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MAP, MAC, and Vortex-rings Configurations in the Weinberg-Salam Model

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arxiv 1402.4222 v8 pith:R2R6XXCQ submitted 2014-02-18 hep-th

classification hep-th
keywords configurationsmagneticpossesschargefracmonopole-antimonopolevortex-ringsantimonopole
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abstract

We report on the presence of new axially symmetric monopoles, antimonopoles and vortex-rings solutions of the SU(2)$\times$U(1) Weinberg-Salam model of electromagnetic and weak interactions. When the $\phi$-winding number $n=1$, and 2, the configurations are monopole-antimonopole pair (MAP) and monopole-antimonopole chain (MAC) with poles of alternating sign magnetic charge arranged along the $z$-axis. Vortex-rings start to appear from the MAP and MAC configurations when the winding number $n=3$. The MAP configurations possess zero net magnetic charge whereas the MAC configurations possess net magnetic charge of $4\pi n/e$. In the MAP configurations, the monopole-antimonopole pair is bounded by the ${\cal Z}^0$ field flux string and there is an electromagnetic current loop encircling it. The monopole and antimonopole possess magnetic charges $\pm\frac{4\pi n}{e}\sin^2\theta_W$ respectively. In the MAC configurations there is no string connecting the monopole and the adjacent antimonopole and they possess magnetic charges $\pm\frac{4\pi n}{e}$ respectively. The MAC configurations possess infinite total energy and zero magnetic dipole moment whereas the MAP configurations which are actually sphalerons possess finite total energy and magnetic dipole moment. The configurations were investigated for varying values of Higgs self-coupling constant $0\leq \lambda\leq 40$ at Weinberg angle $\theta_W=\frac{\pi}{4}$.

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  1. Bifurcations in Bosonic Stars: chains and rings from spherical solutions

    gr-qc 2025-01 conditional novelty 6.0 of 10

    Zero-modes of spherical bosonic stars under axisymmetric perturbations explain the bifurcations into chain, ring, and gyroscope-like bosonic star families.

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