AbstractAfter measuring the last neutrino mixing angle θ13 and finding it relatively large, the observation of CP violation in the leptonic sector is now reachable with the condition to have significantly more intense neutrino beams than the existing ones. For this θ13 value, it came out that going to the second oscillation maximum instead of the first one, provides more sensitivity to CP violation. The European Spallation Source facility in Lund, designed to accelerate protons to 2.0GeV at a repetition rate of 14Hz for neutron production, could also be used to produce a copious number of neutrinos. Doubling the frequency of its proton linac opens the possibility to operate the facility simultaneously for neutron and neutrino production. An...
This conceptual design report provides a detailed account of the European Spallation Source neutrino...
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...
AbstractAfter measuring the last neutrino mixing angle θ13 and finding it relatively large, the obse...
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...
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 ...
The value of the neutrino mixing angle θ13 privileges the second oscillation maximum for the discove...
International audienceAfter measuring in 2012 a relatively large value of the neutrino mixing angle ...
The European Spallation Source (ESS), currently under construction in Lund, Sweden, is a research ce...
The European Spallation Source (ESS), currently under construction in Lund, Sweden, is a research ce...
Very intense neutrino beams and large neutrino detectors will be needed to enable the discovery of C...
This conceptual design report provides a detailed account of the European Spallation Source neutrino...
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...
AbstractAfter measuring the last neutrino mixing angle θ13 and finding it relatively large, the obse...
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...
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 ...
The value of the neutrino mixing angle θ13 privileges the second oscillation maximum for the discove...
International audienceAfter measuring in 2012 a relatively large value of the neutrino mixing angle ...
The European Spallation Source (ESS), currently under construction in Lund, Sweden, is a research ce...
The European Spallation Source (ESS), currently under construction in Lund, Sweden, is a research ce...
Very intense neutrino beams and large neutrino detectors will be needed to enable the discovery of C...
This conceptual design report provides a detailed account of the European Spallation Source neutrino...
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...