Non-radial oscillations in dark matter admixed neutron stars using a two fluid formalism

Key Points

• Non-radial oscillations were observed in neutron stars containing dark matter, indicating complex behavior in these celestial objects.
• The study showed that these oscillations can be described mathematically, providing important metrics for understanding their dynamics.
• Observational analysis using a two fluid formalism allowed for a more detailed examination of the interaction between dark matter and neutron matter.
• These findings may enhance our understanding of neutron star properties, emphasizing the need for further theoretical exploration of dark matter effects.