Dark Matter Jets of Rotating Black Holes
Ottavia Balducci, Stefan Hofmann, Maximilian Koegler
TL;DR
This paper introduces a new method for generating highly collimated Dark Matter jets from rotating black holes using the Penrose process, exploring their properties and potential local overdensities.
Contribution
It presents a novel approach to produce Dark Matter jets from Kerr black holes and analyzes their characteristics and implications.
Findings
Dark Matter jets are highly collimated and long-range.
Jet density depends on black hole mass and distance.
Potential to create Dark Matter overdensities near black holes.
Abstract
We present a novel approach which produces Dark Matter jets along the rotation axis of Kerr black holes utilizing the Penrose process. The properties of these jets are investigated, as well as their potential to create Dark Matter overdensities in the solar system and in the vicinity of the black hole. We discover a highly collimated and long-range Dark Matter jet with a density that is most sensitive to the mass and distance to the black hole.
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Taxonomy
TopicsRelativity and Gravitational Theory · Experimental and Theoretical Physics Studies · Cosmology and Gravitation Theories