Interactions of Non-Abelian Global Strings
arXiv:0708.4092 · doi:10.1016/j.physletb.2008.11.049
Abstract
Non-Abelian global strings are expected to form during the chiral phase transition. They have orientational zero modes in the internal space, associated with the vector-like symmetry SU(N)_{L+R} broken in the presence of strings. The interaction among two parallel non-Abelian global strings is derived for general relative orientational zero modes, giving a non-Abelian generalization of the Magnus force. It is shown that when the orientations of the strings are the same, the repulsive force reaches the maximum, whereas when the relative orientation becomes the maximum, no force exists between the strings. For the Abelian case we find a finite volume correction to the known result. The marginal instability of the previously known Abelian eta' strings is discussed.
12 pages, 2 figures, a brief discussion on stability added, published version
References in corpus (9)
- All Exact Solutions of a 1/4 Bogomol'nyi-Prasad-Sommerfield Equation
- Construction of Non-Abelian Walls and Their Complete Moduli Space
- Non-Abelian Walls in Supersymmetric Gauge Theories
- Universal Reconnection of Non-Abelian Cosmic Strings
- On the moduli space of semilocal strings and lumps
- Cosmic strings reborn?
- Statistical Mechanics of Vortices from D-branes and T-duality
- Non-Abelian Global Strings at Chiral Phase Transition
- and mesons in the Dyson-Schwinger approach at finite temperature