Nick Jelley: Publications

The calibration of the Sudbury Neutrino Observatory using uniformly distributed radioactive sources

ArXiv 0912.2991 (2009)

Authors:

K Boudjemline, B Cai, BT Cleveland, HC Evans, GT Ewan, J Farine, RJ Ford, E Guillian, AL Hallin, ED Hallman, C Howard, P Jagam, NA Jelley, KJ Keeter, JR Klein, C Kraus, CB Krauss, R Lange, IT Lawson, JR Leslie, JC Loach, AB McDonald, G McGregor, AJ Noble, HM O'Keeffe, SJM Peeters, AWP Poon, SD Reitzner, K Rielage, RGH Robertson, VL Rusu, SR Seibert, P Skensved, MJ Thomson

Abstract:

The production and analysis of distributed sources of 24Na and 222Rn in the Sudbury Neutrino Observatory (SNO) are described. These unique sources provided accurate calibrations of the response to neutrons, produced through photodisintegration of the deuterons in the heavy water target, and to low energy betas and gammas. The application of these sources in determining the neutron detection efficiency and response of the 3He proportional counter array, and the characteristics of background Cherenkov light from trace amounts of natural radioactivity is described.

The Sudbury Neutrino Observatory

Annual Review of Nuclear and Particle Science 59 (2009) 431-465

Authors:

N Jelley, AB McDonald, RG Hamish Robertson

Abstract:

The solar neutrino problem arose when the first measurements of the flux of neutrinos from the Sun, taken by Raymond Davis, Jr. with a Cl-Ar radiochemical detector, fell substantially below the value predicted theoretically by John Bahcall. Bahcall's prediction came from a detailed model of the nuclear reactions powering the Sun. Resolution of the problem came three decades later with the observation of nonelectron flavors of neutrinos in the solar flux. The use of heavy water in the Sudbury Neutrino Observatory (SNO) experiment provided a means to measure both electron and nonelectron components, and the presence of the latter showed that neutrino flavor conversion was taking place - a hallmark of neutrino oscillation and mass. The solar models were vindicated, and the Standard Model of elementary particles and fields had to be revised. Here we present an account of the SNO project, its conclusions to date, and its ongoing analysis. Copyright © 2009 by Annual Reviews. All rights reserved.

High sensitivity measurement of ²²⁴Ra and ²²⁶Ra in water with an improved hydrous titanium oxide technique at the Sudbury Neutrino Observatory

NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT 604:3 (2009) 531-535

Authors:

B Aharmim, BT Cleveland, X Dai, G Doucas, J Farine, H Fergani, R Ford, RL Hahn, ED Hallman, NA Jelley, R Lange, S Majerus, C Mifflin, AJ Noble, HM O'Keeffe, R Rodriguez-Jimenez, D Sinclair, M Yeh

Determination of the ν_e and total ⁸B solar neutrino fluxes using the Sudbury Neutrino Observatory Phase I data set

PHYSICAL REVIEW C 75:4 (2007) ARTN 045502

Authors:

B Aharmim, QR Ahmad, SN Ahmed, RC Allen, TC Andersen, JD Anglin, G Buehler, JC Barton, EW Beier, M Bercovitch, M Bergevin, J Bigu, SD Biller, RA Black, I Blevis, RJ Boardman, J Boger, E Bonvin, MG Boulay, MG Bowler, TJ Bowles, SJ Brice, MC Browne, TV Bullard, TH Burritt, J Cameron, YD Chan, HH Chen, M Chen, X Chen, BT Cleveland, JHM Cowan, DF Cowen, GA Cox, CA Currat, X Dai, F Dalnoki-Veress, WF Davidson, H Deng, M DiMarco, PJ Doe, G Doucas, MR Dragowsky, CA Duba, FA Duncan, M Dunford, JA Dunmore, ED Earle, SR Elliott, HC Evans, GT Ewan, J Farine, H Fergani, AP Ferraris, F Fleurot, RJ Ford, JA Formaggio, MM Fowler, K Frame, ED Frank, W Frati, N Gagnon, JV Germani, S Gil, A Goldschmidt, JTM Goon, K Graham, DR Grant, E Guillian, RL Hahn, AL Hallin, ED Hallman, AS Hamer, AA Hamian, WB Handler, RU Haq, CK Hargrove, PJ Harvey, R Hazama, KM Heeger, WJ Heintzelman, J Heise, RL Helmer, R Henning, JD Hepburn, H Heron, J Hewett, A Hime, C Howard, MA Howe, M Huang, JG Hykaway, MCP Isaac, P Jagam, B Jamieson, NA Jelley, C Jillings, G Jonkmans, K Kazkaz, PT Keener, K Kirch, JR Klein, AB Knox, RJ Komar, LL Kormos, M Kos, R Kouzes, A Krueger, C Kraus, CB Krauss, T Kutter, CCM Kyba, H Labranche, R Lange, J Law, IT Lawson, M Lay, HW Lee, KT Lesko, JR Leslie, I Levine, JC Loach, W Locke, S Luoma, J Lyon, R MacLellan, S Majerus, HB Mak, J Maneira, AD Marino, R Martin, N McCauley, AB McDonald, DS McDonald, K McFarlane, S McGee, G McGregor, R Meijer Drees, H Mes, C Mifflin, KKS Miknaitis, ML Miller, G Milton, BA Moffat, B Monreal, M Moorhead, B Morrissette, CW Nally, MS Neubauer, FM Newcomer, HS Ng, BG Nickel, AJ Noble, EB Norman, VM Novikov, NS Oblath, CE Okada, HM O'Keeffe, RW Ollerhead, M Omori, JL Orrell, SM Oser, R Ott, SJM Peeters, AWP Poon, G Prior, SD Reitzner, K Rielage, A Roberge, BC Robertson, RGH Robertson, SSE Rosendahl, JK Rowley, VL Rusu, E Saettler, A Schulke, MH Schwendener, JA Secrest, H Seifert, M Shatkay, JJ Simpson, CJ Sims, D Sinclair, P Skensved, AR Smith, MWE Smith, N Starinsky, TD Steiger, RG Stokstad, LC Stonehill, RS Storey, B Sur, R Tafirout, N Tagg, Y Takeuchi, NW Tanner, RK Taplin, M Thorman, PM Thornewell, N Tolich, PT Trent, YI Tserkovnyak, T Tsui, CD Tunnell, R Van Berg, RG Van De Water, CJ Virtue, TJ Walker, BL Wall, CE Waltham, H Wan Chan Tseung, J-X Wang, DL Wark, J Wendland, N West, JB Wilhelmy, JF Wilkerson, JR Wilson, P Wittich, JM Wouters, A Wright, M Yeh, K Zuber

A search for neutrinos from the solar hep reaction and the diffuse supernova neutrino background with the Sudbury Neutrino Observatory

ASTROPHYSICAL JOURNAL 653:2 (2006) 1545-1551

Authors:

B Aharmim, SN Ahmed, AE Anthony, EW Beier, A Bellerive, M Bergevin, SD Biller, MG Boulay, YD Chan, M Chen, X Chen, BT Cleveland, GA Cox, CA Currat, X Dai, F Dalnoki-Veress, H Deng, J Detwiler, M DiMarco, PJ Doe, G Doucas, P-L Drouin, FA Duncan, M Dunford, JA Dunmore, ED Earle, HC Evans, GT Ewan, J Farine, H Fergani, F Fleurot, RJ Ford, JA Formaggio, N Gagnon, J Tm Goon, K Graham, E Guillian, RL Hahn, AL Hallin, ED Hallman, PJ Harvey, R Hazama, KM Heeger, WJ Heintzelman, J Heise, RL Helmer, RJ Hemingway, R Henning, A Hime, C Howard, MA Howe, M Huang, P Jagam, NA Jelley, JR Klein, LL Kormos, M Kos, A Kruger, C Kraus, CB Krauss, T Kutter, CCM Kyba, H Labranche, R Lange, J Law, IT Lawson, KT Lesko, JR Leslie, JC Loach, S Luoma, R MacLellan, S Majerus, HB Mak, J Maneira, AD Marino, R Martin, N McCauley, AB McDonald, S McGee, C Mifflin, KKS Miknaitis, ML Miller, B Monreal, BG Nickel, AJ Noble, EB Norman, NS Oblath, CE Okada, HM O'Keeffe, GD Orebi Gann, SM Oser, R Ott, SJM Peeters, AWP Poon, G Prior, K Rielage, BC Robertson, RGH Robertson, E Rollin, MH Schwendener, JA Secrest, SR Seibert, O Simard, CJ Sims, D Sinclair, P Skensved, RG Stokstad, LC Stonehill, G Tesic, N Tolich, T Tsui, R Van Berg, RG Van de Water, BA VanDevender, CJ Virtue, TJ Walker, BL Wall, D Waller, H Wan Chan Tseung, DL Wark, J Wendland, N West, JF Wilkerson, JR Wilson, JM Wouters, A Wright, M Yeh, F Zhang, K Zuber

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Nick Jelley

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The calibration of the Sudbury Neutrino Observatory using uniformly distributed radioactive sources

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Abstract:

The Sudbury Neutrino Observatory

Authors:

Abstract:

High sensitivity measurement of ²²⁴Ra and ²²⁶Ra in water with an improved hydrous titanium oxide technique at the Sudbury Neutrino Observatory

Authors:

Determination of the ν_e and total ⁸B solar neutrino fluxes using the Sudbury Neutrino Observatory Phase I data set

Authors:

A search for neutrinos from the solar hep reaction and the diffuse supernova neutrino background with the Sudbury Neutrino Observatory

Authors:

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Nick Jelley

Sub department

The calibration of the Sudbury Neutrino Observatory using uniformly distributed radioactive sources

Authors:

Abstract:

The Sudbury Neutrino Observatory

Authors:

Abstract:

High sensitivity measurement of 224Ra and 226Ra in water with an improved hydrous titanium oxide technique at the Sudbury Neutrino Observatory

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Determination of the νe and total 8B solar neutrino fluxes using the Sudbury Neutrino Observatory Phase I data set

Authors:

A search for neutrinos from the solar hep reaction and the diffuse supernova neutrino background with the Sudbury Neutrino Observatory

Authors:

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High sensitivity measurement of ²²⁴Ra and ²²⁶Ra in water with an improved hydrous titanium oxide technique at the Sudbury Neutrino Observatory

Determination of the ν_e and total ⁸B solar neutrino fluxes using the Sudbury Neutrino Observatory Phase I data set