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SUMMARY:Webinar: The Axiflavon
DTSTART;VALUE=DATE-TIME:20170314T140000Z
DTEND;VALUE=DATE-TIME:20170314T150000Z
DTSTAMP;VALUE=DATE-TIME:20260430T013041Z
UID:indico-event-2953@indico.ific.uv.es
DESCRIPTION:\n    Solving the flavor problem of the Standard Model with a 
 simple U(1)_H flavor symmetry naturally leads to an axion that solves the 
 strong CP problem and constitutes a viable Dark Matter candidate. In this 
 framework\, the ratio of the axion mass and its coupling to photons is rel
 ated to the SM fermion masses and predicted within a small range\, as a di
 rect result of the observed hierarchies in quark and charged lepton masses
 . The same hierarchies determine the axion couplings to fermions\, making 
 the framework very predictive and experimentally testable by future axion 
 and precision flavor experiments\n\nhttps://indico.ific.uv.es/event/2953/
LOCATION:Online http://reunion.uv.es/webinar140317/
URL:https://indico.ific.uv.es/event/2953/
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