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Insertion of STC into TRT at the Department of Physics, Oxford
Credit: CERN

Giles Barr

Professor of Physics

Sub department

  • Particle Physics

Research groups

  • Accelerator Neutrinos
Giles.Barr@physics.ox.ac.uk
Telephone: 01865 (2)73446
Denys Wilkinson Building, room 664a
  • About
  • Publications

The NA31 transition radiation detector

IEEE Transactions on Nuclear Science Institute of Electrical and Electronics Engineers (IEEE) 36:1 (1989) 66-70
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Flux of atmospheric neutrinos

Physical Review D 39:11 (1989) 3532-3534

Authors:

G Barr, TK Gaisser, T Stanev

Abstract:

We have repeated a one-dimensional calculation of neutrino fluxes, including the effect of muon polarization on neutrinos from the decay of muons. Fluxes have been calculated as a function of energy and angle with cutoffs appropriate for locations of five deep nucleon-decay experiments. Overall, the e/ ratio increases by 5% (20%) for neutrinos with energies around 200 MeV (2"3 GeV), in agreement with a previous analytic estimate of the effect. © 1989 The American Physical Society.
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Cosmic-ray neutrinos in the atmosphere

Physical Review D 38:1 (1988) 85-95

Authors:

TK Gaisser, T Stanev, G Barr

Abstract:

In this paper we give a complete account of detailed calculations of the flux of neutrinos of atmospheric origin that we have made for detectors at various locations on the globe. The emphasis here is on neutrinos in the energy range around 1 GeV, and we compare the results with recent measurements made with larger underground detectors. A detailed knowledge of the atmospheric cosmic-ray neutrino flux is a prerequisite for evaluating the background for the search for nucleon decay as well as the background for neutrinos of extraterrestrial origin. © 1988 The American Physical Society.
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SEARCH FOR THE DECAY KL- PI-OE+E

214 (1988) 303-306

Authors:

GD Barr, P Clarke, D Coward, D Cundy, N Doble, L Gatignon, V Gibson, R Hagelberg, G Kesseler, J Vanderlans, T Miczaika, HN Nelson, J Steinberger, H Taureg, H Wahl, C Youngman, R Black, DJ Candlin, J Muir, KJ Peach, B Pijlgroms, IP Shipsey, W Stephenson, H Blumer, R Heinz, M Kasemann, K Kleinknecht, P Mayer, B Panzer, B Renk, H Rohrer, E Auge, RL Chase, M Corti, D Fournier, P Heusse, L Iconomidoufayard, I Harrus, AM Lutz, HG Sander, AC Schaffer, L Bertanza, A Bigi, P Calafiura, M Calvetti, R Carosi, R Casali, C Cerri, I Mannelli, A Nappi, GM Pierazzini, H Burkhardt, M Holder, G Quast, M Rost, W Weihs, G Zech
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Measurement of the $ν_μ$ charged-current cross sections on water, hydrocarbon, iron, and their ratios with the T2K on-axis detectors

Authors:

K Abe, R Akutsu, A Ali, C Andreopoulos, L Anthony, M Antonova, S Aoki, A Ariga, Y Ashida, Y Awataguchi, Y Azuma, S Ban, M Barbi, GJ Barker, G Barr, C Barry, M Batkiewicz-Kwasniak, F Bench, V Berardi, S Berkman, RM Berner, L Berns, S Bhadra, S Bienstock, A Blondely, S Bolognesi, B Bourguille, SB Boyd, D Brailsford, A Bravar, C Bronner, MB Avanzini, J Calcutt, T Campbell, S Cao, SL Cartwright, A Cervera, A Chappell, C Checchia, D Cherdack, N Chikuma, G Christodoulouy, J Coleman, G Collazuol, D Coplowe, A Cudd, A Dabrowska, GD Rosa, T Dealtry

Abstract:

We report a measurement of the flux-integrated $\nu_{\mu}$ charged-current cross sections on water, hydrocarbon, and iron in the T2K on-axis neutrino beam with a mean neutrino energy of 1.5 GeV. The measured cross sections on water, hydrocarbon, and iron are $\sigma^{\rm{H_{2}O}}_{\rm{CC}}$ = (0.840$\pm 0.010$(stat.)$^{+0.10}_{-0.08}$(syst.))$\times$10$^{-38}$cm$^2$/nucleon, $\sigma^{\rm{CH}}_{\rm{CC}}$ = (0.817$\pm 0.007$(stat.)$^{+0.11}_{-0.08}$(syst.))$\times$10$^{-38}$cm$^2$/nucleon, and $\sigma^{\rm{Fe}}_{\rm{CC}}$ = (0.859$\pm 0.003$(stat.) $^{+0.12}_{-0.10}$(syst.))$\times$10$^{-38}$cm$^2$/nucleon respectively, for a restricted phase space of induced muons: $\theta_{\mu}<45^{\circ}$ and $p_{\mu}>$0.4 GeV/$c$ in the laboratory frame. The measured cross section ratios are ${\sigma^{\rm{H_{2}O}}_{\rm{CC}}}/{\sigma^{\rm{CH}}_{\rm{CC}}}$ = 1.028$\pm 0.016$(stat.)$\pm 0.053$(syst.), ${\sigma^{\rm{Fe}}_{\rm{CC}}}/{\sigma^{\rm{H_{2}O}}_{\rm{CC}}}$ = 1.023$\pm 0.012$(stat.)$\pm 0.058$(syst.), and ${\sigma^{\rm{Fe}}_{\rm{CC}}}/{\sigma^{\rm{CH}}_{\rm{CC}}}$ = 1.049$\pm 0.010$(stat.)$\pm 0.043$(syst.). These results, with an unprecedented precision for the measurements of neutrino cross sections on water in the studied energy region, show good agreement with the current neutrino interaction models used in the T2K oscillation analyses.
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