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X-WR-CALDESC:Eventi per INFN-LNF
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TZID:Europe/Rome
BEGIN:DAYLIGHT
TZOFFSETFROM:+0100
TZOFFSETTO:+0200
TZNAME:CEST
DTSTART:20260329T010000
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DTSTART:20261025T010000
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DTSTART;TZID=Europe/Rome:20260701T090000
DTEND;TZID=Europe/Rome:20260702T180000
DTSTAMP:20260508T183424
CREATED:20260508T144723Z
LAST-MODIFIED:20260508T144723Z
UID:40745-1782896400-1783015200@w3.lnf.infn.it
SUMMARY:FLASH Founding and General Meeting
DESCRIPTION:
URL:/event/flash-founding-and-general-meeting/
LOCATION:Aula Salvini
CATEGORIES:Conferenze & Workshops
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20260701T150000
DTEND;TZID=Europe/Rome:20260701T163000
DTSTAMP:20260508T183424
CREATED:20260417T084146Z
LAST-MODIFIED:20260417T084202Z
UID:40663-1782918000-1782923400@w3.lnf.infn.it
SUMMARY:Axion dark matter searches at IBS with cavity haloscopes
DESCRIPTION:Speaker: Sungwoo Youn (IBS\, Daejeon) \nAxions are a well-motivated dark matter candidate arising from the Peccei–Quinn solution to the strong CP problem. \nThe IBS Dark Matter Axion Group (DMAG) is pursuing a comprehensive experimental program to search for axion dark matter using cavity haloscopes\, which exploit the axion–photon coupling in strong magnetic fields. \nIn particular\, IBS-DMAG has achieved world-leading sensitivity in the GHz frequency range\, significantly advancing the exploration of QCD axion parameter space. \nIn this seminar\, I will discuss the key experimental techniques underlying these efforts\, including high-Q resonant cavities\, ultra-low-noise microwave detection\, and high-frequency search strategies. \nI will also present our recent results from the past few years and outline future directions to extend sensitivity and mass coverage.
URL:/event/axion-dark-matter-searches-at-ibs-with-cavity-haloscopes/
LOCATION:Aula Salvini
CATEGORIES:Seminari generali
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