Dynamical evolution of fermion-boson stars
Authors: Susana Valdez-Alvarado, Carlos Palenzuela, Daniela Alic, L. Arturo Ureña-López
AI-generated Key Points
- Study focuses on compact objects like neutron stars and white dwarfs as probes for dark matter
- Researchers use perfect fluid coupled to a complex scalar field to model compact stars with dark matter
- Models known as fermion-boson stars
- Objective is to analyze stability and investigate spectrum of normal modes
- Dynamical evolution simulations used to examine equilibrium configurations and determine stability
- Fermion-boson stars have similar structures to isolated fermion or boson stars
- New oscillation modes discovered in fermionic part due to coupling with bosonic component through gravity
- Study contributes to understanding of compact objects with dark matter component and their stability and behavior
- Normal modes provide insights into presence and properties of dark matter within these systems
Abstract: Compact objects, like neutron stars and white dwarfs, may accrete dark matter, and then be sensitive probes of its presence. These compact stars with a dark matter component can be modeled by a perfect fluid minimally coupled to a complex scalar field (representing a bosonic dark matter component), resulting in objects known as fermion-boson stars. We have performed the dynamical evolution of these stars in order to analyze their stability, and to study their spectrum of normal modes, which may reveal the amount of dark matter in the system. Their stability analysis shows a structure similar to that of an isolated (fermion or boson) star, with equilibrium configurations either laying on the stable or on the unstable branch. The analysis of the spectrum of normal modes indicates the presence of new oscillation modes in the fermionic part of the star, which result from the coupling to the bosonic component through the gravity.
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