2020
DOI: 10.2172/1784163
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Final Design Report. Proton Power Upgrade Project

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Cited by 6 publications
(5 citation statements)
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“…The decay-at-rest production results in an intense, pulsed, and isotropic source of neutrinos with energies up to 52 MeV. The planned Proton Power Upgrade (PPU) will increase the SNS proton power on target from 1.4 MW to 2.8 MW by 2028 [12]. This power increase entails a staged 50% increase in the beam current, from 26 to 38 mA; neutrino production will scale linearly with this increase.…”
Section: B Neutrinos At the Snsmentioning
confidence: 99%
See 1 more Smart Citation
“…The decay-at-rest production results in an intense, pulsed, and isotropic source of neutrinos with energies up to 52 MeV. The planned Proton Power Upgrade (PPU) will increase the SNS proton power on target from 1.4 MW to 2.8 MW by 2028 [12]. This power increase entails a staged 50% increase in the beam current, from 26 to 38 mA; neutrino production will scale linearly with this increase.…”
Section: B Neutrinos At the Snsmentioning
confidence: 99%
“…A comparison of the power deposition profiles at the SNS for operations after (left) and before (right) the PPU. Reproduced from [12].…”
Section: B Neutrinos At the Snsmentioning
confidence: 99%
“…Another approach that has been considered employs a target design which is capable of handling short highpower pulses on the order of 1 µs, similarly to the case at SNS following the Proton Power Upgrade [171]. In such a scenario, the same fast-kicker extraction as for neutrino production, with the same low losses, could be used for the neutron production.…”
Section: Generation Of Short Neutron Pulsesmentioning
confidence: 99%
“…Fig 171. Muon neutrino interaction in the SFGD cube with a secondary muon producing Cherenkov light in the near water Cherenkov detector…”
mentioning
confidence: 99%
“…The allowed region was shown to shrink by roughly a factor of 2, assuming a reduction in the flux uncertainty from the current 10 % to an uncertainty of 3 %, matching the theoretical uncertainty of the ν e + d cross section. Following this initial program to calibrate the neutrino flux for 1 GeV protons at the SNS, the detector will also be used to calibrate the flux at 1.3 GeV following the SNS Proton Power Upgrade [69]. It will later be moved to the ORNL SNS Second Target Station [70] to further support future neutrino efforts at the SNS.…”
Section: Discussionmentioning
confidence: 99%