Your browser doesn't support javascript.
loading
First Direct-Detection Constraints on eV-Scale Hidden-Photon Dark Matter with DAMIC at SNOLAB.
Aguilar-Arevalo, A; Amidei, D; Bertou, X; Butner, M; Cancelo, G; Castañeda Vázquez, A; Cervantes Vergara, B A; Chavarria, A E; Chavez, C R; de Mello Neto, J R T; D'Olivo, J C; Estrada, J; Fernandez Moroni, G; Gaïor, R; Guardincerri, Y; Hernández Torres, K P; Izraelevitch, F; Kavner, A; Kilminster, B; Lawson, I; Letessier-Selvon, A; Liao, J; Matalon, A; Mello, V B B; Molina, J; Privitera, P; Ramanathan, K; Sarkis, Y; Schwarz, T; Settimo, M; Sofo Haro, M; Thomas, R; Tiffenberg, J; Tiouchichine, E; Torres Machado, D; Trillaud, F; You, X; Zhou, J.
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.
  • Bertou X; Centro Atómico Bariloche, CNEA/CONICET/IB, Bariloche 8400, Argentina.
  • Butner M; Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA.
  • Cancelo G; Northern Illinois University, DeKalb, Illinois 60115, USA.
  • Castañeda Vázquez A; Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA.
  • Cervantes Vergara BA; Universidad Nacional Autónoma de México, Mexico City 04510, Mexico.
  • Chavarria AE; Universidad Nacional Autónoma de México, Mexico City 04510, Mexico.
  • Chavez CR; Kavli Institute for Cosmological Physics and The Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637, USA.
  • de Mello Neto JRT; Facultad de Ingeniería, Universidad Nacional de Asunción, Asuncion 2169, Paraguay.
  • D'Olivo JC; Universidade Federal do Rio de Janeiro, Instituto de Física, Rio de Janeiro 21.941-611, Brazil.
  • Estrada J; Universidad Nacional Autónoma de México, Mexico City 04510, Mexico.
  • Fernandez Moroni G; Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA.
  • Gaïor R; Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA.
  • Guardincerri Y; Universidad Nacional del Sur, Bahia Blanca 8000, Argentina.
  • Hernández Torres KP; Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Universités Paris 6 et Paris 7, CNRS-IN2P3, F-75005 Paris, France.
  • Izraelevitch F; Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA.
  • Kavner A; Universidad Nacional Autónoma de México, Mexico City 04510, Mexico.
  • Kilminster B; Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA.
  • Lawson I; Department of Physics, University of Michigan, Ann Arbor, Michigan 48109-1040, USA.
  • Letessier-Selvon A; Universität Zürich Physik Institut, Zurich 8057, Switzerland.
  • Liao J; SNOLAB, Lively, Ontario P3Y 1N2, Canada.
  • Matalon A; Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Universités Paris 6 et Paris 7, CNRS-IN2P3, F-75005 Paris, France.
  • Mello VBB; Universität Zürich Physik Institut, Zurich 8057, Switzerland.
  • Molina J; Kavli Institute for Cosmological Physics and The Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637, USA.
  • Privitera P; Universidade Federal do Rio de Janeiro, Instituto de Física, Rio de Janeiro 21.941-611, Brazil.
  • Ramanathan K; Facultad de Ingeniería, Universidad Nacional de Asunción, Asuncion 2169, Paraguay.
  • Sarkis Y; Kavli Institute for Cosmological Physics and The Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637, USA.
  • Schwarz T; Kavli Institute for Cosmological Physics and The Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637, USA.
  • Settimo M; Universidad Nacional Autónoma de México, Mexico City 04510, Mexico.
  • Sofo Haro M; Department of Physics, University of Michigan, Ann Arbor, Michigan 48109-1040, USA.
  • Thomas R; Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Universités Paris 6 et Paris 7, CNRS-IN2P3, F-75005 Paris, France.
  • Tiffenberg J; Centro Atómico Bariloche, CNEA/CONICET/IB, Bariloche 8400, Argentina.
  • Tiouchichine E; Kavli Institute for Cosmological Physics and The Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637, USA.
  • Torres Machado D; Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA.
  • Trillaud F; Centro Atómico Bariloche, CNEA/CONICET/IB, Bariloche 8400, Argentina.
  • You X; Universidade Federal do Rio de Janeiro, Instituto de Física, Rio de Janeiro 21.941-611, Brazil.
  • Zhou J; Universidad Nacional Autónoma de México, Mexico City 04510, Mexico.
Phys Rev Lett ; 118(14): 141803, 2017 Apr 07.
Article en En | MEDLINE | ID: mdl-28430473
We present direct detection constraints on the absorption of hidden-photon dark matter with particle masses in the range 1.2-30 eV c^{-2} with the DAMIC experiment at SNOLAB. Under the assumption that the local dark matter is entirely constituted of hidden photons, the sensitivity to the kinetic mixing parameter κ is competitive with constraints from solar emission, reaching a minimum value of 2.2×10^{-14} at 17 eV c^{-2}. These results are the most stringent direct detection constraints on hidden-photon dark matter in the galactic halo with masses 3-12 eV c^{-2} and the first demonstration of direct experimental sensitivity to ionization signals <12 eV from dark matter interactions.
Texto completo
Añadir a Mi BVS
Imprimir
XML
PubMed Links
Buscar en Google

Texto completo: 1 Colección: 01-internacional Base de datos: MEDLINE Tipo de estudio: Diagnostic_studies Idioma: En Revista: Phys Rev Lett Año: 2017 Tipo del documento: Article País de afiliación: México Pais de publicación: Estados Unidos
Texto completo
Añadir a Mi BVS
Imprimir
XML
PubMed Links
Buscar en Google

Texto completo: 1 Colección: 01-internacional Base de datos: MEDLINE Tipo de estudio: Diagnostic_studies Idioma: En Revista: Phys Rev Lett Año: 2017 Tipo del documento: Article País de afiliación: México Pais de publicación: Estados Unidos