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Updated search for spectral lines from Galactic dark matter interactions with pass 8 data from the Fermi Large Area Telescope

  • M. Ackermann
  • , M. Ajello
  • , A. Albert
  • , B. Anderson
  • , W. B. Atwood
  • , L. Baldini
  • , G. Barbiellini
  • , D. Bastieri
  • , R. Bellazzini
  • , E. Bissaldi
  • , R. D. Blandford
  • , E. D. Bloom
  • , R. Bonino
  • , E. Bottacini
  • , T. J. Brandt
  • , J. Bregeon
  • , P. Bruel
  • , R. Buehler
  • , S. Buson
  • , G. A. Caliandro
  • R. A. Cameron, R. Caputo, M. Caragiulo, P. A. Caraveo, C. Cecchi, E. Charles, A. Chekhtman, J. Chiang, G. Chiaro, S. Ciprini, R. Claus, J. Cohen-Tanugi, J. Conrad, A. Cuoco, S. Cutini, F. D'Ammando, A. De Angelis, F. De Palma, R. Desiante, S. W. Digel, L. Di Venere, P. S. Drell, A. Drlica-Wagner, C. Favuzzi, S. J. Fegan, A. Franckowiak, Y. Fukazawa, S. Funk, P. Fusco, F. Gargano, D. Gasparrini, N. Giglietto, F. Giordano, M. Giroletti, G. Godfrey, G. A. Gomez-Vargas, I. A. Grenier, J. E. Grove, S. Guiriec, M. Gustafsson, J. W. Hewitt, A. B. Hill, D. Horan, G. Jóhannesson, R. P. Johnson, M. Kuss, S. Larsson, L. Latronico, J. Li, L. Li, F. Longo, F. Loparco, M. N. Lovellette, P. Lubrano, D. Malyshev, M. Mayer, M. N. Mazziotta, J. E. McEnery, P. F. Michelson, T. Mizuno, A. A. Moiseev, M. E. Monzani, A. Morselli, S. Murgia, E. Nuss, T. Ohsugi, M. Orienti, E. Orlando, J. F. Ormes, D. Paneque, M. Pesce-Rollins, F. Piron, G. Pivato, S. Rainò, R. Rando, M. Razzano, A. Reimer, T. Reposeur, S. Ritz, M. Sánchez-Conde, A. Schulz, C. Sgrò, E. J. Siskind, F. Spada, G. Spandre, P. Spinelli, H. Tajima, H. Takahashi, J. B. Thayer, L. Tibaldo, D. F. Torres, G. Tosti, E. Troja, G. Vianello, M. Werner, B. L. Winer, K. S. Wood, M. Wood, G. Zaharijas, S. Zimmer
  • c/o DESY
  • Clemson University
  • Kavli Institute for Particle Astrophysics and Cosmology
  • Stockholm University
  • Oskar Klein Centre
  • University of California at Santa Cruz
  • University of Pisa
  • INFN Sezione di Trieste
  • University of Trieste
  • INFN
  • University of Padova
  • Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
  • INFN Sezione di Bari
  • INFN Sezione di Torino
  • University of Turin
  • NASA Goddard Space Flight Center
  • Laboratoire Univers et Particules de Montpellier
  • Consorzio Interuniversitario per la Fisica Spaziale (CIFS)
  • INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan
  • INFN Sezione di Perugia
  • University of Perugia
  • George Mason University
  • Naval Research Laboratory
  • Science and Research Directorate
  • Osservatorio Astronomico di Roma
  • Royal Swedish Academy of Sciences
  • INAF Istituto di Radioastronomia
  • University of Bologna
  • and Physics University of Udine
  • Università Telematica Pegaso
  • Politecnico di Bari
  • Fermi National Accelerator Laboratory
  • Hiroshima University
  • Sezione di Roma
  • Pontificia Universidad Católica de Chile
  • Universite Paris-Saclay
  • Georg-August-Universität Göttingen
  • Biochemical and Environmental Engineering
  • University of Southampton
  • University of Iceland
  • University of Sheffield
  • KTH Royal Institute of Technology
  • University of Maryland
  • Long Beach VA and University of California
  • University of Denver
  • Max-Planck-Institut für Physik
  • Medical University of Innsbruck
  • UMR 5797
  • NYCB Real-Time Computing Inc.
  • Nagoya University
  • Pompeu Fabra University (UPF)
  • The Ohio State University
  • University of Nova Gorica

Résultats de recherche: Contribution à un journalArticleRevue par des pairs

Résumé

Dark matter in the Milky Way may annihilate directly into γ rays, producing a monoenergetic spectral line. Therefore, detecting such a signature would be strong evidence for dark matter annihilation or decay. We search for spectral lines in the Fermi Large Area Telescope observations of the Milky Way halo in the energy range 200 MeV-500 GeV using analysis methods from our most recent line searches. The main improvements relative to previous works are our use of 5.8 years of data reprocessed with the Pass 8 event-level analysis and the additional data resulting from the modified observing strategy designed to increase exposure of the Galactic center region. We search in five sky regions selected to optimize sensitivity to different theoretically motivated dark matter scenarios and find no significant detections. In addition to presenting the results from our search for lines, we also investigate the previously reported tentative detection of a line at 133 GeV using the new Pass 8 data.

langue originaleAnglais
Numéro d'article122002
journalPhysical Review D - Particles, Fields, Gravitation and Cosmology
Volume91
Numéro de publication12
Les DOIs
étatPublié - 22 juin 2015

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