Numerical relativity simulations of charged black hole mergers demonstrate identical gravitational dynamics across electromagnetic duality rotations, with electromagnetic radiation polarization rotated by the duality angle.
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gr-qc 2years
2026 2representative citing papers
Black holes with resonant scalar hair are dynamically unstable in 3+1 numerical relativity, decaying via fission or absorption into bald black holes.
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Spontaneous spherical symmetry breaking of black holes with resonant hair
Black holes with resonant scalar hair are dynamically unstable in 3+1 numerical relativity, decaying via fission or absorption into bald black holes.