New limits on double electron capture of Ca-40 and W-180

JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS 43:9 (2016) ARTN 095202

Authors:

G Angloher, M Bauer, P Bauer, I Bavykina, A Bento, C Bucci, L Canonica, C Ciemniak, X Defay, G Deuter, A Erb, F von Feilitzsch, NF Iachellini, P Gorla, A Guetlein, D Hauff, P Huff, C Isaila, J Jochum, M Kiefer, M Kimmerle, H Kluck, H Kraus, J-C Lanfranchi, J Loebell, A Muenster, C Pagliarone, F Petricca, S Pfister, W Potzel, F Proebst, F Reindl, S Roth, K Rottler, C Sailer, K Schaffner, J Schieck, J Schmaler, S Scholl, S Schoenert, W Seidel, M von Sivers, L Stodolsky, C Strandhagen, R Strauss, A Tanzke, V Tretyak, HH Trinh Thi, C Tuerkoglu, M Uffinger, A Ulrich, I Usherov, S Wawoczny, M Willers, M Wuestrich, A Zoeller

Results from a search for dark matter in the complete LUX exposure

(2016)

Authors:

DS Akerib, S Alsum, HM Araújo, X Bai, AJ Bailey, J Balajthy, P Beltrame, EP Bernard, A Bernstein, TP Biesiadzinski, EM Boulton, R Bramante, P Brás, D Byram, SB Cahn, MC Carmona-Benitez, C Chan, AA Chiller, C Chiller, A Currie, JE Cutter, TJR Davison, A Dobi, JEY Dobson, E Druszkiewicz, BN Edwards, CH Faham, S Fiorucci, RJ Gaitskell, VM Gehman, C Ghag, KR Gibson, MGD Gilchriese, CR Hall, M Hanhardt, SJ Haselschwardt, SA Hertel, DP Hogan, M Horn, DQ Huang, CM Ignarra, M Ihm, RG Jacobsen, W Ji, K Kamdin, K Kazkaz, D Khaitan, R Knoche, NA Larsen, C Lee, BG Lenardo, KT Lesko, A Lindote, MI Lopes, A Manalaysay, RL Mannino, MF Marzioni, DN McKinsey, DM Mei, J Mock, M Moongweluwan, JA Morad, A St J Murphy, C Nehrkorn, HN Nelson, F Neves, K O`Sullivan, KC Oliver-Mallory, KJ Palladino, EK Pease, P Phelps, L Reichhart, C Rhyne, S Shaw, TA Shutt, C Silva, M Solmaz, VN Solovov, P Sorensen, S Stephenson, TJ Sumner, M Szydagis, DJ Taylor, WC Taylor, BP Tennyson, PA Terman, DR Tiedt, WH To, M Tripathi, L Tvrznikova, S Uvarov, JR Verbus, RC Webb, JT White, TJ Whitis, MS Witherell, FLH Wolfs, J Xu, K Yazdani, SK Young, C Zhang

Low-energy (0.7-74 keV) nuclear recoil calibration of the LUX dark matter experiment using D-D neutron scattering kinematics

ArXiv 1608.05381 (2016)

Authors:

LUX Collaboration, DS Akerib, S Alsum, HM Araújo, X Bai, AJ Bailey, J Balajthy, P Beltrame, EP Bernard, A Bernstein, TP Biesiadzinski, EM Boulton, A Bradley, R Bramante, P Brás, D Byram, SB Cahn, MC Carmona-Benitez, C Chan, JJ Chapman, AA Chiller, C Chiller, A Currie, JE Cutter, TJR Davison, L de Viveiros, A Dobi, JEY Dobson, E Druszkiewicz, BN Edwards, CH Faham, S Fiorucci, RJ Gaitskell, VM Gehman, C Ghag, KR Gibson, MGD Gilchriese, CR Hall, M Hanhardt, SJ Haselschwardt, SA Hertel, DP Hogan, M Horn, DQ Huang, CM Ignarra, M Ihm, RG Jacobsen, W Ji, K Kamdin, K Kazkaz, D Khaitan, R Knoche, NA Larsen, C Lee, BG Lenardo, KT Lesko, A Lindote, MI Lopes, DC Malling, A Manalaysay, RL Mannino, MF Marzioni, DN McKinsey, DM Mei, J Mock, M Moongweluwan, JA Morad, A St J Murphy, C Nehrkorn, HN Nelson, F Neves, K O'Sullivan, KC Oliver-Mallory, KJ Palladino, M Pangilinan, EK Pease, P Phelps, L Reichhart, CA Rhyne, S Shaw, TA Shutt, C Silva, M Solmaz, VN Solovov, P Sorensen, S Stephenson, TJ Sumner, M Szydagis, DJ Taylor, WC Taylor, BP Tennyson, PA Terman, DR Tiedt, WH To, M Tripathi, L Tvrznikova, S Uvarov, JR Verbus, RC Webb, JT White, TJ Whitis, MS Witherell, FLH Wolfs, J Xu, K Yazdani, SK Young, C Zhang

Abstract:

The Large Underground Xenon (LUX) experiment is a dual-phase liquid xenon time projection chamber (TPC) operating at the Sanford Underground Research Facility in Lead, South Dakota. A calibration of nuclear recoils in liquid xenon was performed $\textit{in situ}$ in the LUX detector using a collimated beam of mono-energetic 2.45 MeV neutrons produced by a deuterium-deuterium (D-D) fusion source. The nuclear recoil energy from the first neutron scatter in the TPC was reconstructed using the measured scattering angle defined by double-scatter neutron events within the active xenon volume. We measured the absolute charge ($Q_{y}$) and light ($L_{y}$) yields at an average electric field of 180 V/cm for nuclear recoil energies spanning 0.7 to 74 keV and 1.1 to 74 keV, respectively. This calibration of the nuclear recoil signal yields will permit the further refinement of liquid xenon nuclear recoil signal models and, importantly for dark matter searches, clearly demonstrates measured ionization and scintillation signals in this medium at recoil energies down to $\mathcal{O}$(1 keV).

Characteristics of Four Upward-Pointing Cosmic-Ray-like Events Observed with ANITA

Physical Review Letters American Physical Society (APS) 117:7 (2016) 071101

Authors:

PW Gorham, J Nam, A Romero-Wolf, S Hoover, P Allison, O Banerjee, JJ Beatty, K Belov, DZ Besson, WR Binns, V Bugaev, P Cao, C Chen, P Chen, JM Clem, A Connolly, B Dailey, C Deaconu, L Cremonesi, PF Dowkontt, MA DuVernois, RC Field, BD Fox, D Goldstein, J Gordon, C Hast, CL Hebert, B Hill, K Hughes, R Hupe, MH Israel, A Javaid, J Kowalski, J Lam, JG Learned, KM Liewer, TC Liu, JT Link, E Lusczek, S Matsuno, BC Mercurio, C Miki, P Miočinović, M Mottram, K Mulrey, CJ Naudet, J Ng, RJ Nichol, K Palladino, BF Rauch, K Reil, J Roberts, M Rosen, B Rotter, J Russell, L Ruckman, D Saltzberg, D Seckel, H Schoorlemmer, S Stafford, J Stockham, M Stockham, B Strutt, K Tatem, GS Varner, AG Vieregg, D Walz, SA Wissel, F Wu

The CRESST-III low-mass WIMP detector

Journal of Physics: Conference Series Institute of Physics 718:4 (2016) 042048

Authors:

Godehard Angloher, Antonio Bento, Carlo Bucci, Lucia Canonica, Xavier Defay, Andreas Erb, Franz von Feilitzsch, Nahuel Ferreiro Iachellini, Paolo Gorla, Achim Gütlein, Dieter Hauff, Josef Jochum, Margit Kiefer, Holger Kluck, Hans Kraus, Jean-Come Lanfranchi, Jurek Loebell, Andrea Münster, Carmine Pagliarone, Federica Petricca, Christian Strandhagen, Anja Tanzke, Hong H Trinh Thi, Cenk Türkoğlu, Martin Uffinger

Abstract:

The next generation direct dark matter experiment CRESST-III has a high potential to significantly increase the sensitivity to low-mass WIMPs (mx ≲10 GeV/c2). We present the new CRESST detector module: it consists of a 24 g CaWO4 crystal operated as a phonon detector and a 20x20 mm^2 silicon-on-sapphire light detector. The phonon energy threshold is lowered to ~100 eV and a light detector resolution of typically 5 eV is achieved. A fully-scintillating inner detector housing is realised which efficiently rejects events from surface alpha decays. The CaWO4 sticks holding the target crystal are also operated as calorimeters to discriminate all possible artefacts related to the support structure. A projection for the sensitivity to spin-independent WIMP-nucleon scattering is given for the first phase of CRESSTIII which will start beginning of 2016.