Multipole decomposition of the gravitational field of a point mass at the black hole horizon
arXiv:2512.04976 · doi:10.1103/88br-6mzc
Abstract
The portion of the gravitational energy absorbed by the black hole due to the radial infall of a point mass is known to diverge at leading order in perturbation theory. This divergence is an artifact of the point-particle model, where the contribution of each multipole to the total absorbed energy is observed to be roughly constant. We show explicitly that this divergent energy arises from the infinite energy present in the singular static field arbitrarily close to the point mass, which also flows into the black hole when the particle trajectory crosses the horizon. We perform a multipole decomposition of the linearized gravitational field generated by the point mass near its world line at the black hole horizon. By applying the standard field-theoretical approach to the particle field, we compute the corresponding partial energy and find that it matches the constant multipole contribution.
9 pages, 2 figures
References in corpus (11)
- First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole
- First Sagittarius A* Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole in the Center of the Milky Way
- The Overlap of Numerical Relativity, Perturbation Theory and Post-Newtonian Theory in the Binary Black Hole Problem
- Gravitational waves emitted by a particle rotating around a Schwarzschild black hole: A semiclassical approach
- Scalar radiation from a source rotating around a regular black hole
- Black-hole head-on collisions in higher dimensions
- Divergences in gravitational-wave emission and absorption from extreme mass ratio binaries
- Synchrotron geodesic radiation in Schwarzschild-de Sitter spacetime
- Radiation emitted by a source orbiting a Schwarzschild--anti--de Sitter black hole
- Semiclassical bremsstrahlung from a charge radially falling into a Schwarzschild black hole
- Nonminimally coupled scalar field in Schwarzschild--de Sitter spacetime: Geodesic synchrotron radiation