2020/09/30 by Aydın Tavlayan, Aydin Tavlayan, Bayram Tekin
Mathematics · Physics and Astronomy · #Angular momentum #Astrophysical Phenomena and Observations #Black Holes and Theoretical Physics #Black hole (networking) #Circular orbit #Classical mechanics #General relativity #Geodesic #Geodesics in general relativity #Geometry #Mathematical analysis #Mathematics #Null (SQL) #Orbit (dynamics) #Photon #Photon sphere #Physics #Polar #Pulsars and Gravitational Waves Research #Quantum mechanics #RADIUS #Rotating black hole #Rotation (mathematics) #astro-ph.HE #gr-qc #hep-th
paper · pdf · doi:10.1103/physrevd.102.104036
published as Phys. Rev. D 102, 104036 (2020) · 6 pages, 5 figures and 2 tables; v2 matches the published version
arxiv created 2020/11/10 · openalex publication_date 2020/11/13 · arxiv updated 2020/11/18 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Exact formulas relating the radii of the spherical photon orbits to the black hole's rotation parameter and the effective inclination angle of the orbit have been known only for equatorial and polar orbits up to now. Here we provide exact formulas for nonequatorial orbits that lie between these extreme limits. For a given rotation parameter of the black hole, there is a critical inclination angle below which there are four null photon orbits two of which are in the exterior region. At the critical angle, the radii of these orbits are explicitly found. We also provide approximate but very accurate formulas for any orbit. To arrive at these analytical solutions, we carefully study the sextic polynomial in the radius that arises for null spherical geodesics.