2012/09/21 by Paolo Pani, Vitor Cardoso, Vítor Cardoso +3 · 269 citations
Physics and Astronomy · #Accretion (finance) #Angular momentum #Astrophysical Phenomena and Observations #Astrophysics #Black Holes and Theoretical Physics #Black hole (networking) #Parameter space #Photon #Physics #Pulsars and Gravitational Waves Research #Quantum mechanics #Rotating black hole #Spacetime #Spin (aerodynamics) #Spin-flip #Supermassive black hole #astro-ph.HE #gr-qc #hep-ph #hep-th
paper · pdf · doi:10.1103/physrevlett.109.131102
published in Physical Review Letters 109(13), 131102 (American Physical Society) · 5 pages, 2 figures. References added. Matches published version
arxiv created 2012/09/21 · openalex publication_date 2012/09/27 · arxiv updated 2015/06/11 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Generic extensions of the standard model predict the existence of ultralight bosonic degrees of freedom. Several ongoing experiments are aimed at detecting these particles or constraining their mass range. Here we show that massive vector fields around rotating black holes can give rise to a strong superradiant instability, which extracts angular momentum from the hole. The observation of supermassive spinning black holes imposes limits on this mechanism. We show that current supermassive black-hole spin estimates provide the tightest upper limits on the mass of the photon (m(v) is < or approximately equal to 4×10(-20) eV according to our most conservative estimate), and that spin measurements for the largest known supermassive black holes could further lower this bound to m(v) < or approximately equal to 10(-22) eV. Our analysis relies on a novel framework to study perturbations of rotating Kerr black holes in the slow-rotation regime, that we developed up to second order in rotation, and that can be extended to other spacetime metrics and other theories.