BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//INFN-LNF - ECPv5.14.2.1//NONSGML v1.0//EN
CALSCALE:GREGORIAN
METHOD:PUBLISH
X-WR-CALNAME:INFN-LNF
X-ORIGINAL-URL:https://w3.lnf.infn.it
X-WR-CALDESC:Eventi per INFN-LNF
BEGIN:VTIMEZONE
TZID:Europe/Rome
BEGIN:DAYLIGHT
TZOFFSETFROM:+0100
TZOFFSETTO:+0200
TZNAME:CEST
DTSTART:20260329T010000
END:DAYLIGHT
BEGIN:STANDARD
TZOFFSETFROM:+0200
TZOFFSETTO:+0100
TZNAME:CET
DTSTART:20261025T010000
END:STANDARD
END:VTIMEZONE
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20260615T110000
DTEND;TZID=Europe/Rome:20260618T130000
DTSTAMP:20260508T235039
CREATED:20260322T192154Z
LAST-MODIFIED:20260322T192423Z
UID:40547-1781521200-1781787600@w3.lnf.infn.it
SUMMARY:Convegno Nazionale SIRR 2026
DESCRIPTION:Il Convegno Nazionale SIRR\, che ha una cadenza biennale\, rappresenta il più importante momento di aggregazione sia per gli iscritti alla Società che per potenziali futuri soci interessati a condividere il loro lavoro e a discuterne le prospettive nei vari ambiti di ricerca coperti dalla SIRR. Il Convegno Nazionale SIRR 2026 è organizzato in collaborazione con l’Istituto Nazionale di Fisica Nucleare (INFN)\, grazie al recente accordo INFN–SIRR che formalizza e rafforza la sinergia tra le due comunità scientifiche. \nSito web: https://web.infn.it/convegnonazionalesirr2026/
URL:/event/convegno-nazionale-sirr-2026/
LOCATION:INFN – Laboratori Nazionali di Frascati\, Via Enrico Fermi\, 54\, Frascati\, Roma\, 00044\, Italia
CATEGORIES:Conferenze & Workshops
END:VEVENT
BEGIN:VEVENT
DTSTART;TZID=Europe/Rome:20260615T143000
DTEND;TZID=Europe/Rome:20260615T153000
DTSTAMP:20260508T235039
CREATED:20260508T144151Z
LAST-MODIFIED:20260508T144151Z
UID:40727-1781533800-1781537400@w3.lnf.infn.it
SUMMARY:New Physics searches at BESIII
DESCRIPTION:Speaker: Vindy Prasad (Jilin Univ.) \nThe Standard Model (SM) successfully describes fundamental particles and their interactions but fails to explain several outstanding issues\, including the nature of dark matter (DM). DM constitutes approximately one quarter of the total matter density of the universe and is invisible across the electromagnetic spectrum. It may account for observed anomalies such as galaxy rotation curves and other fundamental characteristics of our universe. DM may couple to SM particles via portals. These portals introduce several new physics particles\, such as light Higgs boson\, dark photon\, axion-like particle\, and sterile neutrinos. \nThese new physics scenarios may also appear in several baryon- and lepton-number-violating processes. Furthermore\, the origin of DM and the observed asymmetry between visible matter and antimatter may be connected through the introduction of a dark baryon. \nThe new physics particles can be accessible at high-intensity electron-positron collider experiments\, such as the BESIII experiment\, if their masses are in the MeV-GeV range. BESIII has recently explored the possibilities of these new physics scenarios using large data samples collected at several energy points\, including the J/psi\, psi(2S) and psi(3770) resonances. \nThis talk will review the recent BESIII results related to searches for new physics.
URL:/event/new-physics-searches-at-besiii/
LOCATION:Aula B-1\, Via Enrico Fermi\, 40\, Frascati\, Roma\, 00044\, Italia
CATEGORIES:Seminari generali
END:VEVENT
END:VCALENDAR