Mass-deformed spherical sigma model ($V(\varphi )=\frac{r{m}^2}{4}{\sin }^2\varphi$)

A spherical sigma model in polar fields $\varphi ,\alpha$ has kinetic metric $r(d{\varphi }^2+{\sin }^2\varphi d{\alpha }^2)/2$ in the usual one-half kinetic convention. The displayed positive potential selects the two polar vacua. For $r>0$ it supports static and rotating charged kinks, and a topological theta term shifts their canonical internal charge without changing the bulk equations.

Locally this density is a total derivative, so it changes neither the bulk field equations nor the energy. Its contribution to the angular canonical momentum is a spatial boundary derivative. With ${ϵ}^{01}=+1$, it produces the theta-angle shift of a sigma-model kink charge.

With ${ϵ}^{01}=+1$, the Noether density for the angular shift gains $\theta {\partial }_x\cos \varphi /(4\pi )$. Its integral gives the displayed topological shift. Mechanical charge $Q_0$ determines the classical rotating-kink energy, while canonical symmetry charge $Q_{\theta }$ is conjugate to the periodic angle and is integral after quantization. Reversing the epsilon convention reverses the theta sign.

For $\alpha =\omega t+{\alpha }_0$ and $|\omega |<m$, the kink is $\varphi =2\arctan e^{\kappa (x-x_0)}$ with $\kappa =\sqrt{m^2-{\omega }^2}$. Its rest energy and mechanical internal charge are $M=r{m}^2/\kappa$ and $Q_0=r\omega /\kappa$. Eliminating the frequency gives the displayed mass relation. The orientation rotates while the energy profile remains stationary.

In units $\hslash =1$, periodic-angle quantization gives canonical charge $Q_{\theta }=\ell \in \mathbb{Z}$. The mechanical charge is $Q_0=\ell +\theta T/(2\pi )$ and the rotating-kink mass gives the displayed leading semiclassical spectrum. The $T=1$ and $T=-1$ families are related by reversing the kink. Theta periodicity relabels the integer; fluctuation corrections are not excluded by this leading calculation.

For $T=-[\cos \varphi {]}_{-\infty }^{+\infty }/2$, complete the static energy into squares $({\varphi }_x\mp m\sin \varphi {)}^2$ and ${\sin }^2\varphi {\alpha }_x^2$. The boundary term is $\pm rmT$. A $T=1$ saturating kink is $\varphi =2\arctan e^{m(x-x_0)}$, with constant $\alpha$ and mass $rm$. This is a model-specific Bogomolny bound.