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SUMMARY:Bulk neutrinos and core cooling in Supernovae
DTSTART;VALUE=DATE-TIME:20021122T110000Z
DTEND;VALUE=DATE-TIME:20021122T120000Z
DTSTAMP;VALUE=DATE-TIME:20261110T113422Z
UID:indico-event-1285@indico.ific.uv.es
DESCRIPTION:In a recent paper we discuss the phenomenology of neutrino mix
 ing with bulk fermions in the context of supernova physics. Following the 
 usual energy loss argument\, the core cooling strongly constraints the siz
 e of such extra dimensions and the mixing parameters. We show that these c
 onstraints can be widely relaxed due to a feedback mechanism that self-lim
 its the loss. This mechanism also affects the protoneutron star evolution 
 through a non trivial interplay with neutrino diffusion. Finally\, we disc
 uss the consistency with the SN1987A signal and possible effects on the ne
 utrino flux composition and the delayed explosion scenario.\n\nhttps://ind
 ico.ific.uv.es/event/1285/
LOCATION:Edf. Institutos de Investigación Sala de Juntas del IFIC
URL:https://indico.ific.uv.es/event/1285/
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