Black holes and the absorption rate of cosmological scalar fields
L. Arturo Urena-Lopez, Lizbeth M. Fernandez

TL;DR
This paper investigates how a massless scalar field is absorbed by a static black hole, revealing that absorption depends on wave characteristics and establishing a minimum absorption fraction of about 50%.
Contribution
It introduces a normalized absorption rate based on the Klein-Gordon equation and analyzes its dependence on wave properties, providing new insights into scalar field-black hole interactions.
Findings
Absorption rate depends on wavelength and wave packet width.
Absorption is insensitive to scalar field strength.
Minimum absorption fraction is approximately 50%.
Abstract
We study the absorption of a massless scalar field by a static black hole. Using the continuity equation that arises from the Klein-Gordon equation, it is possible to define a normalized absorption rate for the scalar field as it falls into the black hole. It is found that the absorption mainly depends upon the characteristics wavelengths involved in the physical system: the mean wavenumber and the width of the wave packet, but that it is insensitive to the scalar field's strength. By taking a limiting procedure, we determine the minimum absorption fraction of the scalar field's mass by the black hole, which is around 50%.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
