51猎奇入口

Skip to main content
Department Of Physics text logo
  • Research
    • Our research
    • Our research groups
    • Our research in action
    • Research funding support
    • Summer internships for undergraduates
  • 51猎奇入口
    • Undergraduates
    • Postgraduates
  • Engage
    • For young people
    • For teachers
    • For the public
    • For alumni
    • For business
  • Support
Menu
Insertion of STC into TRT at the Department of Physics, Oxford
Credit: CERN

Amy Cottle

Visitor

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) radioactivity and cleanliness control programs

European Physical Journal C Springer Nature 80:11 (2020) 1044

Authors:

DS Akerib, CW Akerlof, D Yu Akimov, A Alquahtani, SK Alsum, TJ Anderson, N Angelides, HM Ara煤jo, A Arbuckle, JE Armstrong, M Arthurs, H Auyeung, S Aviles, X Bai, AJ Bailey, J Balajthy, S Balashov, J Bang, MJ Barry, D Bauer, P Bauer, A Baxter, J Belle, P Beltrame, J Bensinger, T Benson, EP Bernard, A Bernstein, A Bhatti, A Biekert, TP Biesiadzinski, HJ Birch, B Birrittella, KE Boast, AI Bolozdynya, EM Boulton, B Boxer, R Bramante, S Branson, P Br谩s, M Breidenbach, CAJ Brew, JH Buckley, VV Bugaev, R Bunker, S Burdin, JK Busenitz, R Cabrita, JS Campbell, C Carels, DL Carlsmith, B Carlson, MC Carmona-Benitez, M Cascella, C Chan, JJ Cherwinka, AA Chiller, C Chiller, NI Chott, A Cole, J Coleman, D Colling, RA Conley, A Cottle, R Coughlen, G Cox, WW Craddock, D Curran, A Currie, JE Cutter, JP da Cunha, CE Dahl, S Dardin, S Dasu, J Davis, TJR Davison, L de Viveiros, N Decheine, A Dobi, JEY Dobson, E Druszkiewicz, A Dushkin, TK Edberg, WR Edwards, BN Edwards, J Edwards, MM Elnimr, WT Emmet, SR Eriksen, CH Faham, A Fan, S Fayer, S Fiorucci, H Flaecher, IM Fogarty Florang, P Ford, VB Francis, ED Fraser, F Froborg, T Fruth, RJ Gaitskell, NJ Gantos, D Garcia, VM Gehman, R Gelfand, J Genovesi, RM Gerhard, C Ghag, E Gibson, MGD Gilchriese, S Gokhale, B Gomber, TG Gonda, A Greenall, S Greenwood, G Gregerson, MGD van der Grinten, CB Gwilliam, CR Hall, D Hamilton, S Hans, K Hanzel, T Harrington, A Harrison, J Harrison, C Hasselkus, SJ Haselschwardt, D Hemer, SA Hertel, J Heise, S Hillbrand, O Hitchcock, C Hjemfelt, MD Hoff, B Holbrook, E Holtom, JY-K Hor, M Horn, DQ Huang, TW Hurteau, CM Ignarra, MN Irving, RG Jacobsen, O Jahangir, SN Jeffery, W Ji, M Johnson, J Johnson, P Johnson, WG Jones, AC Kaboth, A Kamaha, K Kamdin, V Kasey, K Kazkaz, J Keefner, D Khaitan, M Khaleeq, A Khazov, AV Khromov, I Khurana, YD Kim, WT Kim, CD Kocher, D Kodroff, AM Konovalov, L Korley, EV Korolkova, M Koyuncu, J Kras, H Kraus, SW Kravitz, HJ Krebs, L Kreczko, B Krikler, VA Kudryavtsev, AV Kumpan, S Kyre, AR Lambert, B Landerud, NA Larsen, A Laundrie, EA Leason, HS Lee, J Lee, C Lee, BG Lenardo, DS Leonard, R Leonard, KT Lesko, C Levy, J Li, Y Liu, J Liao, F-T Liao, J Lin, A Lindote, R Linehan, WH Lippincott, R Liu, X Liu, C Loniewski, MI Lopes, E Lopez-Asamar, B L贸pez Paredes, W Lorenzon, D Lucero, S Luitz, JM Lyle, C Lynch, PA Majewski, J Makkinje, DC Malling, A Manalaysay, L Manenti, RL Mannino, N Marangou, DJ Markley, P MarrLaundrie, TJ Martin, MF Marzioni, C Maupin, CT McConnell, DN McKinsey, J McLaughlin, D-M Mei, Y Meng, EH Miller, ZJ Minaker, E Mizrachi, J Mock, D Molash, A Monte, ME Monzani, JA Morad, E Morrison, BJ Mount, A St J Murphy, D Naim, A Naylor, C Nedlik, C Nehrkorn, HN Nelson, J Nesbit, F Neves, JA Nikkel, JA Nikoleyczik, A Nilima, J O鈥橠ell, H Oh, FG O鈥橬eill, K O鈥橲ullivan, I Olcina, MA Olevitch, KC Oliver-Mallory, L Oxborough, A Pagac, D Pagenkopf, S Pal, KJ Palladino, VM Palmaccio, J Palmer, M Pangilinan, N Parveen, SJ Patton, EK Pease, BP Penning, G Pereira, C Pereira, IB Peterson, A Piepke, S Pierson, S Powell, RM Preece, K Pushkin, Y Qie, M Racine, BN Ratcliff, J Reichenbacher, L Reichhart, CA Rhyne, A Richards, Q Riffard, GRC Rischbieter, JP Rodrigues, HJ Rose, R Rosero, P Rossiter, R Rucinski, G Rutherford, JS Saba, L Sabarots, D Santone, M Sarychev, ABMR Sazzad, RW Schnee, M Schubnell, PR Scovell, M Severson, D Seymour, S Shaw, GW Shutt, TA Shutt, JJ Silk, C Silva, K Skarpaas, W Skulski, AR Smith, RJ Smith, RE Smith, J So, M Solmaz, VN Solovov, P Sorensen, VV Sosnovtsev, I Stancu, MR Stark, S Stephenson, N Stern, A Stevens, TM Stiegler, K Stifter, R Studley, TJ Sumner, K Sundarnath, P Sutcliffe, N Swanson, M Szydagis, M Tan, WC Taylor, R Taylor, DJ Taylor, D Temples, BP Tennyson, PA Terman, KJ Thomas, JA Thomson, DR Tiedt, M Timalsina, WH To, A Tom谩s, TE Tope, M Tripathi, DR Tronstad, CE Tull, W Turner, L Tvrznikova, M Utes, U Utku, S Uvarov, J Va鈥檝ra, A Vacheret, A Vaitkus, JR Verbus, T Vietanen, E Voirin, CO Vuosalo, S Walcott, WL Waldron, K Walker, JJ Wang, R Wang, L Wang, W Wang, Y Wang, JR Watson, J Migneault, S Weatherly, RC Webb, W-Z Wei, M While, RG White, JT White, DT White, TJ Whitis, WJ Wisniewski, K Wilson, MS Witherell, FLH Wolfs, JD Wolfs, D Woodward, SD Worm, X Xiang, Q Xiao, J Xu, M Yeh, J Yin, I Young, C Zhang, P Zarzhitsky

Projected sensitivity of the LUX-ZEPLIN experiment to the 0谓尾尾 decay of Xe136

Physical Review C American Physical Society (APS) 102:1 (2020) 014602

Authors:

DS Akerib, CW Akerlof, A Alqahtani, SK Alsum, TJ Anderson, N Angelides, HM Ara煤jo, JE Armstrong, M Arthurs, X Bai, J Balajthy, S Balashov, J Bang, A Baxter, J Bensinger, EP Bernard, A Bernstein, A Bhatti, A Biekert, TP Biesiadzinski, HJ Birch, KE Boast, B Boxer, P Br谩s, JH Buckley, VV Bugaev, S Burdin, JK Busenitz, R Cabrita, C Carels, DL Carlsmith, MC Carmona-Benitez, M Cascella, C Chan, NI Chott, A Cole, A Cottle, JE Cutter, CE Dahl, L de Viveiros, JEY Dobson, E Druszkiewicz, TK Edberg, SR Eriksen, A Fan, S Fiorucci, H Flaecher, ED Fraser, T Fruth, RJ Gaitskell, J Genovesi, C Ghag, E Gibson, MGD Gilchriese, S Gokhale, MGD van der Grinten, CR Hall, A Harrison, SJ Haselschwardt, SA Hertel, JY-K Hor, M Horn, DQ Huang, CM Ignarra, O Jahangir, W Ji, J Johnson, AC Kaboth, AC Kamaha, K Kamdin, K Kazkaz, D Khaitan, A Khazov, I Khurana, CD Kocher, L Korley, EV Korolkova, J Kras, H Kraus, S Kravitz, L Kreczko, B Krikler, VA Kudryavtsev, EA Leason, J Lee, DS Leonard, KT Lesko, C Levy, J Li, J Liao, F-T Liao, J Lin, A Lindote, R Linehan, WH Lippincott, R Liu, X Liu, C Loniewski, MI Lopes, B L贸pez Paredes, W Lorenzon, S Luitz, JM Lyle, PA Majewski, A Manalaysay, L Manenti, RL Mannino, N Marangou, MF Marzioni, DN McKinsey, J McLaughlin, Y Meng, EH Miller, E Mizrachi, A Monte, ME Monzani, JA Morad, E Morrison, BJ Mount, A St. J. Murphy, D Naim, A Naylor, C Nedlik, C Nehrkorn, HN Nelson, F Neves, JA Nikoleyczik, A Nilima, K O'Sullivan, I Olcina, KC Oliver-Mallory, S Pal, KJ Palladino, J Palmer, N Parveen, EK Pease, B Penning, G Pereira, K Pushkin, J Reichenbacher, CA Rhyne, Q Riffard, GRC Rischbieter, R Rosero, P Rossiter, G Rutherford, D Santone, ABMR Sazzad, RW Schnee, M Schubnell, D Seymour, S Shaw, TA Shutt, JJ Silk, C Silva, R Smith, M Solmaz, VN Solovov, P Sorensen, I Stancu, A Stevens, K Stifter, TJ Sumner, N Swanson, M Szydagis, M Tan, WC Taylor, R Taylor, DJ Temples, PA Terman, DR Tiedt, M Timalsina, A Tom谩s, M Tripathi, DR Tronstad, W Turner, L Tvrznikova, U Utku, A Vacheret, A Vaitkus, JJ Wang, W Wang, JR Watson, RC Webb, RG White, TJ Whitis, FLH Wolfs, D Woodward, X Xiang, J Xu, M Yeh, P Zarzhitsky

Simulations of events for the LUX-ZEPLIN (LZ) dark matter experiment

Astroparticle Physics Elseveir 125 (2020) 102480

Authors:

DS Akerib, CW Akerlof, A Alqahtani, Kathryn Boast, C Carels, A Cottle, T Fruth, E Gibson, H Kraus, F-T Liao, KJ Palladino, A Stevens, M Tan

Abstract:

The LUX-ZEPLIN dark matter search aims to achieve a sensitivity to the WIMP-nucleon spin-independent cross-section down to (1鈥�2) x 10鈥�12 pb at a WIMP mass of 40鈥� GeV/c2. This paper describes the simulations framework that, along with radioactivity measurements, was used to support this projection, and also to provide mock data for validating reconstruction and analysis software. Of particular note are the event generators, which allow us to model the background radiation, and the detector response physics used in the production of raw signals, which can be converted into digitized waveforms similar to data from the operational detector. Inclusion of the detector response allows us to process simulated data using the same analysis routines as developed to process the experimental data.

Projected WIMP sensitivity of the LUX-ZEPLIN dark matter experiment

Physical Review D American Physical Society (APS) 101:5 (2020) 052002

Authors:

DS Akerib, CW Akerlof, SK Alsum, HM Ara煤jo, M Arthurs, X Bai, AJ Bailey, J Balajthy, S Balashov, D Bauer, J Belle, P Beltrame, T Benson, EP Bernard, TP Biesiadzinski, KE Boast, B Boxer, P Br谩s, JH Buckley, VV Bugaev, S Burdin, JK Busenitz, C Carels, DL Carlsmith, B Carlson, MC Carmona-Benitez, C Chan, JJ Cherwinka, A Cole, A Cottle, WW Craddock, A Currie, JE Cutter, CE Dahl, L de Viveiros, A Dobi, JEY Dobson, E Druszkiewicz, TK Edberg, WR Edwards, A Fan, S Fayer, S Fiorucci, T Fruth, RJ Gaitskell, J Genovesi, C Ghag, MGD Gilchriese, MGD van der Grinten, CR Hall, S Hans, K Hanzel, SJ Haselschwardt, SA Hertel, S Hillbrand, C Hjemfelt, MD Hoff, JY-K Hor, DQ Huang, CM Ignarra, W Ji, AC Kaboth, K Kamdin, J Keefner, D Khaitan, A Khazov, YD Kim, CD Kocher, EV Korolkova, H Kraus, HJ Krebs, L Kreczko, B Krikler, VA Kudryavtsev, S Kyre, J Lee, BG Lenardo, DS Leonard, KT Lesko, C Levy, J Li, J Liao, F-T Liao, J Lin, A Lindote, R Linehan, WH Lippincott, X Liu, MI Lopes, B L贸pez Paredes, W Lorenzon, S Luitz, JM Lyle, P Majewski, A Manalaysay, RL Mannino, C Maupin, DN McKinsey, Y Meng, EH Miller, J Mock, ME Monzani, JA Morad, E Morrison, BJ Mount, A St. J. Murphy, HN Nelson, F Neves, J Nikoleyczik, K O鈥橲ullivan, I Olcina, MA Olevitch, KC Oliver-Mallory, KJ Palladino, SJ Patton, EK Pease, B Penning, A Piepke, S Powell, RM Preece, K Pushkin, BN Ratcliff, J Reichenbacher, CA Rhyne, A Richards, JP Rodrigues, R Rosero, P Rossiter, JS Saba, M Sarychev, RW Schnee, M Schubnell, PR Scovell, S Shaw, TA Shutt, JJ Silk, C Silva, K Skarpaas, W Skulski, M Solmaz, VN Solovov, P Sorensen, I Stancu, MR Stark, TM Stiegler, K Stifter, M Szydagis, WC Taylor, R Taylor, DJ Taylor, D Temples, PA Terman, KJ Thomas, M Timalsina, WH To, A Tom谩s, TE Tope, M Tripathi, CE Tull, L Tvrznikova, U Utku, J Va鈥檝ra, A Vacheret, JR Verbus, E Voirin, WL Waldron, JR Watson, RC Webb, DT White, TJ Whitis, WJ Wisniewski, MS Witherell, FLH Wolfs, D Woodward, SD Worm, M Yeh, J Yin, I Young

Simulations of Events for the LUX-ZEPLIN (LZ) Dark Matter Experiment

(2020)

Authors:

The LUX-ZEPLIN Collaboration, :, DS Akerib, CW Akerlof, A Alqahtani, SK Alsum, TJ Anderson, N Angelides, HM Ara煤jo, JE Armstrong, M Arthurs, X Bai, J Balajthy, S Balashov, J Bang, D Bauer, A Baxter, J Bensinger, EP Bernard, A Bernstein, A Bhatti, A Biekert, TP Biesiadzinski, HJ Birch, KE Boast, B Boxer, P Br谩s, JH Buckley, VV Bugaev, S Burdin, JK Busenitz, R Cabrita, C Carels, DL Carlsmith, MC Carmona-Benitez, M Cascella, C Chan, NI Chott, A Cole, A Cottle, JE Cutter, CE Dahl, L de Viveiros, JEY Dobson, E Druszkiewicz, TK Edberg, SR Eriksen, A Fan, S Fayer, S Fiorucci, H Flaecher, ED Fraser, T Fruth, RJ Gaitskell, J Genovesi, C Ghag, E Gibson, MGD Gilchriese, S Gokhale, MGD van der Grinten, CR Hall, A Harrison, SJ Haselschwardt, SA Hertel, JY-K Hor, M Horn, DQ Huang, CM Ignarra, O Jahangir, W Ji, J Johnson, AC Kaboth, AC Kamaha, K Kamdin, K Kazkaz, D Khaitan, A Khazov, I Khurana, CD Kocher, L Korley, EV Korolkova, J Kras, H Kraus, S Kravitz, L Kreczko, B Krikler, VA Kudryavtsev, EA Leason, J Lee, DS Leonard, KT Lesko, C Levy, J Li, J Liao, F-T Liao, J Lin, A Lindote, R Linehan, WH Lippincott, R Liu, X Liu, C Loniewski, MI Lopes, B L贸pez Paredes, W Lorenzon, S Luitz, JM Lyle, PA Majewski, A Manalaysay, L Manenti, RL Mannino, N Marangou, MF Marzioni, DN McKinsey, J McLaughlin, Y Meng, EH Miller, E Mizrachi, A Monte, ME Monzani, JA Morad, E Morrison, BJ Mount, A St J Murphy, D Naim, A Naylor, C Nedlik, C Nehrkorn, HN Nelson, F Neves, JA Nikoleyczik, A Nilima, I Olcina, KC Oliver-Mallory, S Pal, KJ Palladino, J Palmer, N Parveen, EK Pease, B Penning, G Pereira, A Piepke, K Pushkin, J Reichenbacher, CA Rhyne, A Richards, Q Riffard, GRC Rischbieter, R Rosero, P Rossiter, G Rutherford, D Santone, ABMR Sazzad, RW Schnee, M Schubnell, PR Scovell, D Seymour, S Shaw, TA Shutt, JJ Silk, C Silva, R Smith, M Solmaz, VN Solovov, P Sorensen, I Stancu, A Stevens, K Stifter, TJ Sumner, N Swanson, M Szydagis, M Tan, WC Taylor, R Taylor, DJ Temples, PA Terman, DR Tiedt, M Timalsina, A Tom谩s, M Tripathi, DR Tronstad, W Turner, L Tvrznikova, U Utku, A Vacheret, A Vaitkus, JJ Wang, W Wang, JR Watson, RC Webb, RG White, TJ Whitis, FLH Wolfs, D Woodward, X Xiang, J Xu, M Yeh, P Zarzhitsky

Pagination

  • First page First
  • Previous page Prev
  • …
  • Page 3
  • Page 4
  • Page 5
  • Page 6
  • Page 7
  • Page 8
  • Current page 9
  • Page 10
  • Page 11
  • Next page Next
  • Last page Last

Footer Menu

  • Contact us
  • Giving to the Dept of Physics
  • Work with us
  • Media

User account menu

  • Log in

Follow us

FIND US

Clarendon Laboratory,

Parks Road,

Oxford,

OX1 3PU

CONTACT US

Tel: +44(0)1865272200

Department Of Physics text logo

漏 University of Oxford - Department of Physics

Cookies | Privacy policy | Accessibility statement

  • Home
  • Research
  • 51猎奇入口
  • Engage
  • Our people
  • News & Comment
  • Events
  • Our facilities & services
  • 51猎奇入口
  • Giving to Physics