学术文献库

We consider the Nielsen-Olesen vortex non-minimally coupled to Einstein gravity with cosmological constant $Λ$. A non-minimal coupling term $ξ\,R\,|ϕ|^2$ is natural to add to the vortex as it preserves gauge-invariance (here $R$ is the Ricci scalar and $ξ$ a dimensionless coupling constant). This term plays a dual role: it contributes to the potential of the scalar field and to the Einstein-Hilbert term for gravity. As a consequence, the vacuum expectation value (VEV) of the scalar field and the cosmological constant in the AdS$_3$ background depend on $ξ$. This leads to a novel feature: there is a critical coupling $ξ_c$ where the VEV is zero for $ξ\ge ξ_c$ but becomes non-zero when $ξ$ crosses below $ξ_c$ and the gauge symmetry is spontaneously broken. Moreover, we show that the VEV near the critical coupling has a power law behaviour proportional to $|ξ-ξ_c|^{1/2}$. Therefore $ξ_c$ can be viewed as the analog of the critical temperature $T_c$ in Ginzburg-Landau (GL) mean-field theory where a second-order phase transition occurs below $T_c$ and the order parameter has a similar power law behaviour $|T-T_c|^{1/2}$ near $T_c$. The critical coupling exists only in an AdS$_3$ background; it does not exist in asymptotically flat spacetime (topologically a cone) where the VEV remains at a fixed non-zero value independent of $ξ$. However, the deficit angle of the asymptotic conical spacetime depends on $ξ$ and is no longer determined solely by the mass; remarkably, a higher mass does not necessarily yield a higher deficit angle. The equations of motion are more complicated with the non-minimal coupling term present. However, via a convenient substitution one can reduce the number of equations and solve them numerically to obtain exact vortex solutions.