The resistance to motion between contacting surfaces, absent in superfluids.Friction is the resistance to relative motion between two surfaces in contact. It arises from the microscopic interactions of surface asperities, including adhesion, deformation, and plowing. Friction is not a fundamental force but a macroscopic manifestation of electromagnetic forces between atoms and molecules. It plays a crucial role in everyday life, from walking and writing to braking and machinery, and its absence in superfluids and superconductors leads to remarkable phenomena like persistent flow without energy loss.
The classical laws of friction were formulated by Leonardo da Vinci and later formalized by Guillaume Amontons in 1699 and Charles-Augustin de Coulomb in 1785. The modern understanding of friction as a multi-scale phenomenon developed in the 20th century with contributions from Bowden and Tabor.
When two surfaces slide, the real contact area is only a small fraction of the apparent area, consisting of microscopic peaks (asperities) that deform and bond. The friction force is proportional to the normal load, with a proportionality constant called the coefficient of friction. At the atomic scale, friction involves the excitation of phonons and electrons, dissipating kinetic energy as heat. In superlubricity, certain crystalline surfaces can slide with nearly zero friction due to incommensurate atomic lattices that cancel lateral forces.
Friction is engineered in brakes, tires, and clutches for safety, and minimized in bearings, lubricants, and microelectromechanical systems to reduce wear and energy loss.
In superfluids, friction vanishes entirely, allowing liquid helium to flow through microscopic cracks and even climb up and over the walls of its container.






