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Booster Neutrino Flux Prediction at MicroBooNE

Research output: Working paperPreprint

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Booster Neutrino Flux Prediction at MicroBooNE. / MicroBooNE Collaboration.
2018.

Research output: Working paperPreprint

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MicroBooNE Collaboration. Booster Neutrino Flux Prediction at MicroBooNE. 2018 Jul 6. doi: 10.2172/1573216

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MicroBooNE Collaboration. / Booster Neutrino Flux Prediction at MicroBooNE. 2018.

Bibtex

@techreport{e3b04732ad1749bd88693143c6bcd9dc,
title = "Booster Neutrino Flux Prediction at MicroBooNE",
abstract = "The primary source of neutrinos for the MicroBooNE experiment is Fermilab{\textquoteright}s Booster Neutrino Beamline. The beamline uses 8 GeV protons from the Booster accelerator steered onto a beryllium target. The secondaries are focused by a magnetic horn down a 50m long decay pipe. Decays of these secondaries give rise to a neutrino beam. We use the beamline simulation and techniques previously developed by the MiniBooNE collaboration to calculate the neutrino flux and estimate systematic uncertainties at the MicroBooNE detector location.",
author = "{MicroBooNE Collaboration} and Jaroslaw Nowak",
year = "2018",
month = jul,
day = "6",
doi = "10.2172/1573216",
language = "English",
type = "WorkingPaper",

}

RIS

TY - UNPB

T1 - Booster Neutrino Flux Prediction at MicroBooNE

AU - MicroBooNE Collaboration

AU - Nowak, Jaroslaw

PY - 2018/7/6

Y1 - 2018/7/6

N2 - The primary source of neutrinos for the MicroBooNE experiment is Fermilab’s Booster Neutrino Beamline. The beamline uses 8 GeV protons from the Booster accelerator steered onto a beryllium target. The secondaries are focused by a magnetic horn down a 50m long decay pipe. Decays of these secondaries give rise to a neutrino beam. We use the beamline simulation and techniques previously developed by the MiniBooNE collaboration to calculate the neutrino flux and estimate systematic uncertainties at the MicroBooNE detector location.

AB - The primary source of neutrinos for the MicroBooNE experiment is Fermilab’s Booster Neutrino Beamline. The beamline uses 8 GeV protons from the Booster accelerator steered onto a beryllium target. The secondaries are focused by a magnetic horn down a 50m long decay pipe. Decays of these secondaries give rise to a neutrino beam. We use the beamline simulation and techniques previously developed by the MiniBooNE collaboration to calculate the neutrino flux and estimate systematic uncertainties at the MicroBooNE detector location.

U2 - 10.2172/1573216

DO - 10.2172/1573216

M3 - Preprint

BT - Booster Neutrino Flux Prediction at MicroBooNE

ER -