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Comment on "calorimetric Dark Matter Detection with Galactic Center Gas Clouds"

Farrar, Glennys R; Lockman, Felix J; McClure-Griffiths, Naomi; Wadekar, Digvijay


In a recent Letter, Bhoonah et al. [1] attempted to derive limits on dark matter interactions with ordinary matter by demanding that dark matter (DM) heating of gas clouds not exceed the known astrophysical cooling rate based on the temperature, density, and metallicity of the observed clouds.

CollectionsANU Research Publications
Date published: 2020
Type: Journal article
Source: Physical Review Letters
DOI: 10.1103/PhysRevLett.124.029001
Access Rights: Open Access


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