In the presence of Non-Standard neutral current Interactions (NSI) a new solution to solar neutrino anomaly with cos 2 θ 12 < 0 appears. We investigate how this solution can be tested by upcoming intermediate baseline reactor experiments, JUNO and RENO-50. We point out a degeneracy between the two solutions when both hierarchy and the θ 12 octant are flipped. We then comment on how this degeneracy can be partially lifted by long baseline experiments sensitive to matter effects such as the NOvA experiment
We determine the neutrino parameters for MSW and vacuum oscillations (active and sterile neutrinos) ...
Recent SNO results give strong evidence that the solar neutrinos undergo the flavor conversion. Main...
AbstractThe KamLAND reactor antineutrino experiment has detected a 3.4σ flux suppression relative to...
In presence of non-standard neutrino interactions the neutrino avor evolution equation is affected b...
The robustness of the large mixing angle (LMA) oscillation (OSC) interpretation of the solar neutrin...
The next-generation neutrino experiment JUNO will determine the solar oscillation parameters - $\sin...
We present an updated analysis of solar and reactor neutrino data in the standard framework of neutr...
Dark matter detectors will soon be sensitive to Solar neutrinos via two distinct channels: coherent ...
I review the interpretation of solar and atmospheric neutrino data in terms neutrino oscillations an...
AbstractIt is well-known that in addition to the standard LMA solution to solar anomaly, there is an...
It is well-known that in addition to the standard LMA solution to solar anomaly, there is another so...
Solar neutrino studies triggered and largely motivated the major developments in neutrino physics in...
We present a solution of the solar neutrino deficit using three flavors of neutrinos within the R-pa...
We show that non-standard neutrino interactions (NSI) can be probed in future direct dark matter det...
We reanalyze the non-standard interaction (NSI) solutions to the solar neutrino problem in the light...
We determine the neutrino parameters for MSW and vacuum oscillations (active and sterile neutrinos) ...
Recent SNO results give strong evidence that the solar neutrinos undergo the flavor conversion. Main...
AbstractThe KamLAND reactor antineutrino experiment has detected a 3.4σ flux suppression relative to...
In presence of non-standard neutrino interactions the neutrino avor evolution equation is affected b...
The robustness of the large mixing angle (LMA) oscillation (OSC) interpretation of the solar neutrin...
The next-generation neutrino experiment JUNO will determine the solar oscillation parameters - $\sin...
We present an updated analysis of solar and reactor neutrino data in the standard framework of neutr...
Dark matter detectors will soon be sensitive to Solar neutrinos via two distinct channels: coherent ...
I review the interpretation of solar and atmospheric neutrino data in terms neutrino oscillations an...
AbstractIt is well-known that in addition to the standard LMA solution to solar anomaly, there is an...
It is well-known that in addition to the standard LMA solution to solar anomaly, there is another so...
Solar neutrino studies triggered and largely motivated the major developments in neutrino physics in...
We present a solution of the solar neutrino deficit using three flavors of neutrinos within the R-pa...
We show that non-standard neutrino interactions (NSI) can be probed in future direct dark matter det...
We reanalyze the non-standard interaction (NSI) solutions to the solar neutrino problem in the light...
We determine the neutrino parameters for MSW and vacuum oscillations (active and sterile neutrinos) ...
Recent SNO results give strong evidence that the solar neutrinos undergo the flavor conversion. Main...
AbstractThe KamLAND reactor antineutrino experiment has detected a 3.4σ flux suppression relative to...