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Insertion of STC into TRT at the Department of Physics, Oxford
Credit: CERN

Amy Cottle

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Sub department

  • Particle Physics

Research groups

  • LUX-ZEPLIN
amy.cottle@physics.ox.ac.uk
Telephone: 01865 (2)73459
Denys Wilkinson Building, room 504A
  • About
  • Publications

The LUX-ZEPLIN (LZ) experiment

Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment Elsevier 953 (2019) 163047

Authors:

DS Akerib, CW Akerlof, D Yu Akimov, Kathryn Boast, Amy Cottle, T Fruth, E Gibson, Hans Kraus, Andrew Stevens, Matthew Tan,

Abstract:

We describe the design and assembly of the LUX-ZEPLIN experiment, a direct detection search for cosmic WIMP dark matter particles. The centerpiece of the experiment is a large liquid xenon time projection chamber sensitive to low energy nuclear recoils. Rejection of backgrounds is enhanced by a Xe skin veto detector and by a liquid scintillator Outer Detector loaded with gadolinium for efficient neutron capture and tagging. LZ is located in the Davis Cavern at the 4850’ level of the Sanford Underground Research Facility in Lead, South Dakota, USA. We describe the major subsystems of the experiment and its key design features and requirements.
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Measurement of the gamma ray background in the Davis cavern at the Sanford Underground Research Facility

Astroparticle Physics Elsevier 116:March 2020 (2019) 102391

Authors:

Ds Akerib, Cw Akerlof, Sk Alsum, Ke Boast, C Carels, A Cottle, T Fruth

Abstract:

Deep underground environments are ideal for low background searches due to the attenuation of cosmic rays by passage through the earth. However, they are affected by backgrounds from γ-rays emitted by 40K and the 238U and 232Th decay chains in the surrounding rock. The LUX-ZEPLIN (LZ) experiment will search for dark matter particle interactions with a liquid xenon TPC located within the Davis campus at the Sanford Underground Research Facility, Lead, South Dakota, at the 4850-foot level. In order to characterise the cavern background, in-situ γ-ray measurements were taken with a sodium iodide detector in various locations and with lead shielding. The integral count rates (0–3300 keV) varied from 596 Hz to 1355 Hz for unshielded measurements, corresponding to a total flux from the cavern walls of 1.9 ± 0.4 γ cm−2s−1. The resulting activity in the walls of the cavern can be characterised as 220 ± 60 Bq/kg of 40K, 29 ± 15 Bq/kg of 238U, and 13 ± 3 Bq/kg of 232Th.
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Identification of radiopure titanium for the LZ dark matter experiment and future rare event searches

Astroparticle Physics Elsevier 96 (2017) 1-10

Authors:

DS Akerib, CW Akerlof, D Yu Akimov, SK Alsum, HM Araújo, IJ Arnquist, M Arthurs, X Bai, AJ Bailey, J Balajthy, S Balashov, MJ Barry, J Belle, P Beltrame, T Benson, EP Bernard, A Bernstein, TP Biesiadzinski, KE Boast, A Bolozdynya, B Boxer, R Bramante, P Brás, JH Buckley, VV Bugaev, R Bunker, S Burdin, JK Busenitz, C Carels, DL Carlsmith, B Carlson, MC Carmona-Benitez, C Chan, JJ Cherwinka, AA Chiller, C Chiller, A Cottle, R Coughlen, WW Craddock, A Currie, CE Dahl, TJR Davison, A Dobi, JEY Dobson, E Druszkiewicz, TK Edberg, WR Edwards, WT Emmet, CH Faham, S Fiorucci, T Fruth, RJ Gaitskell, NJ Gantos, VM Gehman, RM Gerhard, C Ghag, MGD Gilchriese, B Gomber, CR Hall, S Hans, K Hanzel, SJ Haselschwardt, SA Hertel, S Hillbrand, C Hjemfelt, MD Hoff, B Holbrook, E Holtom, EW Hoppe, JY-K Hor, M Horn, DQ Huang, TW Hurteau, CM Ignarra, RG Jacobsen, W Ji, A Kaboth, K Kamdin, K Kazkaz, D Khaitan, A Khazov, AV Khromov, AM Konovalov, EV Korolkova, M Koyuncu, H Kraus, HJ Krebs, VA Kudryavtsev, AV Kumpan, S Kyre, C Lee, HS Lee, J Lee, DS Leonard, R Leonard, KT Lesko, C Levy, F-T Liao, J Lin, A Lindote, RE Linehan, WH Lippincott, X Liu, MI Lopes, B Lopez Paredes, W Lorenzon, S Luitz, P Majewski, A Manalaysay, L Manenti, RL Mannino, DJ Markley, TJ Martin, MF Marzioni, CT McConnell, DN McKinsey, D-M Mei, Y Meng, EH Miller, E Mizrachi, J Mock, ME Monzani, JA Morad, BJ Mount, Murphy, C Nehrkorn, HN Nelson, F Neves, JA Nikkel, J O’Dell, K O’Sullivan, I Olcina, MA Olevitch, KC Oliver-Mallory, KJ Palladino, EK Pease, A Piepke, S Powell, RM Preece, K Pushkin, BN Ratcliff, J Reichenbacher, L Reichhart, CA Rhyne, A Richards, JP Rodrigues, HJ Rose, R Rosero, P Rossiter, JS Saba, M Sarychev, RW Schnee, M Schubnell, PR Scovell, S Shaw, TA Shutt, C Silva, K Skarpaas, W Skulski, M Solmaz, VN Solovov, P Sorensen, VV Sosnovtsev, I Stancu, MR Stark, S Stephenson, TM Stiegler, K Stifter, TJ Sumner, M Szydagis, DJ Taylor, WC Taylor, D Temples, PA Terman, KJ Thomas, JA Thomson, DR Tiedt, M Timalsina, WH To, A Tomás, TE Tope, M Tripathi, L Tvrznikova, J Va’vra, A Vacheret, MGD van der Grinten, JR Verbus, CO Vuosalo, WL Waldron, R Wang, R Watson, RC Webb, W-Z Wei, M While, DT White, TJ Whitis, WJ Wisniewski, MS Witherell, FLH Wolfs, D Woodward, S Worm, J Xu, M Yeh, J Yin, C Zhang, Collaboration)
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LUX-ZEPLIN (LZ) Technical Design Report

(2017)

Authors:

BJ Mount, S Hans, R Rosero, M Yeh, C Chan, RJ Gaitskell, DQ Huang, J Makkinje, DC Malling, M Pangilinan, CA Rhyne, WC Taylor, JR Verbus, YD Kim, HS Lee, J Lee, DS Leonard, J Li, J Belle, A Cottle, WH Lippincott, DJ Markley, TJ Martin, M Sarychev, TE Tope, M Utes, R Wang, I Young, HM Araújo, AJ Bailey, D Bauer, D Colling, A Currie, S Fayer, F Froborg, S Greenwood, WG Jones, V Kasey, M Khaleeq, I Olcina, B López Paredes, A Richards, TJ Sumner, A Tomás, A Vacheret, P Brás, A Lindote, MI Lopes, F Neves, JP Rodrigues, C Silva, VN Solovov, MJ Barry, A Cole, A Dobi, WR Edwards, CH Faham, S Fiorucci, NJ Gantos, VM Gehman, MGD Gilchriese, K Hanzel, MD Hoff, K Kamdin, KT Lesko, CT McConnell, K O'Sullivan, KC Oliver-Mallory, SJ Patton, JS Saba, P Sorensen, KJ Thomas, CE Tull, WL Waldron, MS Witherell, A Bernstein, K Kazkaz, J Xu, D Yu Akimov, AI Bolozdynya, AV Khromov, AM Konovalov, AV Kumpan, VV Sosnovtsev, CE Dahl, D Temples, MC Carmona-Benitez, L de Viveiros, DS Akerib, H Auyeung, TP Biesiadzinski, M Breidenbach, R Bramante, R Conley, WW Craddock, A Fan, A Hau, CM Ignarra, W Ji, HJ Krebs, R Linehan, C Lee, S Luitz, E Mizrachi, ME Monzani, FG O'Neill, S Pierson, M Racine, BN Ratcliff, GW Shutt, TA Shutt, K Skarpaas, K Stifter, WH To, J Va'vra, TJ Whitis, WJ Wisniewski, X Bai, R Bunker, R Coughlen, C Hjemfelt, R Leonard, EH Miller, E Morrison, J Reichenbacher, RW Schnee, MR Stark, K Sundarnath, DR Tiedt, M Timalsina, P Bauer, B Carlson, M Horn, M Johnson, J Keefner, C Maupin, DJ Taylor, S Balashov, P Ford, V Francis, E Holtom, A Khazov, A Kaboth, P Majewski, JA Nikkel, J O'Dell, RM Preece, MGD van der Grinten, SD Worm, RL Mannino, TM Stiegler, PA Terman, RC Webb, C Levy, J Mock, M Szydagis, JK Busenitz, M Elnimr, JY-K Hor, Y Meng, A Piepke, I Stancu, L Kreczko, B Krikler, B Penning, EP Bernard, RG Jacobsen, DN McKinsey, R Watson, JE Cutter, S El-Jurf, RM Gerhard, D Hemer, S Hillbrand, B Holbrook, BG Lenardo, AG Manalaysay, JA Morad, S Stephenson, JA Thomson, M Tripathi, S Uvarov, SJ Haselschwardt, S Kyre, C Nehrkorn, HN Nelson, M Solmaz, DT White, M Cascella, JEY Dobson, C Ghag, X Liu, L Manenti, L Reichhart, S Shaw, U Utku, P Beltrame, TJR Davison, MF Marzioni, A St J Murphy, A Nilima, B Boxer, S Burdin, A Greenall, S Powell, HJ Rose, P Sutcliffe, J Balajthy, TK Edberg, CR Hall, JS Silk, S Hertel, CW Akerlof, M Arthurs, W Lorenzon, K Pushkin, M Schubnell, KE Boast, C Carels, T Fruth, H Kraus, F-T Liao, J Lin, PR Scovell, E Druszkiewicz, D Khaitan, M Koyuncu, W Skulski, FLH Wolfs, J Yin, EV Korolkova, VA Kudryavtsev, P Rossiter, D Woodward, AA Chiller, C Chiller, D-M Mei, L Wang, W-Z Wei, M While, C Zhang, SK Alsum, T Benson, DL Carlsmith, JJ Cherwinka, S Dasu, G Gregerson, B Gomber, A Pagac, KJ Palladino, CO Vuosalo, Q Xiao, JH Buckley, VV Bugaev, MA Olevitch, EM Boulton, WT Emmet, TW Hurteau, NA Larsen, EK Pease, BP Tennyson, L Tvrznikova
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A SQUID magnetometry system for a cryogenic neutron electric dipole moment experiment

Nuclear Instruments and Methods in Physics Research Section A Elsevier 763 (2014) 483-494

Authors:

Samuel Henry, C Clarke, A Cottle, A Lynch, M Pipe

Abstract:

Precision magnetometry is an essential component of any neutron electric dipole moment experiment in order to correct shifts in the neutron precession frequency due to changes in the magnetic field. We have developed a magnetometry system using 12 SQUID sensors, designed to operate in 0.5 K superfluid helium. The pick-up loops located near the neutron cell are connected to the SQUID sensors by ~2 m twisted wire pairs. The SQUID readout cables are run via an intermediate stage at 4.2 K. The system has been installed and tested in the cryoEDM apparatus at the ILL, Grenoble, and used to characterise the magnetic environment. Further tests in a suitable low noise environment confirm it meets our requirements.
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