a system.Cooling is the deliberate removal of thermal energy from a system, lowering its temperature. In physics, cooling is not just about comfort—it is a gateway to quantum phenomena. At temperatures near absolute zero, thermal fluctuations become negligible, and quantum effects such as superconductivity, superfluidity, and Bose-Einstein condensation emerge. Cooling also improves the sensitivity of detectors by reducing thermal noise, which is why many astronomical instruments and quantum computers operate at millikelvin temperatures.
The first liquefaction of helium by Heike Kamerlingh Onnes in 1908 opened the door to cryogenics, and his subsequent discovery of superconductivity in 1911 was a direct result of achieving temperatures below 4.2 K.
Cooling methods vary by regime. For moderate cooling, refrigeration cycles use compression and expansion of gases. For reaching microkelvin temperatures, physicists use techniques like laser cooling, where photons scatter off atoms and carry away momentum, or nuclear adiabatic demagnetization, where the magnetic entropy of nuclear spins is reduced by slowly lowering an external magnetic field. Each method exploits a different physical mechanism to extract entropy from the system.
Cooling is essential in MRI machines, superconducting magnets for particle accelerators, and quantum computers that require near-zero temperatures to maintain qubit coherence.
Laser cooling can bring atoms to temperatures below one microkelvin—colder than the average temperature of interstellar space.















