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New CMB spectral distortion constraints on decaying dark matter with full evolution of electromagnetic cascades before recombination

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arxiv 1903.04503 v2 pith:HZINSMHM submitted 2019-03-11 astro-ph.CO astro-ph.HEhep-ph

New CMB spectral distortion constraints on decaying dark matter with full evolution of electromagnetic cascades before recombination

classification astro-ph.CO astro-ph.HEhep-ph
keywords constraintsenergyspectraldistortiondistortionsbeforecascadesdark
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Current constraints on energy injection in the form of energetic particles before the epoch of recombination using CMB spectral distortions assume that all energy goes into $y$ and $\mu$-type distortions. We revisit these constraints with exact calculations of the spectral distortions by evolving the electromagnetic cascades. The actual spectral distortion differs in shape and amplitude from the $y$-type distortion and depends on the energy and nature of injected particles. The constraints on the energy injection processes such as dark matter decay can be relaxed by as much as a factor of 5.

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Cited by 1 Pith paper

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

  1. The Glow of Axion Quark Nugget Dark Matter: (IV) CMB Spectral and Anisotropy Signatures

    astro-ph.CO 2025-12 conditional novelty 5.0

    Axion quark nugget dark matter would create a μ-type CMB spectral distortion near 6×10⁻⁸ with y near 2×10⁻⁹, detectable by proposed missions, while leaving CMB anisotropies essentially unchanged.