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91̽»¨
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
  • About
  • Publications

Measurement of neutrino-induced charged-current charged pion production cross sections on mineral oil at Eν∼1 GeV

Physical Review D American Physical Society (APS) 83:5 (2011) 052007

Authors:

AA Aguilar-Arevalo, CE Anderson, AO Bazarko, SJ Brice, BC Brown, L Bugel, J Cao, L Coney, JM Conrad, DC Cox, A Curioni, R Dharmapalan, Z Djurcic, DA Finley, BT Fleming, R Ford, FG Garcia, GT Garvey, J Grange, 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, C Mauger, VT McGary, G McGregor, W Metcalf, PD Meyers, F Mills, GB Mills, J Monroe, CD Moore, J Mousseau, RH Nelson, P Nienaber, JA Nowak, B Osmanov, S Ouedraogo, RB Patterson, Z Pavlovic, D Perevalov, CC Polly, E Prebys, JL Raaf, H Ray, BP Roe, AD Russell, V Sandberg, R Schirato, D Schmitz, MH Shaevitz, FC Shoemaker, D Smith, M Soderberg, M Sorel, P Spentzouris, J Spitz, 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

Measurement of νμ-induced charged-current neutral pion production cross sections on mineral oil at Eν∈0.5–2.0 GeV

Physical Review D American Physical Society (APS) 83:5 (2011) 052009

Authors:

AA Aguilar-Arevalo, CE Anderson, AO Bazarko, SJ Brice, BC Brown, L Bugel, J Cao, L Coney, JM Conrad, DC Cox, A Curioni, R Dharmapalan, Z Djurcic, DA Finley, BT Fleming, R Ford, FG Garcia, GT Garvey, J Grange, 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, C Mauger, VT McGary, G McGregor, W Metcalf, PD Meyers, F Mills, GB Mills, J Monroe, CD Moore, J Mousseau, RH Nelson, P Nienaber, JA Nowak, B Osmanov, S Ouedraogo, RB Patterson, Z Pavlovic, D Perevalov, CC Polly, E Prebys, JL Raaf, H Ray, BP Roe, AD Russell, V Sandberg, R Schirato, D Schmitz, MH Shaevitz, FC Shoemaker, D Smith, M Soderberg, M Sorel, P Spentzouris, J Spitz, I Stancu, RJ Stefanski, M Sung, HA Tanaka, R Tayloe, M Tzanov, RG Van de Water, MO Wascko, DH White, MJ Wilking, HJ Yang, GP Zeller, ED Zimmerman

LOW-MULTIPLICITY BURST SEARCH AT THE SUDBURY NEUTRINO OBSERVATORY

The Astrophysical Journal American Astronomical Society 728:2 (2011) 83

Authors:

B Aharmim, SN Ahmed, AE Anthony, N Barros, EW Beier, A Bellerive, B Beltran, M Bergevin, SD Biller, K Boudjemline, MG Boulay, B Cai, YD Chan, D Chauhan, M Chen, BT Cleveland, X Dai, H Deng, J Detwiler, G Doucas, P-L Drouin, FA Duncan, M Dunford, ED Earle, SR Elliott, HC Evans, GT Ewan, J Farine, H Fergani, F Fleurot, RJ Ford, JA Formaggio, N Gagnon, JTM Goon, K Graham, E Guillian, S Habib, RL Hahn, AL Hallin, ED Hallman, PJ Harvey, R Hazama, WJ Heintzelman, J Heise, RL Helmer, A Hime, C Howard, M Huang, B Jamieson, NA Jelley, M Jerkins, JR Klein, M Kos, C Kraus, CB Krauss, T Kutter, CCM Kyba, J Law, KT Lesko, JR Leslie, JC Loach, R MacLellan, S Majerus, HB Mak, J Maneira, R Martin, N McCauley, AB McDonald, ML Miller, B Monreal, J Monroe, BG Nickel, AJ Noble, HM O'Keeffe, NS Oblath, GD Orebi Gann, SM Oser, RA Ott, SJM Peeters, AWP Poon, G Prior, SD Reitzner, K Rielage, BC Robertson, RGH Robertson, MH Schwendener, JA Secrest, SR Seibert, O Simard, JJ Simpson, D Sinclair, P Skensved, TJ Sonley, LC Stonehill, G Tešić, N Tolich, T Tsui, R Van Berg, BA VanDevender, CJ Virtue, H Wan Chan Tseung, PJS Watson, N West, JF Wilkerson, JR Wilson, A Wright, M Yeh, F Zhang, and K Zuber

First dark matter search results from a surface run of the 10-L DMTPC directional dark matter detector

Physics Letters Section B Nuclear Elementary Particle and High Energy Physics 695:1-4 (2011) 124-129

Authors:

S Ahlen, JBR Battat, T Caldwell, C Deaconu, D Dujmic, W Fedus, P Fisher, F Golub, S Henderson, A Inglis, A Kaboth, G Kohse, R Lanza, A Lee, J Lopez, J Monroe, T Sahin, G Sciolla, N Skvorodnev, H Tomita, H Wellenstein, I Wolfe, R Yamamoto, H Yegoryan

Abstract:

The Dark Matter Time Projection Chamber (DMTPC) is a low pressure (75 Torr CF4) 10 liter detector capable of measuring the vector direction of nuclear recoils with the goal of directional dark matter detection. In this Letter we present the first dark matter limit from DMTPC from a surface run at MIT. In an analysis window of 80-200 keV recoil energy, based on a 35.7 g-day exposure, we set a 90% C.L. upper limit on the spin-dependent WIMP-proton cross section of 2.0×10-33 cm2 for 115 GeV/c2 dark matter particle mass. © 2010 Elsevier B.V.

Background rejection in the DMTPC dark matter search using charge signals

Proceedings of the 2011 Meeting of the Division of Particles and Fields of the American Physical Society Dpf 2011 (2011)

Authors:

JP Lopez, T Caldwell, C Deaconu, W Fedus, S Henderson, A Kaboth, A Lee, T Sahin, I Wolfe, R Yamamoto, H Yegoryan, S Ahlen, M Chernicoff, A Inglis, H Tomita, J Battat, D Dujmic, A Dushkin, F Golub, L Kirsch, H Ouyang, G Sciolla, N Skvorodnev, H Wellenstein, P Fisher, G Kohse, R Lanza, J Monroe

Abstract:

The Dark Matter Time Projection Chamber (DMTPC) collaboration is developing low-pressure gas TPC detectors for measuring WIMP-nucleon interactions. Optical readout with CCD cameras allows for the detection for the daily modulation in the direction of the dark matter wind, while several charge readout channels allow for the measurement of additional recoil properties. In this article, we show that the addition of the charge readout analysis to the CCD allows us too obtain a statistics-limited 90% C.L. upper limit on the e- rejection factor of 5.6 × 10-6 for recoils with energies between 40 and 200 keVee. In addition, requiring coincidence between charge signals and light in the CCD reduces CCD-specific backgrounds by more than two orders of magnitude.

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