Neutrino backgrounds to dark matter searches
Physical Review D Particles Fields Gravitation and Cosmology 76:3 (2007)
Abstract:
Neutrino coherent scattering cross sections can be as large as 10-39cm2, while current dark matter experiments have sensitivities to WIMP coherent scattering cross sections 5 orders of magnitude smaller; future experiments plan to have sensitivities to cross sections as small as 10-48cm2. With large target masses and few keV recoil energy detection thresholds, neutral current coherent scattering of solar neutrinos becomes an irreducible background in dark matter searches. In the current zero-background analysis paradigm, neutrino coherent scattering will limit the achievable sensitivity to dark matter scattering cross sections, at the level of 10-46cm2. © 2007 The American Physical Society.Search for Electron Neutrino Appearance at the Δm2∼1 eV2 Scale
Physical Review Letters American Physical Society (APS) 98:23 (2007) 231801
Charged current quasi-elastic interactions at MiniBooNE confront cross section Monte Carlos
Nuclear Physics B Proceedings Supplements 139:1-3 SPEC. ISS. (2005) 59-65
Abstract:
Neutrino oscillations have been established in solar and atmospheric neutrinos, but a third signal from the LSND experiment is incompatible with three Standard Model neutrinos. The MiniBooNE experiment can confirm or refute the LSND oscillation signal with 1 × 1021 protons on target. While working towards the oscillation result, MiniBooNE will accumulate more than 1 × 106 neutrino interactions in the 0 to 2 GeV range which will greatly increase the world's knowledge of neutrino cross sections in this energy regime. Preliminary results on the MiniBooNE νFermilab booster orbit correction
Proceedings of the IEEE Particle Accelerator Conference 3 (2003) 1587-1589
Abstract:
The Fermilab particle physics program has recently expanded to include the MiniBooNE experiment in addition to the RunII program. As a result, the effective and reliable performance of the Fermilab Booster has become crucial to the lab. The Booster is an 8 GeV proton synchrotron and is a key element of the Fermilab accelerator chain. It must meet increasing demands for proton intensity and high repetition rates. One important requirement placed on the machine is low radiation levels. These levels are highly correlated with losses in the machine, and can limit Booster production. We will describe how a system of ramped dipole corrector magnets are being used to maintain orbital position throughout the acceleration cycle in order to minimize beam losses, maximize proton intensity, and maintain the required repetition rate.Initial operation of the Fermilab MiniBooNE beamline
Proceedings of the IEEE Particle Accelerator Conference 3 (2003) 1652-1654