Q-Balls in the presence of attractive force

TL;DR

This paper investigates how an attractive cubic interaction affects the stability and maximum charge of Q-balls, revealing a fundamental charge limit and potential implications for primordial black hole formation.

Contribution

It introduces the analysis of attractive forces in Q-balls, showing the existence of a maximum charge and its impact on stability, which was previously overlooked in standard models.

Findings

Existence of a maximum charge for Q-balls with attractive interactions

Analytical solutions align with numerical simulations

Potential role in primordial black hole formation

Abstract

Q-balls are non-topological solitons in field theories whose stability is typically guaranteed by the existence of a global conserved charge. A classic realization is the Friedberg-Lee-Sirlin (FLS) Q-ball in a two-scalar system where a real scalar $\chi$ triggers symmetry breaking and confines a complex scalar $\Phi$ with a global $U(1)$ symmetry. A quartic interaction $\kappa \chi^2|\Phi|^2$ with $\kappa>0$ is usually considered to produce a nontrivial Q-ball configuration, and this repulsive force contributes to its stability. On the other hand, the attractive cubic interaction $\Lambda \chi |\Phi|^2$ is generally allowed in a renormalizable theory and could induce an instability. In this paper, we study the behavior of the Q-ball under the influence of this attractive force which has been overlooked. We find approximate Q-ball solutions in the limit of weak and moderate force couplings using the thin-wall and thick-wall approximations respectively. Our analytical results are consistent with numerical simulations and predict the parameter dependencies of the maximum charge. A crucial difference with the ordinary FLS Q-ball is the existence of the maximum charge beyond which the Q-ball solution is classically unstable. Such a limitation of the charge fundamentally affects Q-ball formation in the early Universe and could plausibly lead to the formation of primordial black holes.