Slowly damped quasinormal modes of the massive Dirac field in d-dimensional Tangherlini spacetime

Understand

We consider quasinormal modes of the massive Dirac field in the background of a Schwarzschild- Tangherlini black hole.

• Different dimensions of the spacetime are considered, from d = 4 to d = 9.
• The quasinormal modes are calculated using two independent methods: WKB and continued fraction.
• We obtain the spectrum of quasinormal modes for different values of the overtone number and angular quantum number.