# BPS Equations of Monopole and Dyon in $SU(2)$ Yang-Mills-Higgs Model,   Nakamula-Shiraishi Models, and Their Generalized Versions from The BPS   Lagrangian Method

**Authors:** Ardian Nata Atmaja, Ilham Prasetyo

arXiv: 1803.06122 · 2018-08-03

## TL;DR

This paper derives BPS equations for monopoles and dyons in various $SU(2)$ models using the BPS Lagrangian method, revealing new features like energy density shifts and constraints on scalar couplings.

## Contribution

It introduces a systematic derivation of BPS equations in generalized models, including a novel identification of effective fields and analysis of energy density modifications.

## Key findings

- BPS equations derived for monopoles and dyons in multiple models.
- Energy density shifts can invert monopole/dyon solutions.
- Constraints relate scalar couplings, e.g., G=w^{-1} for monopoles.

## Abstract

We apply the BPS Lagrangian method~\cite{Atmaja:2015umo} to derive BPS equations of monopole and dyon in the $SU(2)$ Yang-Mills-Higgs model, Nakamula-Shiraishi models, and their Generalized versions. We argue that by identifying the effective fields of scalar field, $f$, and of time-component gauge field, $j$, explicitly by $j=\beta f$ with $\beta$ is a real constant, the usual BPS equations for dyon can be obtained naturally. We validate this identification by showing that both Euler-Lagrange equations for $f$ and $j$ are identical in the BPS limit. The value of $\beta$ is bounded to $|\beta|<1$ due to reality condition on the resulting BPS equations. In the Born-Infeld type of actions, namely Nakamula-Shiraishi models and their Generalized versions, we find a new feature that adding the energy density by a constant $4b^2$, with $b$ is the Born-Infeld parameter, will turn monopole(dyon) to anti-monopole(anti-dyon) and vice versa. In all Generalized versions there are additional constraint equations that relate the scalar-dependent couplings of scalar and of gauge kinectic terms; or $G$ and $w$ respectively. For monopole the constraint equation is $G=w^{-1}$, while for dyon is $w(G-\beta^2 w)=1-\beta^2$ which further gives lower bound to $G$ as such $G\geq|2\beta\sqrt{1-\beta^2}|$. We also write down the complete square-forms of all effective Lagrangians.

## Full text

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## References

27 references — full list in the complete paper: https://tomesphere.com/paper/1803.06122/full.md

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Source: https://tomesphere.com/paper/1803.06122