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X-WR-CALDESC:Eventi per INFN-LNF
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TZID:Europe/Rome
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TZOFFSETFROM:+0100
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TZNAME:CEST
DTSTART:20240331T010000
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DTSTART:20241027T010000
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DTSTART;TZID=Europe/Rome:20240916T090000
DTEND;TZID=Europe/Rome:20240920T200000
DTSTAMP:20260510T083247
CREATED:20240730T135557Z
LAST-MODIFIED:20240730T135557Z
UID:38389-1726477200-1726862400@w3.lnf.infn.it
SUMMARY:GAMBIT XVI @ LNF
DESCRIPTION:This hybrid meeting brings together the GAMBIT Community to discuss and continue work on global fits for Beyond-the-Standard-Model theories. We summarise the status of recently completed and ongoing projects of the various GAMBIT working groups\, improve the GAMBIT software code in dedicated coding sessions\, review the GAMBIT Community policies\, and discuss interesting future directions in light of current developments in the field. We encourage interested researchers at LNF and beyond to join us to learn more about GAMBIT and how to connect it to their own research.\n\nOrganizing Committee\n\nSebastian Hoof (Padova Univ. & INFN Padova\, IT)\nAnders Kvellestad (Oslo Univ.\, NO)\nFederico Mescia (INFN-LNF\, IT)\nEnrico Nardi (INFN-LNF\, IT & NICPB Tallinn\, EE)\nMartin White (Adelaide Univ.\, AU)
URL:/event/gambit-xvi-lnf/
LOCATION:Aula Salvini
CATEGORIES:Conferenze & Workshops
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BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20240918T143000
DTEND;TZID=Europe/Rome:20240918T170000
DTSTAMP:20260510T083247
CREATED:20240729T095641Z
LAST-MODIFIED:20240729T095641Z
UID:38299-1726669800-1726678800@w3.lnf.infn.it
SUMMARY:Low-energy avenues for light dark matter searches
DESCRIPTION:Speaker: Angelo Esposito (Istituto Nazionale di Fisica Nucleare) \nFollowing negative results in standard WIMP searches\, increasing attention has been devoted to models of dark matter with masses in the sub-MeV range. For such masses\, the typical momentum and energy transferred by the dark matter to our detectors is such that the most likely signatures of its passage is given by the emission of collective excitations. \nI will describe two possible ways to look for dark matter this way: superfluid He-4 for spin-independent interactions and anti-ferromagnets for spin-dependent ones. In particular\, I will argue that a powerful tool to describe the interaction between dark matter and collective excitations is that of effective field theories for spontaneously broken spacetime symmetries. In this framework\, the collective modes are nothing but Goldstone bosons\, and their interactions with dark matter (and among themselves) are completely dictated by symmetry\, together with a handful of effective coefficients. \nJoin Zoom Meeting\nhttps://infn-it.zoom.us/j/96975604651?pwd=u0LyX2a0ubWJRPjhjcUOLO7raF1ZQV.1 \nMeeting ID: 969 7560 4651\nPasscode: 116503
URL:/event/low-energy-avenues-for-light-dark-matter-searches/
LOCATION:Aula Salvini
CATEGORIES:Seminari generali
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