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

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

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American Physical Society

Abstract

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.

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Physical Review Letters

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Open Access

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Creative Commons Attribution licence

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