Measurement of Pb(,X) production with a stopped-pion neutrino source
arXiv:2212.11295 · doi:10.1103/PhysRevD.108.072001
Abstract
Using neutrinos produced at the Spallation Neutron Source (SNS) at Oak Ridge National Laboratory (ORNL), the COHERENT collaboration has studied the Pb(,X) process with a lead neutrino-induced-neutron (NIN) detector. Data from this detector are fit jointly with previously collected COHERENT data on this process. A combined analysis of the two datasets yields a cross section that is times that predicted by the MARLEY event generator using experimentally-measured Gamow-Teller strength distributions, consistent with no NIN events at 1.8. This is the first inelastic neutrino-nucleus process COHERENT has studied, among several planned exploiting the high flux of low-energy neutrinos produced at the SNS.
11 pages, 9 figures, version accepted by Phys. Rev. D
References in corpus (10)
- Observation of Coherent Elastic Neutrino-Nucleus Scattering
- SNEWS 2.0: A Next-Generation SuperNova Early Warning System for Multi-messenger Astronomy
- Coherent Elastic Neutrino-Nucleus Scattering at the European Spallation Source
- Neutrino beams as a probe of the nuclear isospin and spin-isospin excitations
- Fitting the annual modulation in DAMA with neutrons from muons and neutrinos
- No role for neutrons, muons and solar neutrinos in the DAMA annual modulation results
- Nuclear de-excitations in low-energy charged-current scattering on Ar
- A DO detector for flux normalization of a pion decay-at-rest neutrino source
- Supernova neutrino fluxes in HALO-1kT, Super-Kamiokande, and JUNO
- Comment on "Fitting the annual modulation in DAMA with neutrons from muons and neutrinos''
Cited by in corpus (5)
- Measurement of the Electron-Neutrino Charged-Current Cross Sections on I with the COHERENT NaIE detector
- Theoretical tools for neutrino scattering: interplay between lattice QCD, EFTs, nuclear physics, phenomenology, and neutrino event generators
- Demonstration of neutron identification in neutrino interactions in the MicroBooNE liquid argon time projection chamber
- Supernova electron-neutrino interactions with xenon in the nEXO detector
- Supernova Detection at SNOLAB