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Bullet cluster image
Credit: Credit: X-ray: NASA/CXC/CfA/M.Markevitch et al.; Optical: NASA/STScI; Magellan/U.Arizona/D.Clowe et al.; Lensing Map: NASA/STScI

Professor Jocelyn Monroe

Professor of Particle Physics

Research theme

  • Particle astrophysics & cosmology

Sub department

  • Particle Physics
jocelyn.monroe@physics.ox.ac.uk
Telephone: 273317
en.wikipedia.org/wiki/Jocelyn_Monroe
  • About
  • Publications

The MiniBooNE detector

Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment Elsevier 599:1 (2009) 28-46

Authors:

AA Aguilar-Arevalo, CE Anderson, LM Bartoszek, AO Bazarko, SJ Brice, BC Brown, L Bugel, J Cao, L Coney, JM Conrad, DC Cox, A Curioni, Z Djurcic, DA Finley, BT Fleming, R Ford, FG Garcia, GT Garvey, C Green, JA Green, TL Hart, E Hawker, R Imlay, RA Johnson, G Karagiorgi, P Kasper, T Katori, T Kobilarcik, I Kourbanis, S Koutsoliotas, EM Laird, SK Linden, JM Link, Y Liu, Y Liu, WC Louis, KBM Mahn, W Marsh, PS Martin, G McGregor, W Metcalf, H-O Meyer, PD Meyers, F Mills, GB Mills, J Monroe, CD Moore, RH Nelson, VT Nguyen, P Nienaber, JA Nowak, S Ouedraogo, RB Patterson, D Perevalov, CC Polly, E Prebys, JL Raaf, H Ray, BP Roe, AD Russell, V Sandberg, W Sands, R Schirato, G Schofield, D Schmitz, MH Shaevitz, FC Shoemaker, D Smith, M Soderberg, M Sorel, P Spentzouris, I Stancu, RJ Stefanski, M Sung, HA Tanaka, R Tayloe, M Tzanov, R Van de Water, MO Wascko, DH White, MJ Wilking, HJ Yang, GP Zeller, ED Zimmerman, The MiniBooNE Collaboration
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The DMTPC detector

Proceedings of Science (2008)

Authors:

G Sciolla, J Battat, T Caldwell, B Cornell, D Dujmic, P Fisher, S Henderson, R Lanza, A Lee, J Lopez, A Kaboth, G Kohse, J Monroe, T Sahin, R Vanderspek, R Yamamoto, H Yegoryan, S Ahlen, D Avery, K Otis, A Roccaro, H Tomita, A Dushkin, H Wellenstein

Abstract:

Directional Dark Matter detectors have the potential of yielding an unambiguous observation of WIMPs even in presence of insidious background. In addition, by measuring the direction of the Dark Matter particles such detectors can discriminate between the various models that describe Dark Matter in our galaxy. The DMTPC detector is a novel directional DM detector consisting of a low-pressure CF4 time projection chamber with optical readout. Recent measurements proved that this technology is able to reconstruct the energy, direction, and sense of the low-energy nuclear recoils produced by neutrons from a 252Cf source, as well as efficiently reject electromagnetic backgrounds. A 10-liter DMTPC detector is ready for underground operation. A 1 m3 detector, now in the design phase, will soon allow us to improve the existing limits of SD-interactions of WIMPs on protons by over one order of magnitude.

Independent Measurement of the Total Active B8 Solar Neutrino Flux Using an Array of He3 Proportional Counters at the Sudbury Neutrino Observatory

Physical Review Letters American Physical Society (APS) 101:11 (2008) 111301

Authors:

B Aharmim, SN Ahmed, JF Amsbaugh, AE Anthony, J Banar, N Barros, EW Beier, A Bellerive, B Beltran, M Bergevin, SD Biller, K Boudjemline, MG Boulay, TJ Bowles, MC Browne, TV Bullard, TH Burritt, B Cai, YD Chan, D Chauhan, M Chen, BT Cleveland, GA Cox-Mobrand, CA Currat, X Dai, H Deng, J Detwiler, M DiMarco, PJ Doe, G Doucas, P-L Drouin, CA Duba, FA Duncan, M Dunford, ED Earle, SR Elliott, HC Evans, GT Ewan, J Farine, H Fergani, F Fleurot, RJ Ford, JA Formaggio, MM Fowler, N Gagnon, JV Germani, A Goldschmidt, JTM Goon, K Graham, E Guillian, S Habib, RL Hahn, AL Hallin, ED Hallman, AA Hamian, GC Harper, PJ Harvey, R Hazama, KM Heeger, WJ Heintzelman, J Heise, RL Helmer, R Henning, A Hime, C Howard, MA Howe, M Huang, P Jagam, B Jamieson, NA Jelley, KJ Keeter, JR Klein, LL Kormos, M Kos, A Krüger, C Kraus, CB Krauss, T Kutter, CCM Kyba, R Lange, J Law, IT Lawson, KT Lesko, JR Leslie, JC Loach, R MacLellan, S Majerus, HB Mak, J Maneira, R Martin, K McBryde, N McCauley, AB McDonald, S McGee, C Mifflin, GG Miller, ML Miller, B Monreal, J Monroe, B Morissette, A Myers, BG Nickel, AJ Noble, NS Oblath, HM O’Keeffe, RW Ollerhead, GD Orebi Gann, SM Oser, RA Ott, SJM Peeters, AWP Poon, G Prior, SD Reitzner, K Rielage, BC Robertson, RGH Robertson, E Rollin, MH Schwendener, JA Secrest, SR Seibert, O Simard, JJ Simpson, L Sinclair, P Skensved, MWE Smith, TD Steiger, LC Stonehill, G Tešić, PM Thornewell, N Tolich, T Tsui, CD Tunnell, T Van Wechel, R Van Berg, BA VanDevender, CJ Virtue, TJ Walker, BL Wall, D Waller, H Wan Chan Tseung, J Wendland, N West, JB Wilhelmy, JF Wilkerson, JR Wilson, JM Wouters, A Wright, M Yeh, F Zhang, K Zuber
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Charge amplification concepts for direction-sensitive dark matter detectors

Astroparticle Physics 30:2 (2008) 58-64

Authors:

D Dujmic, P Fisher, G Sciolla, S Ahlen, V Dutta, S Henderson, A Kaboth, G Kohse, R Lanza, J Monroe, A Roccaro, N Skvorodnev, H Tomita, R Vanderspek, H Wellenstein, R Yamamoto

Abstract:

Direction measurement of weakly interacting massive particles in time-projection chambers can provide definite evidence of their existence and help to determine their properties. This article demonstrates several concepts for charge amplification in time-projection chambers that can be used in direction-sensitive dark matter search experiments. We demonstrate reconstruction of the "head-tail" effect for nuclear recoils above 100 keV, and discuss the detector performance in the context of dark matter detection and scaling to large detector volumes. © 2008 Elsevier B.V. All rights reserved.
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Maximum patch method for directional dark matter detection

Physical Review D Particles Fields Gravitation and Cosmology 78:1 (2008)

Authors:

S Henderson, J Monroe, P Fisher

Abstract:

Present and planned dark matter detection experiments search for WIMP-induced nuclear recoils in poorly known background conditions. In this environment, the maximum gap statistical method provides a way of setting more sensitive cross section upper limits by incorporating known signal information. We give a recipe for the numerical calculation of upper limits for planned directional dark matter detection experiments, that will measure both recoil energy and angle, based on the gaps between events in two-dimensional phase space. © 2008 The American Physical Society.
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