Resonant Pseudo-Dirac Dark Matter as a Sub-GeV Thermal Target
Nirmalya Brahma, Saniya Heeba, Katelin Schutz

TL;DR
This paper explores a resonant pseudo-Dirac dark matter model with sub-GeV mass, showing that the excited state persists without violating CMB bounds and could lead to new detection signatures.
Contribution
It demonstrates that in the resonant regime, the excited state remains thermally populated without conflicting with CMB constraints, expanding the potential detection avenues for pseudo-Dirac dark matter.
Findings
Resonance reduces couplings needed for relic abundance
Excited state not thermally depopulated in this regime
Excited state can produce detectable signals today
Abstract
Dark matter (DM) could be a pseudo-Dirac thermal relic with a small mass splitting that is coupled off-diagonally to a kinetically mixed dark photon. This model, particularly in the sub-GeV mass range, is a key benchmark for accelerator searches and direct detection experiments. Typically, the presence of even a tiny fraction of pseudo-Dirac DM in the excited state around the time of recombination would be excluded by DM annihilation bounds from the cosmic microwave background (CMB); thus, viable thermal histories must typically feature an exponential suppression of the excited state. We revisit assumptions about the thermal history in the resonant regime, where the dark photon mass is slightly more than twice the DM mass (to within ), leading to an -channel resonance in the annihilation cross section. This resonance substantially reduces the couplings required for…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Advanced Thermodynamics and Statistical Mechanics · Quantum Mechanics and Applications
