Axionic dark matter signatures in various halo models
J. D. Vergados (KAIST University), Y. Semertzidis (KAIST, University)

TL;DR
This paper investigates how axion dark matter signals might vary over time in different galactic halo models, focusing on resonance width modulation and directional detection asymmetries.
Contribution
It introduces a detailed analysis of time-dependent signatures in axion searches across various halo models, including resonance modulation and directional asymmetries.
Findings
Resonance width shows characteristic time modulation patterns.
Directional experiments reveal potential asymmetries in axion signal detection.
Results vary significantly across different halo models.
Abstract
In the present work we study possible time signatures Axion Dark Matter searches employing resonant cavities for various halo models. We study in particular the time dependence of the resonance width (modulation) and possible asymmetries in directional experiments.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
