A continuous range of energy states in a system, where resonances are usually smeared out.In physics, a continuum refers to a continuous range of possible energy values that a quantum system can possess, as opposed to discrete bound states. For example, a free electron has a continuous spectrum of kinetic energies, while an electron bound to a proton has only specific discrete energy levels. In scattering and resonance phenomena, the continuum is the background of states through which particles propagate, and resonances appear as temporary enhancements in the cross-section that decay into continuum states.
The concept of a continuum of states emerged with the development of quantum mechanics in the 1920s, particularly through the work of Max Born, Werner Heisenberg, and others on scattering theory. The mathematical treatment of resonances as poles in the scattering amplitude was developed by Eugene Wigner and others in the 1930s–1940s.
In quantum mechanics, bound states have quantized energies because the wavefunction must satisfy boundary conditions that confine it. In contrast, unbound states have no such constraints, so their energies form a continuum. When a system is coupled to a continuum, discrete states can acquire a finite lifetime and become resonances, with an energy width inversely related to their decay time. The continuum also plays a role in phenomena like the photoelectric effect, where an electron absorbs a photon and transitions from a bound state to a continuum state.
The continuum is central to nuclear and particle physics, where it describes the final states of reactions, and to condensed matter physics, where it underlies the electronic band structure of metals and semiconductors.
In quantum field theory, the vacuum itself is not empty but a continuum of virtual particle-antiparticle pairs, which gives rise to observable effects like the Casimir force.

