International audienceThe measured relatively high value of $\theta_{13}$ in 2012 privileges the 2nd neutrino oscillation maximum for the discovery of CP violation in the leptonic sector instead of the usually used 1st oscillation maximum.At the 2nd oscillation maximum the importance of systematic errors is significantly less while the sensitivity to CP violation is about three times higher than for the 1st oscillation maximum.Compared to the 1st oscillation maximum, for the same neutrino energy, the far detector has to be placed in a distance about three times longer than for the 1st oscillation maximum.For this a very intense neutrino beam is necessary.The European Spallation Source under construction, will have a proton linac of 5 MW pow...
AbstractIn addition to the world's most intense pulsed spallation neutron source, the European Spall...
AbstractVery intense neutrino beams and large neutrino detectors will be needed in order to enable t...
Very intense neutrino beams and large neutrino detectors will be needed in order to enable the disco...
International audienceThe measured relatively high value of $\theta_{13}$ in 2012 privileges the 2nd...
International audienceAfter measuring in 2012 a relatively large value of the neutrino mixing angle ...
International audienceAfter measuring in 2012 a relatively large value of the neutrino mixing angle ...
International audienceAfter measuring in 2012 a relatively large value of the neutrino mixing angle ...
International audienceAfter measuring in 2012 a relatively large value of the neutrino mixing angle ...
International audienceThe relatively large value of the neutrino mixing angle $\theta_{13}$ measured...
This conceptual design report provides a detailed account of the European Spallation Source neutrino...
International audienceAfter measuring in 2012 a relatively large value of the neutrino mixing angle ...
The value of the neutrino mixing angle θ13 privileges the second oscillation maximum for the discove...
AbstractAfter measuring the last neutrino mixing angle θ13 and finding it relatively large, the obse...
This conceptual design report provides a detailed account of the European Spallation Source neutrino...
International audienceIn addition to the world's most intense pulsed spallation neutron source, the ...
AbstractIn addition to the world's most intense pulsed spallation neutron source, the European Spall...
AbstractVery intense neutrino beams and large neutrino detectors will be needed in order to enable t...
Very intense neutrino beams and large neutrino detectors will be needed in order to enable the disco...
International audienceThe measured relatively high value of $\theta_{13}$ in 2012 privileges the 2nd...
International audienceAfter measuring in 2012 a relatively large value of the neutrino mixing angle ...
International audienceAfter measuring in 2012 a relatively large value of the neutrino mixing angle ...
International audienceAfter measuring in 2012 a relatively large value of the neutrino mixing angle ...
International audienceAfter measuring in 2012 a relatively large value of the neutrino mixing angle ...
International audienceThe relatively large value of the neutrino mixing angle $\theta_{13}$ measured...
This conceptual design report provides a detailed account of the European Spallation Source neutrino...
International audienceAfter measuring in 2012 a relatively large value of the neutrino mixing angle ...
The value of the neutrino mixing angle θ13 privileges the second oscillation maximum for the discove...
AbstractAfter measuring the last neutrino mixing angle θ13 and finding it relatively large, the obse...
This conceptual design report provides a detailed account of the European Spallation Source neutrino...
International audienceIn addition to the world's most intense pulsed spallation neutron source, the ...
AbstractIn addition to the world's most intense pulsed spallation neutron source, the European Spall...
AbstractVery intense neutrino beams and large neutrino detectors will be needed in order to enable t...
Very intense neutrino beams and large neutrino detectors will be needed in order to enable the disco...