Quasinormal modes of a Schwarzschild black hole surrounded by free static spherically symmetric quintessence: Electromagnetic perturbations

In this paper, we evaluated the quasinormal modes of electromagnetic perturbation in a Schwarzschild black hole surrounded by the static spherically symmetric quintessence by using the third-order WKB approximation when the quintessential state parameter $ w_{q}$ in the range of $-1/3

Keywords:

• Perturbation (astronomy)
• Physics
• Black hole
• Schwarzschild metric
• Spacetime
• Quintessence
• WKB approximation
• Boundary value problem
• maxwell field
• Mathematical physics

• Correction
• Source
• Cite
• Save
• Machine Reading By IdeaReader