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Anomalous Ionization in the Central Molecular Zone by sub-GeV Dark Matter

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arxiv 2409.07515 v3 pith:Q5IZ26KB submitted 2024-09-11 hep-ph astro-ph.HE

classification hep-phastro-ph.HE
keywords darkmatteranomalouscentralgalacticgammaionizationmolecular
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abstract

We demonstrate that the anomalous ionization rate observed in the Central Molecular Zone can be attributed to MeV dark matter annihilations into $e^+e^-$ pairs for galactic dark matter profiles with slopes $\gamma>1$. The low annihilation cross-sections required avoid cosmological constraints and imply no detectable inverse Compton, bremsstrahlung or synchrotron emissions in radio, X and gamma rays. The possible connection to the source of the unexplained 511 keV line emission in the Galactic Center suggests that both observations could be correlated and have a common origin.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Molecular clouds constraints on sub-GeV DM and asteroid-mass PBHs

    hep-ph 2026-07 conditional novelty 5.0 of 10

    Molecular-cloud ionization yields competitive constraints on sub-GeV dark matter annihilation/decay and on asteroid-mass primordial black holes, particularly for PBHs above 10^16 g.

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