Quasinormal modes of magnetized black hole
Abstract
We investigate a charged, massive scalar field around a static, spherically symmetric black hole immersed into an external asymptotically uniform magnetic field B . It is shown that for given multipole number ℓ there are 2 ℓ+1 numbers of modes due to the Zeeman effect appearing by an interaction of the external magnetic and charged scalar fields introducing an effective mass of the scalar field μ_{eff}=√{μ^{2}m q B } where m is the azimuthal number and q is the charge coupling constant. We calculate threshold value of effective mass in which quasinormal modes are arbitrarily long lived and beyond that value quasinormal modes vanish. In the case of m q B <0 quasinormal modes are longer lived with larger oscillation frequencies. Whenever, magnetic and massive scalar fields satisfies condition μ_{eff}^{2}<0 , an instability appears, i.e., if q B >0 or q B <0 there is an instability for the values of azimuthal number m >μ^{2}/q B or m <μ^{2}/q B , respectively.
 Publication:

Physical Review D
 Pub Date:
 October 2019
 DOI:
 10.1103/PhysRevD.100.084038
 arXiv:
 arXiv:1910.00939
 Bibcode:
 2019PhRvD.100h4038T
 Keywords:

 General Relativity and Quantum Cosmology
 EPrint:
 8 pages, 2 tables, 4 figures. Accepted for publication in Phys. Rev. D