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SUMMARY:Webinar: Is a non-standard interaction a solution to the three neu
 trino tensions?
DTSTART;VALUE=DATE-TIME:20161018T130000Z
DTEND;VALUE=DATE-TIME:20161018T140000Z
DTSTAMP;VALUE=DATE-TIME:20260613T194659Z
UID:indico-event-2840@indico.ific.uv.es
DESCRIPTION:\n    In this work we present a scenario in which a nonstandar
 d interaction in neutrino propagation can explain the three major tensions
  in the neutrino oscillation data at present. These tensions are: (i) a no
 n-zero best-fit value of the non-standard oscillation parameters in the gl
 obal analysis of the solar and KamLAND data which rules out the standard o
 scillation scenario at  90% C.L\, (ii) the measurement of the non-maximal
  value of theta23 by Nova which excludes  maximal mixing at 2.5 sigma and
  (iii)  the discrepancy in the theta13 measurement by T2K and  reactors 
 at 90% C.L.  Our results show that all these three  anomalies can be exp
 lained if one assumes the existence of non-standard interactions in neutri
 no propagation  in the case of normal hierarchy.  In our scenario the ph
 ase of $\\epsilon_{e\\tau}$ is zero and the most favorable value of the Di
 rac CP phase is approximately 255 degrees.\n    \n    http://reunion.uv.es
 /webinar18102016/\n\nhttps://indico.ific.uv.es/event/2840/
LOCATION:IFIC retransmitted from Seminar Room\, 1.1.1
URL:https://indico.ific.uv.es/event/2840/
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