Statut | Confirmé |
Série | LPENS-ACE |
Domaines | astro-ph |
Date | Mercredi 4 Mars 2020 |
Heure | 14:00 |
Institut | LPENS |
Salle | L369 |
Nom de l'orateur | Tito D'agnolo |
Prenom de l'orateur | Raffaele |
Addresse email de l'orateur | |
Institution de l'orateur | IPhT/Sacaly |
Titre | A New Concept for the Detection of Axion Dark Matter |
Résumé | I will discuss an approach to search for axion dark matter with an especially desigend superconducting radio frequency cavity. Our approach exploits axion-induced transitions between nearly degenerate resonant modes of frequency close to a GHz. Compared to traditional detection strategies this allows for parametrically enhanced signal power for axions lighter than a GHz (~micro-eV). The projected sensitivity covers unexplored parameter space for QCD axion dark matter for axion masses between a GHz and 10 MHz. It is also sensitive to about eight orders of magnitude in axion-like dark matter coupling to photons for axion masses between GHz and Hz. |
Numéro de preprint arXiv | |
Commentaires | |
Fichiers attachés |
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