Dynamical evolution of fermion-boson stars

Authors: Susana Valdez-Alvarado, Carlos Palenzuela, Daniela Alic, L. Arturo Ureña-López

Phys. Rev. D 87, 084040 (2013)
12 pages, 14 figures

Results of the summarizing process for the arXiv paper: 1210.2299v1

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The study focuses on compact objects such as neutron stars and white dwarfs that can accrete dark matter and serve as sensitive probes for its presence. To model these compact stars with a dark matter component, researchers use a perfect fluid minimally coupled to a complex scalar field representing bosonic dark matter. These models are known as fermion-boson stars. The main objective is to analyze the stability of these stars and investigate their spectrum of normal modes, providing insights into the amount of dark matter present. Through dynamical evolution simulations, the team examines various equilibrium configurations and determines their stability. The analysis reveals that fermion-boson stars have similar structures to isolated fermion or boson stars. Additionally, new oscillation modes in the fermionic part are discovered due to its coupling with the bosonic component through gravity. This study contributes to our understanding of compact objects with a dark matter component and sheds light on their stability and behavior. By studying their normal modes, scientists can gain further knowledge about the presence and properties of dark matter within these systems.
AI-generated keywords: Compact objects dark matter fermion-boson stars stability analysis normal modes

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
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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.

Submitted to arXiv on 08 Oct. 2012

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