Accelerator Neutrinos

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OBSERVATION OF THE DECAY KL- PI-0-GAMMA-GAMMA

242 (1990) 523-530

Authors:

GD Barr, R Carosi, D Coward, D Cundy, N Doble, L Gatignon, V Gibson, P Grafstrom, R Hagelberg, G Kesseler, J Vanderlans, HN Nelson, H Wahl, R Black, DJ Candlin, J Muir, KJ Peach, H Blumer, R Heinz, K Kleinknecht, P Mayer, B Panzer, B Renk, H Rohrer, E Auge, D Fournier, P Heusse, L Iconomidoufayard, I Harrus, AM Lutz, O Perdereau, AC Schaffer, L Serin, L Bertanza, A Bigi, P Calafiura, M Calvetti, R Casali, C Cerri, R Fantechi, I Mannelli, A Nappi, GM Pierazzini, H Burkhardt, M Holder, A Kreutz, G Quast, M Rost, HG Sander, W Weihs, R Werthenbach, G Zech
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SEARCH FOR A NEUTRAL HIGGS PARTICLE IN THE DECAY SEQUENCE KL0- PI-0H0 AND H0- E+E

235 (1990) 356-362

Authors:

GD Barr, P Clarke, D Coward, D Cundy, N Doble, L Gatignon, V Gibson, P Grafstrom, R Hagelberg, G Kesseler, J Vanderlans, T Miczaika, HN Nelson, 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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Energy of the 32-keV transition of 83Krm and the atomic mass difference between 3H and 3He.

Physical review. C, Nuclear physics 39:4 (1989) 1503-1510

Authors:

ST Staggs, RG Robertson, DL Wark, PP Nguyen, JF Wilkerson, TJ Bowles
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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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