Advertisement

Prospects for the Detection of SUSY Dark Matter

  • David B. Cline
Conference paper

Keywords

Dark Matter Direct Search Dark Matter Particle Pulse Shape Analysis Liquid Xenon 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

References

  1. 1.
    See the Proceedings of the 5th Symposium on Sources and Detection of Dark Matter and Dark Energy in the Universe, Elsevier 2004.Google Scholar
  2. 2.
    F. Zwicky, Helv. Phys. Act. 6, 110 (1933)MATHADSGoogle Scholar
  3. 3.
    C. Rubbia and W.K. Ford, Ap. J. 159, 379 (1970); D.H. Rogstad and G.S. Shostak, Ap. J. 176, 315 (1972)CrossRefADSGoogle Scholar
  4. 4.
    C.L. Bennett et al, Ap. J. Suppl. 148, 1 (2003)CrossRefADSGoogle Scholar
  5. 5.
    P. Sikivie, Phys. Lett. B. 432, 139 (1998)CrossRefADSGoogle Scholar
  6. 6.
    A. Green, Phys Rev D 68, 023004 (2003); C. Copi, L. Krauss, Phys Rev D 67, 103507 (2003); J.F. Navarro, C.S. Frank and S.D.M. White, Ap. J. 462, 563 (1996); B. Moore et al, Ap. J. Lett. 499, L5 (1998)CrossRefADSGoogle Scholar
  7. 7.
    K. Freese, J.A. Frieman and A Gould, Phys. Rev. D 37, 3388 (1988); G. Gelmini and P. Gondolo, Phys. Rev. D 64, 023504 (2001); F.S. Ling, P. Sikivie and S. Wick, Diurnal and Annual Modulation of Cold Dark Matter Signals, UFIFTHET-04-6CrossRefADSGoogle Scholar
  8. 8.
    D.B. Cline: Direct Search for Dark Matter Particles with Very Large Detectors, in: Proceedings for Beyond the Desert 2003, Springer Proceedings in Physics v. 92, Hans Klapdor-Kleingrothaus, ed., 2004Google Scholar
  9. 9.
    M.W. Goodman and E. Witten, Phys. Rev. D 31, 3059 (1985); A. Drukier, K. Freese and D.N. Spergel, Phys. Rev. D 33, 3495 (1986); I. Wasserman, Phys. Rev. D 33, 2071 (1986)CrossRefADSGoogle Scholar
  10. 10.
    J.R. Primack, D. Seckel and B. Sadoulet, Ann. Rev. Nucl. Part. Sci. 38, 751 (1988); P.F. Smith and J.D. Lewin, Phys. Rep. 187 203 (1990); G. Jungman, M. Kamionkowski and K. Griest, Phys. Rep. 267, 195 (1996)CrossRefADSGoogle Scholar
  11. 11.
    D. Cline, Scientific American 288:3, 50–59 (2003)MathSciNetCrossRefGoogle Scholar
  12. 12.
    D. Cline, A. Curioni, A. Lamarina et al, Astropart. Phys. 12, 373–377 (1999)CrossRefGoogle Scholar
  13. 13.
    A. Bottino et al, Phys. Rev. D 69, 037302 (2004)CrossRefADSGoogle Scholar
  14. 14.
    U. Chattopadhyay and P. Nath, hep-ph/0405157Google Scholar
  15. 15.
    D.S. Akerib et al (CDMS Collaboration), Phys. Rev. D 68, 82002 (2003)CrossRefADSGoogle Scholar
  16. 16.
    A. Benoit et al, Phys. Lett. B 545 43 (2002)Google Scholar
  17. 17.
    L. Stodolksy and F. Probst, talk at Dark Side of the Universe, Ann Arbor, May 2004Google Scholar
  18. 18.
    CDMS II; see Table 3Google Scholar
  19. 19.
    D. Cline, Y. Seo, H. Wang et al.: Status of ZEPLIN II and ZEPLIN IV Study, in: Nuclear Physics B, Proceedings Supplements, 5th International Symposium on Search and Detection of Dark Matter and Dark Energy in the Universe, ed. by D.B. Cline (Elsevier, Amsterdam 2003) pp 229–232Google Scholar
  20. 20.
    XENON Detector; see Table 3Google Scholar
  21. 21.
    See for example D. Cline: ZEPLIN IV: A One Ton WIMP Detector, a paper given at the Dark 2002 meeting, Capetown, January 2002, to be published in: Proceedings of DARK 2002, eds. H.V. Klapdor-Kleingrothaus and R. Viollier, pp 492–498Google Scholar
  22. 22.
    Private communication from H. WangGoogle Scholar
  23. 23.
    GENIUS; see Table 3Google Scholar

Copyright information

© Springer-Verlag Berlin Heidelberg 2006

Authors and Affiliations

  • David B. Cline
    • 1
  1. 1.Astrophysics Division, Department of Physics & AstronomyUniversity of CaliforniaLos AngelesUSA

Personalised recommendations