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The data acquisition system of the LZ dark matter detector: FADR

  • J. Aalbers
  • , D. S. Akerib
  • , A. K. Al Musalhi
  • , F. Alder
  • , C. S. Amarasinghe
  • , A. Ames
  • , T. J. Anderson
  • , N. Angelides
  • , H. M. Araújo
  • , J. E. Armstrong
  • , M. Arthurs
  • , A. Baker
  • , S. Balashov
  • , J. Bang
  • , E. E. Barillier
  • , J. W. Bargemann
  • , K. Beattie
  • , T. Benson
  • , A. Bhatti
  • , A. Biekert
  • T. P. Biesiadzinski, H. J. Birch, E. Bishop, G. M. Blockinger, B. Boxer, C. A.J. Brew, P. Brás, J. H. Buckley, S. Burdin, M. Buuck, M. C. Carmona-Benitez, M. Carter, A. Chawla, H. Chen, J. J. Cherwinka, Y. T. Chin, N. I. Chott, M. V. Converse, A. Cottle, G. Cox, D. Curran, C. E. Dahl, A. David, J. Delgaudio, S. Dey, L. de Viveiros, L. Di Felice, T. Dimino, C. Ding, J. E.Y. Dobson, E. Druszkiewicz, S. R. Eriksen, A. Fan, N. M. Fearon, N. Fieldhouse, S. Fiorucci, H. Flaecher, E. D. Fraser, T. M.A. Fruth, R. J. Gaitskell, A. Geffre, R. Gelfand, J. Genovesi, C. Ghag, R. Gibbons, S. Gokhale, J. Green, M. G.D. van der Grinten, J. J. Haiston, C. R. Hall, S. Han, E. Hartigan-O'Connor, S. J. Haselschwardt, M. A. Hernandez, S. A. Hertel, G. Heuermann, G. J. Homenides, M. Horn, D. Q. Huang, D. Hunt, E. Jacquet, R. S. James, J. Johnson, A. C. Kaboth, A. C. Kamaha, M. Kannichankandy, D. Khaitan, A. Khazov, I. Khurana, J. Kim, Y. D. Kim, J. Kingston, R. Kirk, D. Kodroff, L. Korley, E. V. Korolkova, M. Koyuncu, H. Kraus, S. Kravitz, L. Kreczko, V. A. Kudryavtsev, D. S. Leonard, K. T. Lesko, C. Levy, J. Lin, A. Lindote, R. Linehan, W. H. Lippincott, C. Loniewski, M. I. Lopes, W. Lorenzon, C. Lu, S. Luitz, P. A. Majewski, A. Manalaysay, R. L. Mannino, C. Maupin, M. E. McCarthy, G. McDowell, D. N. McKinsey, J. McLaughlin, J. B. Mclaughlin, R. McMonigle, E. H. Miller, E. Mizrachi, A. Monte, M. E. Monzani, M. Moongweluwan, J. D.Morales Mendoza, E. Morrison, B. J. Mount, M. Murdy, A. St J. Murphy, A. Naylor, H. N. Nelson, F. Neves, A. Nguyen, J. A. Nikoleyczik, H. Oh, I. Olcina, M. A. Olevitch, K. C. Oliver-Mallory, J. Orpwood, K. J. Palladino, J. Palmer, N. J. Pannifer, N. Parveen, S. J. Patton, B. Penning, G. Pereira, E. Perry, T. Pershing, A. Piepke, Y. Qie, J. Reichenbacher, C. A. Rhyne, Q. Riffard, G. R.C. Rischbieter, H. S. Riyat, R. Rosero, T. Rushton, D. Rynders, D. Santone, R. Sarkis, A. B.M.R. Sazzad, R. W. Schnee, S. Shaw, T. Shutt, J. J. Silk, C. Silva, G. Sinev, J. Siniscalco, W. Skulski, R. Smith, V. N. Solovov, P. Sorensen, J. Soria, I. Stancu, A. Stevens, K. Stifter, B. Suerfu, T. J. Sumner, M. Szydagis, W. C. Taylor, D. R. Tiedt, M. Timalsina, Z. Tong, D. R. Tovey, J. Tranter, M. Trask, M. Tripathi, D. R. Tronstad, A. Vacheret, A. C. Vaitkus, J. Vaitkus, O. Valentino, V. Velan, A. Wang, J. J. Wang, Y. Wang, J. R. Watson, R. C. Webb, L. Weeldreyer, T. J. Whitis, M. Williams, W. J. Wisniewski, F. L.H. Wolfs, J. D. Wolfs, S. Woodford, D. Woodward, C. J. Wright, Q. Xia, X. Xiang, J. Xu, M. Yeh, J. Yin
  • SLAC National Accelerator Laboratory
  • Kavli Institute for Particle Astrophysics and Cosmology
  • University College London
  • University of California at Santa Barbara
  • University of Michigan, Ann Arbor
  • Imperial College London
  • University of Maryland, College Park
  • STFC Rutherford Appleton Laboratory (RAL)
  • Brown University
  • University of Zurich
  • Lawrence Berkeley National Laboratory
  • University of Wisconsin-Madison
  • University of California at Berkeley
  • University of Edinburgh
  • SUNY Albany
  • University of California at Davis
  • University of Coimbra
  • Washington University St. Louis
  • University of Liverpool
  • Pennsylvania State University
  • Royal Holloway University of London
  • South Dakota School of Mines & Technology
  • University of Rochester
  • South Dakota Science and Technology Authority
  • Northwestern University
  • Fermi National Accelerator Laboratory
  • University of Oxford
  • King's College London
  • University of Bristol
  • University of Sydney
  • Brookhaven National Laboratory
  • University of Massachusetts
  • University of Alabama
  • University of California at Los Angeles
  • Institute for Basic Science
  • University of Sheffield
  • University of Texas at Austin
  • Lawrence Livermore National Laboratory
  • Vatican Observatory
  • Black Hills State University
  • SkuTek Instrumentation
  • Texas A&M University

Research output: Contribution to journalArticlepeer-review

2 Scopus citations

Abstract

The Data Acquisition System (DAQ) for the LUX-ZEPLIN (LZ) dark matter detector is described. The signals from 745 PMTs, distributed across three subsystems, are sampled with 100-MHz 32-channel digitizers (DDC-32s). A basic waveform analysis is carried out on the on-board Field Programmable Gate Arrays (FPGAs) to extract information about the observed scintillation and electroluminescence signals. This information is used to determine if the digitized waveforms should be preserved for offline analysis. The system is designed around the Kintex-7 FPGA. In addition to digitizing the PMT signals and providing basic event selection in real time, the flexibility provided by the use of FPGAs allows us to monitor the performance of the detector and the DAQ in parallel to normal data acquisition. The hardware and software/firmware of this FPGA-based Architecture for Data acquisition and Realtime monitoring (FADR) are discussed and performance measurements are described.

Keywords

  • Dark matter
  • Data acquisition
  • FPGA
  • Firmware

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