LUX-ZEPLIN

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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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Measurement of the cosmogenic activation of germanium detectors in EDELWEISS-III

Astroparticle Physics Elsevier 91 (2017) 51-64

Authors:

E Armengaud, Q Arnaud, C Augier, Hans Kraus

Abstract:

We present a measurement of the cosmogenic activation in the cryogenic germanium detectors of the EDELWEISS III direct dark matter search experiment. The decay rates measured in detectors with different exposures to cosmic rays above ground are converted into production rates of different isotopes. The measured production rates in units of nuclei/kg/day are 82 ± 21 for 3H, 2.8 ± 0.6 for 49V, 4.6 ± 0.7 for 55Fe, and 106 ± 13 for 65Zn. These results are the most accurate for these isotopes. A 90% C.L. lower limit on the production rate of 68Ge of 71 nuclei/kg/day is also presented. They are compared to model predictions present in literature and to estimates calculated with the ACTIVIA code.
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Non-contact luminescence lifetime cryothermometry for macromolecular crystallography

(2017)

Authors:

V Mykhaylyk A Wagner, H Kraus
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A tool to convert CAD models for importation into Geant4

(2017)

Authors:

Carl Vuosalo, Duncan Carlsmith, Sridhara Dasu, Kimberly Palladino
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Identification of Radiopure Titanium for the LZ Dark Matter Experiment and Future Rare Event Searches

(2017)

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, A St J 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
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