NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = J.F.Beacom Found 11 matches. 2019ZH29 Phys.Rev. C 99, 055810 (2019) Developing the MeV potential of DUNE: Detailed considerations of muon-induced spallation and other backgrounds NUCLEAR REACTIONS 40Ar(μ, X)8B/8He/8Li/9Li/9C/11Be/11Be/11Li/12B/12N/12Be/13O/13B/14B/15C/16C/16N/17N/18N/20F/23F/26Na/27Na/29Mg/30Al/31Al/32Al/32P/33P/34P/35S/36Cl/37Ar/38Cl/39Cl/39Ar/40Cl/41Ar, E=1-10000 GeV; calculated β-decaying isotopic production yield from cosmic ray muon spallation on liquid argon in the Deep Underground Neutrino Experiment (DUNE), spallation product β--decay spectra and time evolution, and data cuts for background minimization using the Monte Carlo code FLUKA; quantified rates of single and multiple MeV events due to spallation, radiogenic neutron capture, and other background activities. Comparison with other calculated yields from spallation reactions.
doi: 10.1103/PhysRevC.99.055810
2014LI16 Phys.Rev. C 89, 045801 (2014) First calculation of cosmic-ray muon spallation backgrounds for MeV astrophysical neutrino signals in Super-Kamiokande NUCLEAR REACTIONS 18O(n, X), (π+, X), (π-, X), (μ-, X), (γ, X), [π and γ from interaction of cosmic muons with water], E=high energy; calculated yields of spallation products from interaction of cosmic-ray muons with water, and resultant background from β decays of spallation products of 8He, 8,9,11Li, 8,12,13,14B, 9,15,16C, 11,12Be, 12,16,17,18N, 13O, and that by stable isotopes of 9,10Be, 10,11B, 10,11,12,13,14C, 13,14,15N, 14,15O; calculated simulated cosmic-ray muon flux spectrum, energy loss for vertical through-going muons passing through Super-Kamiokande (Super-K) fiducial volume, secondary particle path length spectra and absorption distance produced by cosmic-ray muons in Super-K, spallation decay rate distribution and background energy spectra, parent particle kinetic energy spectra, cumulative distribution of isotopes perpendicular to the muon track. Relevance to backgrounds for experiments concerned with detection of solar neutrinos or diffuse supernova neutrino background (DSNB) signals as in Super-Kamiokande project. Used simulation code FLUKA and other theoretical insights. Comparison with available experimental data from Super-Kamiokande.
doi: 10.1103/PhysRevC.89.045801
2007AN07 Phys.Rev.Lett. 98, 121101 (2007) L.A.Anchordoqui, J.F.Beacom, H.Goldberg, S.Palomares-Ruiz, T.J.Weiler TeV γ Rays from Photodisintegration and Daughter Deexcitation of Cosmic-Ray Nuclei
doi: 10.1103/PhysRevLett.98.121101
2006BE13 Phys.Rev. C 73, 035807 (2006) New test of supernova electron neutrino emission using Sudbury Neutrino Observatory sensitivity to the diffuse supernova neutrino background
doi: 10.1103/PhysRevC.73.035807
2006YU06 Phys.Rev. C 74, 015803 (2006) Direct measurement of supernova neutrino emission parameters with a gadolinium-enhanced Super-Kamiokande detector
doi: 10.1103/PhysRevC.74.015803
2005GA34 Phys.Rev. C 72, 025807 (2005); Erratum Phys.Rev. C 73, 049906 (2006) Measuring the cosmic ray muon-induced fast neutron spectrum by (n, p) isotope production reactions in underground detectors NUCLEAR REACTIONS 12C, 16O(n, p), (μ-, ν), E=low; calculated reaction rates in underground detectors.
doi: 10.1103/PhysRevC.72.025807
2003BE36 Phys.Rev. D 67, 093001 (2003) Neutral-current atmospheric neutrino flux measurement using neutrino-proton elastic scattering in Super-Kamiokande NUCLEAR REACTIONS 1H(ν, ν), E=1-50 GeV; calculated σ(θ), proton recoil momentum. Application to atmospheric neutrino flux measurement discussed.
doi: 10.1103/PhysRevD.67.093001
2001BE60 Phys.Rev. D64, 091302 (2001) Normalization of the Neutrino-Deuteron Cross Section NUCLEAR REACTIONS 2H(ν, ep), E=12 MeV; calculated σ(E), radiative corrections, normalization features. Comparison of solar neutrino flux in different detectors.
doi: 10.1103/PhysRevD.64.091302
2001MA02 Phys.Rev. C63, 015801 (2001) L.E.Marcucci, R.Schiavilla, M.Viviani, A.Kievsky, S.Rosati, J.F.Beacom Weak Proton Capture on 3He NUCLEAR REACTIONS 3He(p, e+ν), E(cm)=0, 5, 10 keV; calculated astrophysical S-factors. Correlated hyperspherical harmonics method. Comparison with data.
doi: 10.1103/PhysRevC.63.015801
1999VO14 Phys.Rev. D60, 053003 (1999) Angular Distribution of Neutron Inverse Beta Decay, (ν-bar)e + p → e+ + n NUCLEAR REACTIONS 1H(ν, e+), E ≤ 60 MeV; calculated total σ, positrons, neutrons σ(θ); deduced role of weak magnetism, recoil corrections.
doi: 10.1103/PhysRevD.60.053003
1998BA96 J.Phys.(London) G24, 2087 (1998) A.B.Balantekin, J.F.Beacom, M.A.Candido Ribeiro Green's Function for Nonlocal Potentials
doi: 10.1088/0954-3899/24/11/010
Back to query form |