Statut | Confirmé |
Série | APC-COLLOQUIUM |
Domaines | astro-ph |
Date | Vendredi 29 Mars 2019 |
Heure | 11:00 |
Institut | APC |
Salle | Amphitheatre Pierre Gilles de Gennes |
Nom de l'orateur | Sigl |
Prenom de l'orateur | Guenter |
Addresse email de l'orateur | |
Institution de l'orateur | DESY |
Titre | Radio signatures from conversion of axionlike particles to photons |
Résumé | Axionlike particles (ALPs) can convert into photons in several different ways: in an external magnetic field (known as the Primakoff effect), by decay into two photons, or through parametric amplification of incoming radio photons in an oscillating ALP field within a narrow frequency range. For nonrelativistic ALPs all three effects can give rise to radio lines, in particular from astrophysical objects with strong magnetic fields or from regions with ALP overdensities, such as ALP stars. I will give an overview over estimated intensities and prospects for detectability of such radio lines. |
Numéro de preprint arXiv | |
Commentaires | |
Fichiers attachés |
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