Cosmic ray (CR) interactions can be a challenging source of background for neutrino oscillation and cross-section measurements in surface detectors. We present methods for CR rejection in measurements of charged-current quasielastic-like (CCQE-like) neutrino interactions, with a muon and a proton in the final state, measured using liquid argon time projection chambers (LArTPCs). Using a sample of cosmic data collected with the MicroBooNE detector, mixed with simulated neutrino scattering events, a set of event selection criteria is developed that produces an event sample with minimal contribution from CR background. Depending on the selection criteria used a purity between 50 and 80% can be achieved with a signal selection efficiency betwee...
Primary challenges for current and future precision neutrino experiments using liquid argon time pro...
We present a measurement of νe interactions from the Fermilab Booster Neutrino Beam using the Micro...
We present a search for eV-scale sterile neutrino oscillations in the MicroBooNE liquid argon detect...
For a large liquid argon time projection chamber (LArTPC) operating on or near the Earth's surface t...
Thanks to the good tracking and calorimetric capabilities of a Liquid Argon Time Projection Chamber ...
Abstract: Cosmic ray (CR) interactions can be a challenging source of background for neutrino oscill...
Cosmic ray (CR) interactions can be a challenging source of background for neutrino oscillation and ...
Cosmic ray (CR) interactions can be a challenging source of background for neutrino oscillation and ...
Cosmic ray (CR) interactions can be a challenging source of background for neutrino oscillation and ...
Cosmic ray (CR) interactions can be a challenging source of background for neutrino oscillation and ...
The MicroBooNE detector utilizes a liquid argon time projection chamber (LArTPC) with an 85 t active...
Primary challenges for current and future precision neutrino experiments using liquid argon time pro...
Primary challenges for current and future precision neutrino experiments using liquid argon time pro...
Primary challenges for current and future precision neutrino experiments using liquid argon time pro...
Primary challenges for current and future precision neutrino experiments using liquid argon time pro...
Primary challenges for current and future precision neutrino experiments using liquid argon time pro...
We present a measurement of νe interactions from the Fermilab Booster Neutrino Beam using the Micro...
We present a search for eV-scale sterile neutrino oscillations in the MicroBooNE liquid argon detect...
For a large liquid argon time projection chamber (LArTPC) operating on or near the Earth's surface t...
Thanks to the good tracking and calorimetric capabilities of a Liquid Argon Time Projection Chamber ...
Abstract: Cosmic ray (CR) interactions can be a challenging source of background for neutrino oscill...
Cosmic ray (CR) interactions can be a challenging source of background for neutrino oscillation and ...
Cosmic ray (CR) interactions can be a challenging source of background for neutrino oscillation and ...
Cosmic ray (CR) interactions can be a challenging source of background for neutrino oscillation and ...
Cosmic ray (CR) interactions can be a challenging source of background for neutrino oscillation and ...
The MicroBooNE detector utilizes a liquid argon time projection chamber (LArTPC) with an 85 t active...
Primary challenges for current and future precision neutrino experiments using liquid argon time pro...
Primary challenges for current and future precision neutrino experiments using liquid argon time pro...
Primary challenges for current and future precision neutrino experiments using liquid argon time pro...
Primary challenges for current and future precision neutrino experiments using liquid argon time pro...
Primary challenges for current and future precision neutrino experiments using liquid argon time pro...
We present a measurement of νe interactions from the Fermilab Booster Neutrino Beam using the Micro...
We present a search for eV-scale sterile neutrino oscillations in the MicroBooNE liquid argon detect...