Maxwell perturbations in a cavity with Robin boundary conditions: two branches of modes with spectrum bifurcation on Schwarzschild black holes
Yunhe Lei, Mengjie Wang, Jiliang Jing

TL;DR
This paper investigates Maxwell quasinormal modes in a cavity around Schwarzschild black holes, revealing two distinct mode sets and spectrum bifurcation effects similar to those in AdS black holes, through analytical and numerical methods.
Contribution
It introduces two boundary condition sets based on the vanishing energy flux principle and demonstrates spectrum bifurcation in Maxwell fields in a cavity, paralleling AdS black hole phenomena.
Findings
Two sets of Maxwell modes identified under different boundary conditions.
Analytical expressions for the imaginary parts of the modes derived.
Spectrum bifurcation occurs when the mirror is near the black hole horizon.
Abstract
We perform a systematic study of the Maxwell quasinormal spectrum in a mirror-like cavity following the generic Robin type vanishing energy flux principle, by starting with the Schwarzschild black holes in this paper. It is shown that, for black holes in a cavity, the vanishing energy flux principle leads to \textit{two} different sets of boundary conditions. By solving the Maxwell equations with these two boundary conditions both analytically and numerically, we observe \textit{two} distinct sets of modes. This indicates that the vanishing energy flux principle may be applied not only to asymptotically anti-de Sitter (AdS) black holes but also to black holes in a cavity. In the analytic calculations, the imaginary part of the Maxwell quasinormal modes are derived analytically for both boundary conditions, which match well with the numeric results. While in the numeric calculations, we…
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