Steve Biller: Publications

Measurement of the rate of ve + d → p + p + e^- interactions produced by ⁸B solar neutrinos at the sudbury neutrino observatory

Physical Review Letters 87:7 (2001)

Authors:

QR Ahmad, RC Allen, TC Andersen, JD Anglin, G Bühler, JC Barton, EW Beier, M Bercovitch, J Bigu, S Biller, RA Black, I Blevis, RJ Bardman, J Boger, E Bonvin, MG Boulay, MG Bowler, TJ Bowles, SJ Brice, MC Browne, TV Bullard, TH Burritt, K Cameron, J Cameron, YD Chan, M Chen, HH Chen, X Chen, MC Chon, BT Cleveland, ETH Clifford, JHM Cowan, DF Cowen, GA Cox, Y Dai, X Dai, F Dalnoki-Veress, WF Davidson, PJ Doe, G Doucas, MR Dragowsky, CA Duba, FA Duncan, J Dunmore, ED Earle, SR Elliott, HC Evans, GT Ewan, J Farine, H Fergani, AP Ferraris, RJ Ford, MM Fowler, K Frame, ED Frank, W Frati, JV Germani, S Gil, A Goldschmidt, DR Grant, RL Hahn, AL Hallin, ED Hallman, A Hamer, AA Hamian, RU Haq, CK Hargrove, PJ Harvey, R Hazama, R Heaton, KM Heeger, WJ Heintzelman, J Heise, RL Helmer, JD Hepburn, H Heron, J Hewett, A Hime, M Howe, JG Hykawy, MCP Isaac, P Jagam, NA Jelley, C Jillings, G Jonkmans, J Karn, PT Keener, K Kirch, JR Klein, AB Knox, RJ Komar, R Kouzes, T Kutter, CCM Kyba, J Law, IT Lawson, M Lay, HW Lee, KT Lesko, JR Leslie

Abstract:

The 8B flux from elastic scattering (ES) and charged current (CC) of electrons was recorded at the Sudbury Neutrino Observatory (SNO) between November 2, 1999 and January 15, 2001. Data were partitioned into two sets then analyzed. As a result, the first direct indication of a nonelectron flavor component in the solar neutrino flux was established.

Measurement of the Rate of nu_e + d -> p+p+e- Interactions Produced by B-8 Solar Neutrinos at the Sudbury Neutrino Observatory

Physical Review Letters 87 (2001) 071301 6pp

Authors:

SD Biller, Q.R. Ahmad, R.C. Allen, T.C. Anderson

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First neutrino observations from the sudbury neutrino observatory

Nuclear Physics B - Proceedings Supplements 91:1-3 (2001) 21-28

Authors:

AB McDonald, MG Boulay, E Bonvin, M Chen, FA Duncan, ED Earle, HC Evans, GT Ewan, RJ Ford, AL Hallin, PJ Harvey, JD Hepburn, C Jillings, HW Lee, JR Leslie, HB Mak, W McLatchie, BA Moffat, BC Robertson, P Skensved, B Sur, I Blevis, F Dalnoki-Veress, W Davidson, J Farine, DR Grant, CK Hargrove, I Levine, K McFarlane, T Noble, VM Novikov, M O'Neill, M Shatkay, C Shewchuk, D Sinclair, T Andersen, MC Chon, P Jagam, J Law, IT Lawson, RW Ollerhead, JJ Simpson, N Tagg, JX Wang, J Bigu, JHM Cowan, ED Hallman, RU Haq, J Hewett, JG Hykawy, G Jonkmans, A Roberge, E Saettler, MH Schwendener, H Seifert, R Tafirout, CJ Virtue, S Gil, J Heise, R Helmer, RJ Komar, T Kutter, CW Nally, HS Ng, R Schubank, Y Tserkovnyak, CE Waltham, EW Beier, DF Cowen, ED Frank, W Frati, PT Keener, JR Klein, C Kyba, DS McDonald, MS Neubauer, FM Newcomer, V Rusu, R van Berg, RG van de Water, P Wittich, TJ Bowles, SJ Brice, M Dragowsky, MM Fowler, A Goldschmidt, A Hamer, A Hime, K Kirch, JB Wilhelmy, JM Wouters, YD Chan, X Chen, MCP Isaac, KT Lesko, AD Marino, EB Norman, CE Okada, AWP Poon, AR Smith

Abstract:

The first neutrino observations from the Sudbury Neutrino Observatory are presented from preliminary analyses. Based on energy, direction and location, the data in the region of interest appear to be dominated by 8B solar neutrinos, detected by the charged current reaction on deuterium and elastic scattering from electrons, with very little background. Measurements of radioactive backgrounds indicate that the measurement of all active neutrino types via the neutral current reaction on deuterium will be possible with small systematic uncertainties. Quantitative results for the fluxes observed with these reactions will be provided when further calibrations have been completed.

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Sudbury neutrino observatory

Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 449:1 (2000) 172-207

Authors:

J Boger, RL Hahn, JK Rowley, AL Carter, B Hollebone, D Kessler, I Blevis, F Dalnoki-Veress, A Dekok, J Farine, DR Grant, CK Hargrove, G Laberge, I Levine, K McFarlane, H Mes, AT Noble, VM Novikov, M O'Neill, M Shatkay, C Shewchuk, D Sinclair, ETH Clifford, R Deal, ED Earle, E Gaudette, G Milton, B Sur, J Bigu, JHM Cowan, DL Cluff, ED Hallman, RU Haq, J Hewett, JG Hykawy, G Jonkmans, R Michaud, A Roberge, J Roberts, E Saettler, MH Schwendener, H Seifert, D Sweezey, R Tafirout, CJ Virtue, DN Beck, YD Chan, X Chen, MR Dragowsky, FW Dycus, J Gonzalez, MCP Isaac, Y Kajiyama, GW Koehler, KT Lesko, MC Moebus, EB Norman, CE Okada, AWP Poon, P Purgalis, A Schuelke, AR Smith, RG Stokstad, S Turner, I Zlimen, JM Anaya, TJ Bowles, SJ Brice, EI Esch, MM Fowler, A Goldschmidt, A Hime, AF McGirt, GG Miller, WA Teasdale, JB Wilhelmy, JM Wouters, JD Anglin, M Bercovitch, WF Davidson, RS Storey, S Biller, RA Black, RJ Boardman, MG Bowler, J Cameron, B Cleveland, AP Ferraris, G Doucas, H Heron, C Howard, NA Jelley, AB Knox, M Lay, W Locke, J Lyon, S Majerus, M Moorhead, M Omori

Abstract:

The Sudbury Neutrino Observatory is a second-generation water Cherenkov detector designed to determine whether the currently observed solar neutrino deficit is a result of neutrino oscillations. The detector is unique in its use of D2O as a detection medium, permitting it to make a solar model-independent test of the neutrino oscillation hypothesis by comparison of the charged- and neutral-current interaction rates. In this paper the physical properties, construction, and preliminary operation of the Sudbury Neutrino Observatory are described. Data and predicted operating parameters are provided whenever possible.

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TeV blazars: Status of observations

Astrophysical Letters and Communications 39:1-6 (1999) 9-16

Authors:

F Krennrich, SD Biller, IH Bond, PJ Boyle, SM Bradbury, AC Breslin, JH Buckley, AM Burdett, J Bussons Gordo, DA Carter-Lewis, M Catanese, MF Cawley, DJ Fegan, JP Finley, JA Gaidos, T Hall, AM Hillas, RC Lamb, RW Lessard, C Masterson, JE McEnery, G Mohanty, P Moriarty, J Quinn, AJ Rodgers, HJ Rose, FW Samuelson, GH Sembroski, R Srinivasan, VV Vassiliev, TC Weekes

Abstract:

The close relation between ground-based TeV observations and satellite borne γ-ray measurements has been important for the understanding of blazars. The observations which involve the TeV component in blazar studies are reviewed. © 1999 OPA (Overseas Publishers Association) N.V. Published by license under the Gordon and Breach Science Publishers imprint.

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Measurement of the rate of ve + d → p + p + e^- interactions produced by ⁸B solar neutrinos at the sudbury neutrino observatory

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Abstract:

Measurement of the Rate of nu_e + d -> p+p+e- Interactions Produced by B-8 Solar Neutrinos at the Sudbury Neutrino Observatory

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First neutrino observations from the sudbury neutrino observatory

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Sudbury neutrino observatory

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TeV blazars: Status of observations

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Measurement of the rate of ve + d → p + p + e- interactions produced by 8B solar neutrinos at the sudbury neutrino observatory

Authors:

Abstract:

Measurement of the Rate of nu_e + d -> p+p+e- Interactions Produced by B-8 Solar Neutrinos at the Sudbury Neutrino Observatory

Authors:

First neutrino observations from the sudbury neutrino observatory

Authors:

Abstract:

Sudbury neutrino observatory

Authors:

Abstract:

TeV blazars: Status of observations

Authors:

Abstract:

Measurement of the rate of ve + d → p + p + e^- interactions produced by ⁸B solar neutrinos at the sudbury neutrino observatory