Frozen solitonic Hayward-boson stars in Anti-de Sitter Spacetime
Shu-Cong Liu, Yong-Qiang Wang, Zhen-Hua Zhao
TL;DR
We construct and analyze solitonic Hayward boson stars (SHBSs) in Anti-de Sitter spacetime by coupling Einstein gravity to a nonlinear electromagnetic field and a complex scalar with a solitonic potential. A critical magnetic charge $q_c$ governs frozen behavior as $ω\to0$, with $q_c$ depending on the cosmological constant $Λ$ and the self-interaction $η$, and frozen interiors occurring for $q\ge q_c$ only within a finite parameter window; decreasing $Λ$ can destroy the frozen state. For $q<q_c$ the solutions exhibit spiraling $M$–$ω$ relations and a rich light-ring structure, while for $q\ge q_c$ extreme ($ω\to0$) solutions appear, accompanied by an additional pair of light rings on the second branch; increasing $η$ can move high-frequency solutions toward pure Hayward geometry, or suppress freezing at low frequencies. Overall, the work maps out the interplay of magnetic charge, AdS curvature, and self-interaction in shaping SHBSs, their horizon-like features, and photon orbits, with potential implications for holographic duals and extensions to higher dimensions.
Abstract
We construct solitonic Hayward-boson stars (SHBSs) in Anti-de Sitter (AdS) spacetime, which consists of the Einstein-Hayward model and a complex scalar field with a soliton potential. Our results reveal a critical magnetic charge $q_c$. For $q\geq q_c$ in the limit of $ω\rightarrow 0$, the matter field is primarily distributed within the critical radius $r_c$, beyond which it decays rapidly, while the metric components $-g_{tt}$ and $1/g_{rr}$ become very small at $r_c$. These solutions are termed ``frozen solitonic Hayward-boson stars" (FSHBSs). Continuously decreasing $Λ$ disrupts the frozen state. However, we did not find a frozen solution when $q<q_c$. The value of $q_c$ depends both on the cosmological constant $Λ$ and the self-interaction coupling $η$. We also found that for high frequency solutions, increasing $η$ can yield a pure Hayward solution. However, for low frequency solutions, increasing $η$ reduces both $1/g_{rr}$ and $-g_{tt}$. Furthermore, we analyzed the effective potential of SHBSs and identified an extra pair of light rings in the second solution branch.
