Analytical formulation reveals absorption cross-section and stability properties in black holes with dark matter, highlighting implications for black hole thermodynamics.
Key Points
The analysis shows that absorption cross-section is influenced by parameters like black hole mass and charge, with specific wave interactions observed.
Key findings indicate that modified stability properties result from the generalized uncertainty principle affecting black holes in curved spacetimes.
Klein–Gordon equation was employed to assess energy emission rates and interactions, revealing insights into dark matter's role in black hole dynamics.
The exploration enhances understanding of nonlinear electrodynamics and its impact on black hole thermodynamics alongside exotic matter.