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In scintillator detectors, the forward displacement of the neutron in the reaction $bar u_e+pto e^++n$ provides neutrino directional information as demonstrated by the CHOOZ reactor experiment with 2,500 events. The near detector of the forthcoming Double Chooz experiment will collect $1.6times10^5$ events per year, enough to determine the average neutrino direction with a $1 sigma$ half-cone aperture of $2.3^circ$ in one year. It is more difficult to separate the two Chooz reactors that are viewed at a separation angle $phi=30^circ$. If their strengths are known and approximately equal, the azimuthal location of each reactor is obtained with $pm6^circ$ ($1 sigma$) and the probability of confusing them with a single source is less than 11%. Five years data reduce this ``confusion probability to less than 0.3%, i.e., a $3 sigma$ separation is possible. All of these numbers improve rapidly with increasing angular separation of the sources. For a setup with $phi=90^circ$ and one years data, the azimuthal $1 sigma$ uncertainty for each source decreases to $pm3.2^circ$. Of course, for Double Chooz the two reactor locations are known, allowing one instead to measure their individual one-year integrated power output to $pm11%$ ($1 sigma$), and their five-year integrated output to $pm4.8%$ ($1 sigma$).
The Double Chooz experiment presents improved measurements of the neutrino mixing angle $theta_{13}$ using the data collected in 467.90 live days from a detector positioned at an average distance of 1050 m from two reactor cores at the Chooz nuclear
Distinguishing the signals due to scattering of WIMP dark matter off of nuclear targets from those due to background noise is a major challenge. The Earths motion relative to the galactic halo should produce halo-dependent seasonal modulation in the
By correlating nuclear recoil directions with the Earths direction of motion through the Galaxy, a directional dark matter detector can unambiguously detect Weakly Interacting Massive Particles (WIMPs), even in the presence of backgrounds. Here, we d
The Double Chooz experiment has observed 8,249 candidate electron antineutrino events in 227.93 live days with 33.71 GW-ton-years (reactor power x detector mass x livetime) exposure using a 10.3 cubic meter fiducial volume detector located at 1050 m
The most challenging and impactful uncertainties that future accelerator-based measurements of neutrino oscillations must overcome stem from our limited ability to model few-GeV neutrino-nucleus interactions. In particular, it is crucial to better un