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DTSTART;TZID=Europe/Madrid:20260602T150000
DTEND;TZID=Europe/Madrid:20260602T160000
DTSTAMP:20260718T163245
CREATED:20260527T141356Z
LAST-MODIFIED:20260603T093853Z
UID:25107-1780412400-1780416000@www.ift.uam-csic.es
SUMMARY:A diffuse flux of MeV ALPs
DESCRIPTION:Title: ‘A diffuse flux of MeV ALPs’ \nSpeaker: Marina Cermeño \nVenue&Time: Red Room / 15:00 \nAbstract: MeV scale axion-like particles can be produced with semi-relativistic velocities in Galactic supernovae\, leading to a diffuse flux that can be detectable in neutrino water-Cherenkov detectors (Super + HyperK). In this talk\, I will explain the details of the calculation that we recently did in 2602.17597 also with some content from our previous works 2412.09595 \, 2412.19890) \n 
URL:https://www.ift.uam-csic.es/event/a-diffuse-flux-of-mev-alps/
LOCATION:IFT Seminar Room/Red Room\, Instituto de Física Teórica (IFT) -C. Nicolás Cabrera\, 13-15\, Fuencarral-El Pardo\, Madrid\, 28049\,\, Spain
CATEGORIES:Scientific activities,Seminars
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