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Absorption of Sub-MeV Fermionic Dark Matter by Electron Targets

1 Pith paper cite this work. Polarity classification is still indexing.

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abstract

We study a new class of signals where fermionic dark matter is absorbed by bound electron targets. Fermionic absorption signals in direct detection and neutrino experiments are sensitive to dark matter with sub-MeV mass, probing a region of parameter space in which dark matter is otherwise challenging to detect. We calculate the rate and energy deposition spectrum in xenon-based detectors, making projections for current and future experiments. We present two possible models that display fermionic absorption by electrons and study the detection prospects in light of other constraints.

fields

hep-ph 1

years

2025 1

verdicts

CONDITIONAL 1

representative citing papers

Supernova cooling from neutrino-devouring dark matter

hep-ph · 2025-07-29 · conditional · novelty 6.0

Supernova cooling excludes fermionic dark matter produced by neutrino scattering down to cross sections of about 10^-58 cm^2 for electrons and 10^-56 cm^2 for nucleons across the keV to 100 MeV mass range.

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  • Supernova cooling from neutrino-devouring dark matter hep-ph · 2025-07-29 · conditional · none · ref 6 · internal anchor

    Supernova cooling excludes fermionic dark matter produced by neutrino scattering down to cross sections of about 10^-58 cm^2 for electrons and 10^-56 cm^2 for nucleons across the keV to 100 MeV mass range.