This paper presents a framework for studying boson star chains in alternative gravity theories, analyzing their stability and gravitational wave signatures, with implications for dark matter and gravitational wave observatories.
Key findings
Boson star chains are multi-component scalar field condensates with potential implications for dark matter physics and gravitational wave astronomy.
The paper develops a methodology for constructing stationary chain solutions and analyzes their stability in modified gravity theories.
Identifies phenomena unique to alternative gravity, such as spontaneous scalarization-induced chain formation and modified orbital dynamics.
Establishes boson star chains as probes of strong-field gravity, with potential detection by upcoming gravitational wave observatories.
Limitations & open questions
The study primarily focuses on theoretical analysis and numerical simulations, requiring further observational validation.
The implications for gravitational wave observatories are based on current predictions and may evolve with technological advancements.