Intermediate Mass Black Holes and Nearby Dark Matter Point Sources: A Critical Reassessment
Torsten Bringmann, Julien Lavalle, Pierre Salati

TL;DR
This paper critically reassesses the detectability of intermediate mass black holes with dark matter mini-spikes, showing current gamma-ray data already impose strong limits, making future detection prospects unlikely for various cosmic messengers.
Contribution
It provides a detailed statistical analysis demonstrating that existing gamma-ray and cosmic ray data severely constrain the presence of dark matter mini-spikes around intermediate mass black holes.
Findings
EGRET data impose stringent limits on dark matter mini-spikes.
Detection prospects with Fermi/GLAST and Cherenkov telescopes are unlikely.
Cosmic ray and gamma-ray data exclude the possibility that PAMELA/ATIC excesses are due to nearby dark matter sources.
Abstract
The proposal of a galactic population of intermediate mass black holes (IMBHs), forming dark matter (DM) ``mini-spikes'' around them, has received considerable attention in recent years. In fact, leading in some scenarios to large annihilation fluxes in gamma rays, neutrinos and charged cosmic rays, these objects are sometimes quoted as one of the most promising targets for indirect DM searches. In this letter, we apply a detailed statistical analysis to point out that the existing EGRET data already place very stringent limits on those scenarios, making it rather unlikely that any of these objects will be observed with, e.g., the Fermi/GLAST satellite or upcoming Air Cherenkov telescopes. We also demonstrate that prospects for observing signals in neutrinos or charged cosmic rays seem even worse. Finally, we address the question of whether the excess in the cosmic ray positron/electron…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Astrophysics and Cosmic Phenomena · Particle physics theoretical and experimental studies
