Situation in which a Feynman integral diverges due to high-energy (short-distance) contributions, requiring regularization/renormalization or some ultraviolet completion
fenomeno en kvantuma kampoteorio, je kiu Feynman-integral diverĝas pro kontribuo de grandenergiaj partikloj, solvenda per reguligo/renormumo aŭ alia ultraviola kompletigo (eo)
situation in which a Feynman integral diverges due to high-energy (short-distance) contributions, requiring regularization/renormalization or some ultraviolet completion (en)