BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//CERN//INDICO//EN
BEGIN:VEVENT
SUMMARY:Confronting spin flavor solutions of the solar neutrino problem wi
 th current and future solar neutrino data
DTSTART;VALUE=DATE-TIME:20021218T110000Z
DTEND;VALUE=DATE-TIME:20021218T120000Z
DTSTAMP;VALUE=DATE-TIME:20261110T151418Z
UID:indico-event-1293@indico.ific.uv.es
DESCRIPTION:A global analysis of spin-flavour precession (SFP) solutions t
 o thesolar neutrino problem is given.We fix the neutrino magnetic moment t
 o be $10^{-11}$ Bohr magneton\,with a corresponding optimum self-consisten
 t magneto-hydrodynamicsmagnetic field profile with maximum strength of 80 
 KGauss in theconvective zone.We find that no LOW-quasi-vacuum or vacuum so
 lutions are present at 3sigma. In addition to the standard LMA oscillation
  solution\, thereare two SFP solutions\, in the resonant (RSFP) and non-re
 sonant (NRSFP)regimes. These two SFP solutions have a goodness of fit slig
 htlybetter than the LMA oscillation solution. We also discuss the role of 
 solar anti-neutrino searches in the fit.Should KamLAND confirm the LMA sol
 ution\, the SFP solutions may at bestbe present at a sub-leading level. In
  the event LMA is not the solution realized in nature\,then experiments su
 ch as Borexino can help distinguishing LMA from theNRSFP solution and the 
 simplest RSFP solution with no mixing.\n\nhttps://indico.ific.uv.es/event/
 1293/
LOCATION:Edf. Institutos de Investigación Sala de Juntas del IFIC
URL:https://indico.ific.uv.es/event/1293/
END:VEVENT
END:VCALENDAR