Revisiting superradiant stability of Kerr-Newman black holes under a charged massive scalar

We revisit the superradiant stability of Kerr-Newman black holes under a charged massive scalar perturbation. We obtain a newly suitable potential which is not singular at the outer horizon when a radial equation is expressed the Schrodinger-type equation in terms of the tortoise coordinate. From the potential analysis, we find a condition for the superradiant stability of Kerr-Newman black holes.

Automated summary

The study revisits the superradiant stability of Kerr-Newman black holes under a charged massive scalar perturbation and obtains a newly suitable potential which is not singular at the outer horizon. From the potential analysis, a condition for the superradiant stability of Kerr-Newman black holes is found.