Classicalization via Path Integral

Understand

Recently, it was suggested that a large class of non-renormalizable theories may need no UV completion.

• By analogy with gravity where classical black holes are expected to be created in high-energy scatterings, it is conjectured that similar classical solutions, so-called classicalons, should occur.
• In this way the theory protects itself against non-unitarity, for instead of probing small distances at high energies one enters a classical regime.
• An effective theory of Goldstone bosons provides and example in which the size of classicalons grows with energy, and the high energy scattering is cut-off by small momenta, inversely proportional to the classicalon size.