An infrared divergence is a divergence caused by contributions from arbitrarily low energies or long wavelengths.
An observable unchanged by adding a particle with vanishing energy or replacing one massless particle by exactly collinear particles with the same total momentum. This property permits cancellation of real and virtual infrared divergences and collinear divergences in its perturbative cross-section. Fully inclusive electron-positron hadronic rates and suitably defined jet observables are examples.
A singularity of a massless scattering or radiation integral when momenta of two particles become parallel. In Quantum chromodynamics, unresolved quark-gluon splittings cause such divergences. A mass regulator or dimensional regularization exposes them; they cancel between suitable inclusive real and virtual contributions or are absorbed into factorized distributions where appropriate.
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Infrared divergence refers to a type of divergence that occurs in quantum field theory (QFT) and certain fields of theoretical physics when dealing with low-energy (or long-wavelength) phenomena. Specifically, it manifests when evaluating Feynman integrals or loop diagrams that include virtual particles with very low momenta (approaching zero). In such scenarios, the contributions from these low-energy states can lead to integrals that diverge, meaning they yield infinite values.