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First Constraints from DAMIC-M on Sub-GeV Dark-Matter Particles Interacting with Electrons.
Arnquist, I; Avalos, N; Baxter, D; Bertou, X; Castelló-Mor, N; Chavarria, A E; Cuevas-Zepeda, J; Gutiérrez, J Cortabitarte; Duarte-Campderros, J; Dastgheibi-Fard, A; Deligny, O; De Dominicis, C; Estrada, E; Gadola, N; Gaïor, R; Hossbach, T; Iddir, L; Khalil, L; Kilminster, B; Lantero-Barreda, A; Lawson, I; Lee, S; Letessier-Selvon, A; Loaiza, P; Lopez-Virto, A; Matalon, A; Munagavalasa, S; McGuire, K J; Mitra, P; Norcini, D; Papadopoulos, G; Paul, S; Piers, A; Privitera, P; Ramanathan, K; Robmann, P; Settimo, M; Smida, R; Thomas, R; Traina, M; Vila, I; Vilar, R; Warot, G; Yajur, R; Zopounidis, J-P.
Afiliação
  • Arnquist I; Pacific Northwest National Laboratory (PNNL), Richland, Washington, USA.
  • Avalos N; Centro Atómico Bariloche and Instituto Balseiro, Comisión Nacional de Energía Atómica (CNEA), Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET), Universidad Nacional de Cuyo (UNCUYO), San Carlos de Bariloche 8400, Argentina.
  • Baxter D; Kavli Institute for Cosmological Physics and The Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637, USA.
  • Bertou X; Centro Atómico Bariloche and Instituto Balseiro, Comisión Nacional de Energía Atómica (CNEA), Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET), Universidad Nacional de Cuyo (UNCUYO), San Carlos de Bariloche 8400, Argentina.
  • Castelló-Mor N; Instituto de Física de Cantabria (IFCA), CSIC-Universidad de Cantabria, Santander 39005, Spain.
  • Chavarria AE; Center for Experimental Nuclear Physics and Astrophysics, University of Washington, Seattle, Washington 98195, USA.
  • Cuevas-Zepeda J; Kavli Institute for Cosmological Physics and The Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637, USA.
  • Gutiérrez JC; Instituto de Física de Cantabria (IFCA), CSIC-Universidad de Cantabria, Santander 39005, Spain.
  • Duarte-Campderros J; Instituto de Física de Cantabria (IFCA), CSIC-Universidad de Cantabria, Santander 39005, Spain.
  • Dastgheibi-Fard A; LPSC LSM, CNRS/IN2P3, Université Grenoble-Alpes, Grenoble 38026, France.
  • Deligny O; CNRS/IN2P3, IJCLab, Université Paris-Saclay, Orsay 91405, France.
  • De Dominicis C; Laboratoire de physique nucléaire et des hautes énergies (LPNHE), Sorbonne Université, Université Paris Cité, CNRS/IN2P3, Paris 75005, France.
  • Estrada E; SUBATECH, Nantes Université, IMT Atlantique, CNRS-IN2P3, Nantes 44300, France.
  • Gadola N; Centro Atómico Bariloche and Instituto Balseiro, Comisión Nacional de Energía Atómica (CNEA), Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET), Universidad Nacional de Cuyo (UNCUYO), San Carlos de Bariloche 8400, Argentina.
  • Gaïor R; Universität Zürich Physik Institut, Zürich 8057, Switzerland.
  • Hossbach T; Laboratoire de physique nucléaire et des hautes énergies (LPNHE), Sorbonne Université, Université Paris Cité, CNRS/IN2P3, Paris 75005, France.
  • Iddir L; Pacific Northwest National Laboratory (PNNL), Richland, Washington, USA.
  • Khalil L; Laboratoire de physique nucléaire et des hautes énergies (LPNHE), Sorbonne Université, Université Paris Cité, CNRS/IN2P3, Paris 75005, France.
  • Kilminster B; Laboratoire de physique nucléaire et des hautes énergies (LPNHE), Sorbonne Université, Université Paris Cité, CNRS/IN2P3, Paris 75005, France.
  • Lantero-Barreda A; Universität Zürich Physik Institut, Zürich 8057, Switzerland.
  • Lawson I; Instituto de Física de Cantabria (IFCA), CSIC-Universidad de Cantabria, Santander 39005, Spain.
  • Lee S; SNOLAB, Lively, Ontario P341N2, Canada.
  • Letessier-Selvon A; Universität Zürich Physik Institut, Zürich 8057, Switzerland.
  • Loaiza P; Laboratoire de physique nucléaire et des hautes énergies (LPNHE), Sorbonne Université, Université Paris Cité, CNRS/IN2P3, Paris 75005, France.
  • Lopez-Virto A; CNRS/IN2P3, IJCLab, Université Paris-Saclay, Orsay 91405, France.
  • Matalon A; Instituto de Física de Cantabria (IFCA), CSIC-Universidad de Cantabria, Santander 39005, Spain.
  • Munagavalasa S; Kavli Institute for Cosmological Physics and The Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637, USA.
  • McGuire KJ; Laboratoire de physique nucléaire et des hautes énergies (LPNHE), Sorbonne Université, Université Paris Cité, CNRS/IN2P3, Paris 75005, France.
  • Mitra P; Kavli Institute for Cosmological Physics and The Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637, USA.
  • Norcini D; Center for Experimental Nuclear Physics and Astrophysics, University of Washington, Seattle, Washington 98195, USA.
  • Papadopoulos G; Center for Experimental Nuclear Physics and Astrophysics, University of Washington, Seattle, Washington 98195, USA.
  • Paul S; Kavli Institute for Cosmological Physics and The Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637, USA.
  • Piers A; Laboratoire de physique nucléaire et des hautes énergies (LPNHE), Sorbonne Université, Université Paris Cité, CNRS/IN2P3, Paris 75005, France.
  • Privitera P; Kavli Institute for Cosmological Physics and The Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637, USA.
  • Ramanathan K; Center for Experimental Nuclear Physics and Astrophysics, University of Washington, Seattle, Washington 98195, USA.
  • Robmann P; 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 Paris Cité, CNRS/IN2P3, Paris 75005, France.
  • Smida R; Kavli Institute for Cosmological Physics and The Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637, USA.
  • Thomas R; Universität Zürich Physik Institut, Zürich 8057, Switzerland.
  • Traina M; SUBATECH, Nantes Université, IMT Atlantique, CNRS-IN2P3, Nantes 44300, France.
  • Vila I; Kavli Institute for Cosmological Physics and The Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637, USA.
  • Vilar R; Kavli Institute for Cosmological Physics and The Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637, USA.
  • Warot G; Center for Experimental Nuclear Physics and Astrophysics, University of Washington, Seattle, Washington 98195, USA.
  • Yajur R; Laboratoire de physique nucléaire et des hautes énergies (LPNHE), Sorbonne Université, Université Paris Cité, CNRS/IN2P3, Paris 75005, France.
  • Zopounidis JP; Instituto de Física de Cantabria (IFCA), CSIC-Universidad de Cantabria, Santander 39005, Spain.
Phys Rev Lett ; 130(17): 171003, 2023 Apr 28.
Article em En | MEDLINE | ID: mdl-37172255
ABSTRACT
We report constraints on sub-GeV dark matter particles interacting with electrons from the first underground operation of DAMIC-M detectors. The search is performed with an integrated exposure of 85.23 g days, and exploits the subelectron charge resolution and low level of dark current of DAMIC-M charge-coupled devices (CCDs). Dark-matter-induced ionization signals above the detector dark current are searched for in CCD pixels with charge up to 7e^{-}. With this dataset we place limits on dark matter particles of mass between 0.53 and 1000 MeV/c^{2}, excluding unexplored regions of parameter space in the mass ranges [1.6,1000] MeV/c^{2} and [1.5,15.1] MeV/c^{2} for ultralight and heavy mediator interactions, respectively.

Texto completo: 1 Base de dados: MEDLINE Idioma: En Ano de publicação: 2023 Tipo de documento: Article

Texto completo: 1 Base de dados: MEDLINE Idioma: En Ano de publicação: 2023 Tipo de documento: Article