In today's world, Ultraviolet completion is a topic that has captured the attention of millions of people around the world. From its impact on society to its influence on popular culture, Ultraviolet completion has generated unprecedented debate. As we continue to explore this ever-evolving phenomenon, it is important to understand its ramifications and how it is shaping the world around us. In this article, we will delve into the different aspects of Ultraviolet completion, from its history to its impact today, in order to shed light on this topic and encourage informed discussion.
In theoretical physics, ultraviolet completion, or UV completion, of a quantum field theory is the passing from a lower energy quantum field theory to a more general quantum field theory above a threshold value known as the cutoff. In particular, the more general high energy theory must be well-defined at arbitrarily high energies.[1]
The word "ultraviolet" in this so-called "ultraviolet regime" is only figurative, and refers to energies much higher than ultraviolet light per se. Rather, by analogy to the relationship between ultraviolet and visible light, it refers to energies higher than (and wavelengths shorter than) those "visible" to laboratory experiment.
The ultraviolet theory must be renormalizable;[1][2][3] it can have no Landau poles; and most typically, it enjoys asymptotic freedom in the case that it is a quantum field theory (or at least has a nontrivial fixed point). However, it may also be a background of string theory whose ultraviolet behavior is at least as good as that of renormalizable quantum field theories.[1][3] Besides these two known examples (QFT and string theory), it could be a completely different theory than string theory that behaves well at very high energies.
There is an analogous phrase "infrared completion", which applies to length scales longer than those "visible" to normal experiment, particularly cosmology distances.