Accès ouvert déclaré
2020
article
Projected WIMP sensitivity of the LUX-ZEPLIN dark matter experiment
D. S. Akerib, C. Akerlof, S. K. Alsum, H. M. Araújo, M. Arthurs, X. Bai, A. J. Bailey, J. Balajthy, S. Balashov, D. Bauer, Jean Louis Van Belle, P. Beltrame, Theophilus Benson, E. P. Bernard, T. P. Biesiadzinski, K. E. Boast, B. Boxer, P. Brás, J. Buckley, V. V. Bugaev, S. Burdin, J. K. Busenitz, C. Carels, D. Carlsmith, B. T. Carlson, M. C. Carmona-Benitez, C. Chan, J. J. Cherwinka, A. Cole, A. Cottle, W. W. Craddock, A. Currie, J. E. Cutter, C. E. Dahl, L. de Viveiros, A. Dobi, J. E. Y. Dobson, E. Druszkiewicz, T. K. Edberg, W. R. Edwards, A. Fan, Simon Fayer, S. Fiorucci, T. Fruth, R. J. Gaitskell, J. Genovesi, C. Ghag, M. G. D. Gilchriese, M. G. D. van der Grinten, C. Hall, S. Hans, K. Hanzel, S. J. Haselschwardt, S. A. Hertel, Seth Hillbrand, C. Hjemfelt, M. D. Hoff, J. Y-K. Hor, D. Q. Huang, C. M. Ignarra, W. Ji, A. C. Kaboth, K. Kamdin, J. Keefner, D. Khaitan, A. Khazov, Y. D. Kim, Charles D. Kocher, E. V. Korolkova, H. Kraus, H. J. Krebs, L. Kreczko, B. Krikler, V. A. Kudryavtsev, S. Kyre, C. Lee, B. G. Lenardo, D. S. Leonard, K. T. Lesko, C. Levy, J. Li, J. Liao, F.-T. Liao, J. Lin, A. Lindote, R. Linehan, W. H. Lippincott, X. Liu, I. Lopes, B. López Paredes, W. Lorenzon, S. Luitz, Justin Lyle, Peter Majewski, A. Manalaysay, R. L. Mannino, C. Maupin, D. N. McKinsey, Yue Meng, E. H. Miller, J. Mock, M. E. Monzani, J. A. Morad, E. Morrison, B. J. Mount, A. St. J. Murphy, H. N. Nelson, F. Neves, J. A. Nikoleyczik, K. O’Sullivan, I. Olcina, M. A. Olevitch, K. C. Oliver-Mallory, K. J. Palladino, S. J. Patton, E. K. Pease, B. Penning, A. Piepke, Samuel B. Powell, R. M. Preece, K. Pushkin, B. N. Ratcliff, J. Reichenbacher, C. A. Rhyne, A. Richards, Juliana Petrocchi Rodrigues, R. Rosero, P. Rossiter, J. S. Saba, Michael Sarychev, R. W. Schnee, M. Schubnell, P. R. Scovell, S. Shaw, T. A. Shutt, J. J. Silk, C. Silva, W. Skulski, M. Solmaz, V. N. Solovov, P. Sørensen, I. Stancu, M. R. Stark, T. M. Stiegler, K. Stifter, M. Szydagis, W. C. Taylor, R. Taylor, D. J. Taylor, Dylan Temples, P. A. Terman, Keenan Thomas, M. Timalsina, W. To, A. Tomás, T. Tope, M. Tripathi, C. E. Tull, L. Tvrznikova, U. Utku, J. Va’vra, A. Vacheret, J.R. Verbus, E. Voirin, W. L. Waldron, J. R. Watson, R. C. Webb, D. T. White, T. J. Whitis, W. J. Wisniewski, M. S. Witherell, F. L. H. Wolfs, D. Woodward, S. D. Worm, M. Yeh, J. Yin, Ian T. Young
296Citations signalées, ce qui n’est pas une note de qualité
38Institutions déclarées
3Pays d’affiliation déclarés
Rattachement africain : us, gb, pt.
Niveau de preuve : code pays fourni par la source.
Le résumé fourni par la source
LUX-ZEPLIN (LZ) is a next-generation dark matter direct detection experiment that will operate 4850 feet underground at the Sanford Underground Research Facility (SURF) in Lead, South Dakota, USA. Using a two-phase xenon detector with an active mass of 7 tonnes, LZ will search primarily for low-energy interactions with weakly interacting massive particles (WIMPs), which are hypothesized to make up the dark matter in our galactic halo. In this paper, the projected WIMP sensitivity of LZ is presented based on the latest background estimates and simulations of the detector. For a 1000 live day run using a 5.6-tonne fiducial mass, LZ is projected to exclude at 90% confidence level spin-independent WIMP-nucleon cross sections above $1.4\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}48}\text{ }\text{ }{\mathrm{cm}}^{2}$ for a $40\text{ }\text{ }\mathrm{GeV}/{c}^{2}$ mass WIMP. Additionally, a $5\ensuremath{\sigma}$ discovery potential is projected, reaching cross sections below the exclusion limits of recent experiments. For spin-dependent WIMP-neutron(-proton) scattering, a sensitivity of $2.3\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}43}\text{ }\text{ }{\mathrm{cm}}^{2}$ ($7.1\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}42}\text{ }\text{ }{\mathrm{cm}}^{2}$) for a $40\text{ }\text{ }\mathrm{GeV}/{c}^{2}$ mass WIMP is expected. With underground installation well underway, LZ is on track for commissioning at SURF in 2020.
Ce résumé expose les affirmations des auteurs. BNTIC ne l’interprète pas comme une validation indépendante des résultats.
Le contrôle bibliographique ouvert
DOI retrouvé dans Crossref DOI retrouvé ; titre concordant.
- Titre Crossref
- Projected WIMP sensitivity of the LUX-ZEPLIN dark matter experiment
- Date Crossref
- 04/03/2020
- Éditeur
- American Physical Society (APS)
- Type
- journal-article
Ce recoupement confirme des métadonnées liées au DOI. Il ne confirme ni la méthode ni les conclusions de l’étude, et il ne compte pas comme une seconde source scientifique indépendante.
Les institutions déclarées
Une affiliation ne permet pas de déduire la nationalité d’un auteur.
Les sujets associés
Dark Matter and Cosmic PhenomenaParticle physics theoretical and experimental studiesAtomic and Subatomic Physics Research