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DTSTART:20240331T010000
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DTSTART;TZID=Europe/Rome:20240617T083000
DTEND;TZID=Europe/Rome:20240621T200000
DTSTAMP:20260509T194737
CREATED:20231125T113428Z
LAST-MODIFIED:20240513T100829Z
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SUMMARY:Present and future perspectives in Hadron Physics
DESCRIPTION:The Workshop will be held in person from 17 to 19 June 2024\, in Frascati (Italy) in the context of the project STRONG-2020 (http://www.strong-2020.eu/).The objective is to gather a broad Hadron Physics Community\, including both young and experienced researchers. The first day will be dedicated to selected contributions. STRONG-2020 offers an opportunity to cover local and travel expenses for young researchers.During the second and third days\, invited speakers will present their work and perspectives in various areas of Hadron Physics and related fields.  The Workshop will be followed by the STRONG-2020 Annual Meeting organized in Frascati on 20-21 June 2024 and open to a large audience. The Agenda will be soon available and the Registration is possible at the dedicated site here.   This project has received funding from the European Union’s Horizon 2020 research and innovation programme under grant agreement No 824093 
URL:/event/present-and-future-perspectives-in-hadron-physics-in-the-21st-century/
LOCATION:Auditorium B. Touschek\, Via Enrico Fermi\, 54\, Frascati\, Roma\, 00044\, Italia
CATEGORIES:Conferenze & Workshops
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DTSTART;TZID=Europe/Rome:20240619T143000
DTEND;TZID=Europe/Rome:20240619T170000
DTSTAMP:20260509T194737
CREATED:20240604T114935Z
LAST-MODIFIED:20240613T121226Z
UID:37712-1718807400-1718816400@w3.lnf.infn.it
SUMMARY:Axion emission from strange matter in core-collapse supernova events
DESCRIPTION:The duration of the neutrino burst from the supernova event SN 1987A is known to be sensitive to exotic sources of cooling\, such as axions radiated from the dense and hot hadronic matter thought to constitute the inner core of the supernova. We perform the first quantitative study of the role of hadronic matter beyond the first generation — in particular strange matter. We do so by consistently including the full baryon and meson octets\, and computing axion emissivity induced from baryon-meson to baryon-axion scatterings as well as from baryon decays. We consider a range of supernova thermodynamic conditions\, including equation-of-state models with different strangeness content\, in order to make sure our results are robust. We obtain the first bound on the axial axion-strange-strange coupling\, as well as the strongest existing bound on the axion-down-strange counterpart. Our bound on this coupling can be as small as O(10^−2) for the QCD axion\, i.e. for an axion decay constant f_a = 10^9 GeV.  Join Zoom Meetinghttps://infn-it.zoom.us/j/98320147600?pwd=r7X6GpLqnWK9h9wnZKgj3g3ePNICEw.1Meeting ID: 983 2014 7600Passcode: 392002 
URL:/event/axion-emission-from-strange-matter-in-core-collapse-supernova-events/
LOCATION:Aula Salvini
CATEGORIES:Seminari generali
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