The study presents a detailed analytical framework to examine the stochastic wave vector dark matter signal by evaluating marginalized likelihoods. This builds a foundation for future research.
Aligning the lab's coordinate system with the local dark matter velocity provides a clearer view of the detector signals, impacting our understanding of dark matter interactions.
The findings suggest the potential of accelerometer studies in probing dark matter components. By recasting limits, we highlight the significance of B − L dark matter in current research.
Future directions indicated include refining statistical analysis techniques for dark matter detection, emphasizing the necessity for establishing clearer connections between theoretical models and observational data.
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