Limits on momentum-dependent asymmetric dark matter with CRESST-II

(2016)

Authors:

G Angloher, A Bento, C Bucci, L Canonica, X Defay, A Erb, FV Feilitzsch, N Ferreiro Iachellini, P Gorla, A Gütlein, D Hauff, J Jochum, M Kiefer, H Kluck, H Kraus, J-C Lanfranchi, J Loebell, A Münster, C Pagliarone, F Petricca, W Potzel, F Pröbst, F Reindl, K Schäffner, J Schieck, S Schönert, W Seidel, L Stodolsky, C Strandhagen, R Strauss, A Tanzke, HH Trinh Thi, C Türkoğlu, M Uffinger, A Ulrich, I Usherov, S Wawoczny, M Willers, M Wüstrich, A Zöller

Direct dark matter search with the CRESST II experiment

Proceedings of Science Part F128556 (2016)

Authors:

J Schieck, G Angloher, A Bento, C Bucci, L Canonica, X Defay, A Erb, FV Feilitzsch, NF Iachellini, P Gorla, A Gütlein, D Hauff, J Jochum, M Kiefer, H Kluck, H Kraus, JC Lanfranchi, J Loebell, M Mancuso, A Münster, C Pagliarone, F Petricca, W Potzel, F Pröbst, R Puig, F Reindl, K Schäffner, S Schönert, W Seidel, M Stahlberg, L Stodolsky, C Strandhagen, R Strauss, A Tanzke, HHT Thi, C Türkoǧlu, M Uffinger, A Ulrich, I Usherov, S Wawoczny, M Willers, M Wüstrich, A Zöller

Abstract:

The quest for the particle nature of dark matter is one of the big open questions of modern physics. A well motivated candidate for dark matter is the so-called WIMP - a weakly interacting massive particle. Recently several theoretically well-motivated models with dark matter candidates in a mass region below the WIMP mass-scale gained also a lot of interest, theoretically and experimentally. The CRESST II experiment located at the Gran Sasso laboratory in Italy is optimised for the detection of the elastic scattering of these low-mass dark matter particles with ordinary matter. We show the results obtained with an improved detector setup with increased radio purity and enhanced background rejection and the results obtained with a dedicated low-threshold analysis of a single conventional detector module. The limit achieved is the most stringent limit achieved for direct dark matter experiments in the mass region below 1.8 GeV/c2. We will discuss the expected performance for new small CRESST-type detectors to be used during the next data taking phase. We conclude with an outlook of the future potential for direct dark matter detection using further improved CRESST CaWO4 cryogenic detectors.

Results on light dark matter particles with a low-threshold CRESST-II detector

European Physical Journal C Springer Nature 76:1 (2016) 25

Authors:

G Angloher, A Bento, C Bucci, L Canonica, X Defay, A Erb, F von Feilitzsch, N Ferreiro Iachellini, P Gorla, A Gütlein, D Hauff, J Jochum, M Kiefer, H Kluck, H Kraus, JC Lanfranchi, J Loebell, A Münster, C Pagliarone, F Petricca, W Potzel, F Pröbst, F Reindl, K Schäffner, J Schieck, S Schönert, W Seidel, L Stodolsky, C Strandhagen, R Strauss, A Tanzke, HH Trinh Thi, C Türkoğlu, M Uffinger, A Ulrich, I Usherov, S Wawoczny, M Willers, M Wüstrich, A Zöller

Simulation of light collection in calcium tungstate scintillation detectors

Nuclear Physics and Atomic Energy National Academy of Sciences of Ukraine 16:4 (2015) 329-336

Authors:

FA Danevich, Academy of Sciences of Ukraine Institute for Nuclear Research, VV Kobychev, RV Kobychev, H Kraus, VB Mikhailik, VM Mokina, University of Ukraine Kyiv Politechnic Institute Heat Power Engineering Faculty, University of Oxford Department of Physics, Didcot Diamond Light Source

Improved Limits on Scattering of Weakly Interacting Massive Particles from Reanalysis of 2013 LUX data

(2015)

Authors:

LUX Collaboration, DS Akerib, HM Araújo, X Bai, AJ Bailey, J Balajthy, P Beltrame, EP Bernard, A Bernstein, TP Biesiadzinski, EM Boulton, A Bradley, R Bramante, 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 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, RA Ott, KJ Palladino, M Pangilinan, EK Pease, P Phelps, L Reichhart, C Rhyne, S Shaw, TA Shutt, C Silva, VN Solovov, P Sorensen, S Stephenson, TJ Sumner, M Szydagis, DJ Taylor, W 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, K Yazdani, SK Young, C Zhang