Abstract

We consider the quantum multisoliton scattering problem. For BPS theories one truncates the full field theory to the moduli space, a finite dimensional manifold of energy minimising field configurations, and studies the quantum mechanical problem on this. Non-BPS theories — the generic case — have no such obvious truncation. We define a quantum soliton scattering manifold as a configuration space which satisfies asymptotic completeness and respects the underlying classical dynamics of slow moving solitons. Having done this, we present a new method to construct such manifolds. In the BPS case the dimension of the n-soliton moduli space ℳn is n multiplied by the dimension of ℳ1. We show that this scaling is not necessarily valid for scattering manifolds in non-BPS theories, and argue that it is false for the Skyrme and baby-Skyrme models. In these models, we show that a relative phase difference can generate a relative size difference during a soliton collision. Asymptotically, these are zero and non-zero modes respectively and this new mechanism softens the dichotomy between such modes. Using this discovery, we then show that all previous truncations of the 2-Skyrmion configuration space are unsuitable for the quantum scattering problem as they have the wrong dimension. This gives credence to recent numerical work which suggests that the low-energy configuration space is 14- dimensional (rather than 12-dimensional, as previously thought). We suggest some ways to construct a suitable manifold for the 2-Skyrmion problem, and discuss applications of our new definition and construction for general soliton theories.

Highlights

  • When the solitons are closer together, the structure of Mn+m deforms significantly, but the asymptotic picture can be helpful

  • We have proposed a definition and a construction of a quantum soliton scattering manifold (QSSM); the minimal manifold required to describe quantum multisoliton scattering

  • If the late-time configurations contain new configurations, a mistake has been made and these should have been included from the start. We applied this idea to two- and threedimensional Skyrmions, showing that the late-time configurations include a relative size orientation, not seen in Ma1s,1y

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Summary

The sine-Gordon model

To start exploring the new definition and construction let us consider a well understood system: two sine-Gordon kinks, where the questions we’ll ask have well known answers. The moduli space of a single kink is M1 ∼= R and so the asymptotic submanifold of two kinks is given by. We wish to construct a configuration space using the scattering paths whose initial configurations are in the reduced asymptotic submanifold. We must investigate the scattering paths and ensure that the set of outgoing configurations contains Ma1s,1y. In this case, we must scatter two well separated kinks and check if two well separated kinks emerge after their collision. This says that at early time, the two kinks are separated by 2X0 and are moving towards one another, each with velocity v We can solve these equations numerically and a solution is.

The baby Skyrme model
The Skyrme model
Conclusions and further work
A Unattractive channel scattering
Full Text
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