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Results on Low-Mass Weakly Interacting Massive Particles from an 11 kg d Target Exposure of DAMIC at SNOLAB.
Aguilar-Arevalo, A; Amidei, D; Baxter, D; Cancelo, G; Vergara, B A Cervantes; Chavarria, A E; D'Olivo, J C; Estrada, J; Favela-Perez, F; Gaïor, R; Guardincerri, Y; Hoppe, E W; Hossbach, T W; Kilminster, B; Lawson, I; Lee, S J; Letessier-Selvon, A; Matalon, A; Mitra, P; Overman, C T; Piers, A; Privitera, P; Ramanathan, K; Da Rocha, J; Sarkis, Y; Settimo, M; Smida, R; Thomas, R; Tiffenberg, J; Traina, M; Vilar, R; Virto, A L.
Afiliación
  • Aguilar-Arevalo A; Universidad Nacional Autónoma de México, Mexico City, 04510, Mexico.
  • Amidei D; Department of Physics, University of Michigan, Ann Arbor, Michigan 48109-1040, USA.
  • Baxter D; Kavli Institute for Cosmological Physics and The Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637, USA.
  • Cancelo G; Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA.
  • Vergara BAC; Universidad Nacional Autónoma de México, Mexico City, 04510, Mexico.
  • Chavarria AE; Center for Experimental Nuclear Physics and Astrophysics, University of Washington, Seattle, Washington 98195, USA.
  • D'Olivo JC; Universidad Nacional Autónoma de México, Mexico City, 04510, Mexico.
  • Estrada J; Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA.
  • Favela-Perez F; Universidad Nacional Autónoma de México, Mexico City, 04510, Mexico.
  • Gaïor R; Laboratoire de Physique Nucléaire et des Hautes Énergies (LPNHE), Sorbonne Université, Université de Paris, CNRS-IN2P3, 75005 Paris, France.
  • Guardincerri Y; Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA.
  • Hoppe EW; Pacific Northwest National Laboratory (PNNL), Richland, Washington 99354, USA.
  • Hossbach TW; Pacific Northwest National Laboratory (PNNL), Richland, Washington 99354, USA.
  • Kilminster B; Universität Zürich Physik Institut, Zurich 8057, Switzerland.
  • Lawson I; SNOLAB, Lively, Ontario P3Y 1N2, Canada.
  • Lee SJ; Universität Zürich Physik Institut, Zurich 8057, Switzerland.
  • Letessier-Selvon A; Laboratoire de Physique Nucléaire et des Hautes Énergies (LPNHE), Sorbonne Université, Université de Paris, CNRS-IN2P3, 75005 Paris, France.
  • Matalon A; Kavli Institute for Cosmological Physics and The Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637, USA.
  • Mitra P; Laboratoire de Physique Nucléaire et des Hautes Énergies (LPNHE), Sorbonne Université, Université de Paris, CNRS-IN2P3, 75005 Paris, France.
  • Overman CT; Center for Experimental Nuclear Physics and Astrophysics, University of Washington, Seattle, Washington 98195, USA.
  • Piers A; Pacific Northwest National Laboratory (PNNL), Richland, Washington 99354, USA.
  • Privitera P; Center for Experimental Nuclear Physics and Astrophysics, University of Washington, Seattle, Washington 98195, USA.
  • Ramanathan K; Kavli Institute for Cosmological Physics and The Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637, USA.
  • Da Rocha J; Laboratoire de Physique Nucléaire et des Hautes Énergies (LPNHE), Sorbonne Université, Université de Paris, CNRS-IN2P3, 75005 Paris, France.
  • Sarkis Y; Kavli Institute for Cosmological Physics and The Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637, USA.
  • Settimo M; Laboratoire de Physique Nucléaire et des Hautes Énergies (LPNHE), Sorbonne Université, Université de Paris, CNRS-IN2P3, 75005 Paris, France.
  • Smida R; Universidad Nacional Autónoma de México, Mexico City, 04510, Mexico.
  • Thomas R; SUBATECH, CNRS-IN2P3, IMT Atlantique, Université de Nantes, Nantes 44300, France.
  • Tiffenberg J; Kavli Institute for Cosmological Physics and The Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637, USA.
  • Traina M; Kavli Institute for Cosmological Physics and The Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637, USA.
  • Vilar R; Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA.
  • Virto AL; Laboratoire de Physique Nucléaire et des Hautes Énergies (LPNHE), Sorbonne Université, Université de Paris, CNRS-IN2P3, 75005 Paris, France.
Phys Rev Lett ; 125(24): 241803, 2020 Dec 11.
Article en En | MEDLINE | ID: mdl-33412014
ABSTRACT
We present constraints on the existence of weakly interacting massive particles (WIMPs) from an 11 kg d target exposure of the DAMIC experiment at the SNOLAB underground laboratory. The observed energy spectrum and spatial distribution of ionization events with electron-equivalent energies >200 eV_{ee} in the DAMIC CCDs are consistent with backgrounds from natural radioactivity. An excess of ionization events is observed above the analysis threshold of 50 eV_{ee}. While the origin of this low-energy excess requires further investigation, our data exclude spin-independent WIMP-nucleon scattering cross sections σ_{χ-n} as low as 3×10^{-41} cm^{2} for WIMPs with masses m_{χ} from 7 to 10 GeV c^{-2}. These results are the strongest constraints from a silicon target on the existence of WIMPs with m_{χ}<9 GeV c^{-2} and are directly relevant to any dark matter interpretation of the excess of nuclear-recoil events observed by the CDMS silicon experiment in 2013.

Texto completo: 1 Colección: 01-internacional Banco de datos: MEDLINE Idioma: En Revista: Phys Rev Lett Año: 2020 Tipo del documento: Article País de afiliación: México

Texto completo: 1 Colección: 01-internacional Banco de datos: MEDLINE Idioma: En Revista: Phys Rev Lett Año: 2020 Tipo del documento: Article País de afiliación: México