arXiv · 2312.15755
Rotating multistate Proca stars
Abstract
In this paper, we construct the rotating multistate Proca stars (RMPSs) composed of two coexisting Proca fields including the ground state and first excited state. We consider the solution families of RMPSs in synchronized frequency and non-synchronized frequency scenarios, respectively. We discuss the characteristics of the matter fields changing with the synchronized frequency or non-synchronized frequency, and then we explore the relationship between the ADM mass $M$ and the frequency. We also analyze the characteristics of ADM mass $M$ as a function of the angular momentum $J$ simultaneously. Furthermore, we calculate the binding energy of RMPSs and analyze the stability of the solutions. Finally, we discuss the ergosphere of RMPSs.
Explore related subjects
Keep this discovery
Rong Zhang, Long-Xing Huang, Yong-Qiang Wang. 2023-12-25. Rotating multistate Proca stars. https://arxiv.org/abs/2312.15755
Cite the original work for its findings. Save a collection to share your selection of sources.