Abstract
We study the classical color radiation from very high energy collisions that produce colored particles. In the extreme high energy limit, the classical color fields are confined to a light-shell expanding at $c$ and are associated with a non-linear $\sigma$-model on the 2D light-shell with specific symmetry breaking terms. We argue that the quantum version of this picture exhibits asymptotic freedom and may be a useful starting point for an effective light-shell theory of the structure between the jets at a very high energy collider.
Highlights
We argue that the quantum version of this picture exhibits asymptotic freedom and may be a useful starting point for an effective light-shell theory of the structure between the jets at a very high energy collider
Those of us who have had the pleasure of learning or teaching from Ed Purcell’s classic book on electricity and magnetism [1] cannot forget the evocative figure in chapter 5 illustrating how a pulse of electromagnetic radiation emerges from a kink in the field of a charge that starts and stops
We suggest that a similar picture may yield a useful starting point for a description of very high energy collisions between hadrons
Summary
Those of us who have had the pleasure of learning or teaching from Ed Purcell’s classic book on electricity and magnetism [1] cannot forget the evocative figure in chapter 5 illustrating how a pulse of electromagnetic radiation emerges from a kink in the field of a charge that starts and stops. In the extreme high energy limit, the classical color fields are confined to a light-shell expanding at c and are associated with a non-linear σ-model on the 2D light-shell with specific symmetry breaking terms.
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