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The case for a directional dark matter detector and the status of current experimental efforts

  • S. Ahlen
  • , N. Afshordi
  • , J. B.R. Battat
  • , J. Billard
  • , N. Bozorgnia
  • , S. Burgos
  • , T. Caldwell
  • , J. M. Carmona
  • , S. Cebrian
  • , P. Colas
  • , T. Dafni
  • , E. Daw
  • , D. Dujmic
  • , A. Dushkin
  • , W. Fedus
  • , E. Ferrer
  • , D. Finkbeiner
  • , P. H. Fisher
  • , J. Forbes
  • , T. Fusayasu
  • J. Galan, T. Gamble, C. Ghag, I. Giomataris, M. Gold, H. Gomez, M. E. Gomez, P. Gondolo, A. Green, C. Grignon, O. Guillaudin, C. Hagemann, K. Hattori, S. Henderson, N. Higashi, C. Ida, F. J. Iguaz, A. Inglis, I. G. Irastorza, S. Iwaki, A. Kaboth, S. Kabuki, J. Kadyk, N. Kallivayalil, H. Kubo, S. Kurosawa, V. A. Kudryavtsev, T. Lamy, R. Lanza, T. B. Lawson, A. Lee, E. R. Lee, T. Lin, D. Loomba, J. Lopez, G. Luzon, T. Manobu, J. Martoff, F. Mayet, B. McCluskey, E. Miller, K. Miuchi, J. Monroe, B. Morgan, D. Muna, A. St J. Murphy, T. Naka, K. Nakamura, M. Nakamura, T. Nakano, G. G. Nicklin, H. Nishimura, K. Niwa, S. M. Paling, J. Parker, A. Petkov, M. Pipe, K. Pushkin, M. Robinson, A. Rodriguez, J. Rodriguez-Quintero, T. Sahin, R. Sanderson, N. Sanghi, D. Santos, O. Sato, T. Sawano, G. Sciolla, H. Sekiya, T. R. Slatyer, D. P. Snowden-Ifft, N. J.C. Spooner, A. Sugiyama, A. Takada, M. Takahashi, A. Takeda, T. Tanimori, K. Taniue, A. Tomas, H. Tomita, K. Tsuchiya, J. Turk, E. Tziaferi, K. Ueno, S. Vahsen, R. Vanderspek, J. Vergados, J. A. Villar, H. Wellenstein, I. Wolfe, R. K. Yamamoto, H. Yegoryan
  • Boston University
  • Perimeter Institute for Theoretical Physics
  • University of Waterloo
  • Massachusetts Institute of Technology
  • Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
  • University of California at Los Angeles
  • Occidental College
  • University of Pennsylvania
  • University of Zaragoza
  • Laboratorio Subterráneo de Canfranc
  • DBJC/SBFM CEA-Saclay
  • University of Sheffield
  • Brandeis University
  • Harvard University
  • Nagasaki Institute of Applied Science
  • University of Edinburgh
  • University of New Mexico
  • University of Huelva
  • University of Utah
  • University of Nottingham
  • Kyoto University
  • Lawrence Berkeley National Laboratory
  • High Energy Accelerator Research Organization, Institute of Particle and Nuclear Physics
  • Temple University
  • University of Warwick
  • New York University
  • Nagoya University
  • The University of Tokyo
  • Saga University
  • JAXA Institute of Space and Astronautical Science
  • University of Ioannina

Research output: Contribution to journalArticlepeer-review

Abstract

We present the case for a dark matter detector with directional sensitivity. This document was developed at the 2009 CYGNUS workshop on directional dark matter detection, and contains contributions from theorists and experimental groups in the field. We describe the need for a dark matter detector with directional sensitivity; each directional dark matter experiment presents their project's status; and we close with a feasibility study for scaling up to a one ton directional detector, which would cost around $150M.

Original languageEnglish
Pages (from-to)1-51
Number of pages51
JournalInternational Journal of Modern Physics A
Volume25
Issue number1
DOIs
Publication statusPublished - 10 Jan 2010
Externally publishedYes

Keywords

  • Dark matter
  • Directional detection

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