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Indirect, Direct and Collider Detection of SUSY Dark Matter

  • Howard Baer
Conference paper

Keywords

Dark Matter Minimal Supersymmetric Standard Model Hide Sector Standard Model Particle Neutralino Dark Matter 
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.

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References

  1. 1.
    A. Chamseddine, R. Arnowitt and P. Nath, Phys. Rev. Lett. 49 (1982) 970; R. Barbieri, S. Ferrara and C. Savoy, Phys. Lett. B119 (1982) 343; L. J. Hall, J. Lykken and S. Weinberg, Phys. Rev. D27 (1983) 2359; for a review, P. Nath, hep-ph/0307123CrossRefADSGoogle Scholar
  2. 2.
    E. Cremmer, S. Ferrara, L. Girardello and A. van Proeyen, Nucl. Phys. B212, 413 (1983)CrossRefADSGoogle Scholar
  3. 3.
    H. Baer, C. Balazs and A. Belyaev, J. K. Mizukoshi, X. Tata and Y. Wang, JHEP0207, 050 (2002)MathSciNetCrossRefADSGoogle Scholar
  4. 4.
    T. C. Yuan, R. Arnowitt, A. Chamseddine and P. Nath, Z. Phys. C26, 407 (1984). See also U. Chattopadhyay and P. Nath, Phys. Rev. Lett. 86, 5854 (2001)CrossRefADSGoogle Scholar
  5. 5.
    K. Hagiwara, A. Martin, D. Nomura and T. Teubner, Phys. Rev. D69, 093003 (2004)CrossRefADSGoogle Scholar
  6. 6.
    D. N. Spergel et al. (WMAP Collaboration), Astrophys. J. Suppl. 148, 175 (2003)CrossRefADSGoogle Scholar
  7. 7.
    H. Baer and C. Balazs, JCAP0305, 006 (2003).ADSGoogle Scholar
  8. 8.
    J. Ellis, T. Falk and K. Olive, Phys. Lett. B444, 367 (1998); J. Ellis, T. Falk, K. Olive and M. Srednicki, Astropart. Phys. 13, 181 (2000)CrossRefADSGoogle Scholar
  9. 9.
    K. Chan, U. Chattopadhyay and P. Nath, Phys. Rev. D58, 096004 (1998)CrossRefADSGoogle Scholar
  10. 10.
    J. Feng, K. Matchev and T. Moroi, Phys. Rev. D61, 075005 (2000)CrossRefADSGoogle Scholar
  11. 11.
    See also H. Baer, C. H. Chen, F. Paige and X. Tata, Phys. Rev. D52, 2746 (1995) and Phys. Rev. D53, 6241 (1996)CrossRefADSGoogle Scholar
  12. 12.
    M. Drees and M. Nojiri, Phys. Rev. D47, 376 (1993); H. Baer and M. Brhlik, Phys. Rev. D57, 567 (1998); H. Baer, M. Brhlik, M. Diaz, J. Ferrandis, P. Mercadante, P. Quintana and X. Tata, Phys. Rev. D63, 015007 (2001); A. Djouadi, M. Drees and J. Kneur, JHEP0108, 055 (2001); J. Ellis, T. Falk, G. Ganis, K. Olive and M. Srednicki, Phys. Lett. B510, 236 (2001); L. Roszkowski, R. Ruiz de Austri and T. Nihei, JHEP0108, 024 (2001); A. Lahanas and V. Spanos, Eur. Phys. Jou. C23, 185 (2002)CrossRefADSGoogle Scholar
  13. 13.
    D. Dicus, S. Nandi and X. Tata, Phys. Lett. B129, 451 (1983); A. Chamseddine, P. Nath and R. Arnowitt, Phys. Lett. B129, 445 (1983); H. Baer, K. Hagiwara and X. Tata, Phys. Rev. Lett. 57, 294 (1986) and Phys. Rev. D35, 1598 (1987); R. Arnowitt and P. Nath, Mod. Phys. Lett. 2, 331 (1987); H. Baer and X. Tata, Phys. Rev. D47, 2739 (1993)CrossRefADSGoogle Scholar
  14. 14.
    V. Barger and C. Kao, Phys. Rev. D60, 115015 (1999); H. Baer, M. Drees, F. Paige, P. Quintana and X. Tata, Phys. Rev. D61, 095007 (2000); K. Matchev and D. Pierce, Phys. Rev. D60, 075004 (1999) and Phys. Lett. B467, 225 (1999). For an update, see H. Baer, T. Krupovnickas and X. Tata, JHEP0307, 020 (2003)CrossRefADSGoogle Scholar
  15. 15.
    H. Baer, C. Balazs, A. Belyaev, T. Krupovnickas and X. Tata, JHEP0306, 054 (2003)CrossRefADSGoogle Scholar
  16. 16.
    H. Baer, A. Belyaev, T. Krupovnickas and X. Tata, JHEP0402, 007 (2004); H. Baer, T. Krupovnickas and X. Tata, JHEP0406, 061 (2004)CrossRefADSGoogle Scholar
  17. 17.
    For a recent analysis, see H. Baer, C. Balazs, A. Belyaev and J. O’Farrill, JCAP0309, 2003 (007); a subset of earlier work includes M. Goodman and E. Witten, Phys. Rev. D31, 3059 (1985); K. Griest, Phys. Rev. Lett. 61, 666 (1988) and Phys. Rev. D38, 2357 (1988) [Erratum-ibid. D39, 3802 (1989)]; M. Drees and M. Nojiri, Phys. Rev. D47, 4226 (1993) and Phys. Rev. D48, 3483 (1993); V. A. Bednyakov, H. V. Klapdor-Kleingrothaus and S. Kovalenko, Phys. Rev. D50, 7128 (1994); P. Nath and R. Arnowitt, Phys. Rev. Lett. 74, 4592 (1995); L. Bergstrom and P. Gondolo, Astropart. Phys. 5, 263 (1996); H. Baer and M. Brhlik, Phys. Rev. D57, 567 (1998); J. Ellis, A. Ferstl and K. Olive, Phys. Lett. B481, 304 (2000) and Phys. Rev. D63, 065016 (2001); E. Accomando, R. Arnowitt, B. Dutta and Y. Santoso, Nucl. Phys. B585, 124 (2000); A. Bottino, F. Donato, N. Fornengo and S. Scopel, Phys. Rev. D63, 125003 (2001); M. E. Gomez and J. D. Vergados, Phys. Lett. B512, 252 (2001); A. B. Lahanas, D. V. Nanopoulos and V. C. Spanos, Phys. Lett. B518, 94 (2001); A. Corsetti and P. Nath, Phys. Rev. D64, 115009 (2001); E. A. Baltz and P. Gondolo, Phys. Rev. Lett. 86, 5004 (2001); M. Drees, Y. G. Kim, T. Kobayashi and M. M. Nojiri, Phys. Rev. D63, 115009 (2001); see also J. Feng, K. Matchev and F. Wilczek, Ref. [18]; J. R. Ellis, A. Ferstl, K. A. Olive and Y. Santoso, Phys. Rev. D67, 123502 (2003); J. R. Ellis, K. A. Olive, Y. Santoso and V. C. Spanos, Phys. Rev. D69, 015005 (2004); see C. Munoz, hep-ph/0309346 for a recent reviewGoogle Scholar
  18. 18.
    J. Feng, K. Matchev and F. Wilczek, Phys. Rev. D63, 045024 (2001)CrossRefADSGoogle Scholar
  19. 19.
    F. Paige, S. Protopopescu, H. baer and X. Tata, hep-ph/0312045 (2003)Google Scholar
  20. 20.
    DarkSUSY, by P. Gondolo, J. Edsjo, P. Ullio, L. Bergstrom, M. Schelke and E. Baltz, JCAP0407, 008 (2004)ADSGoogle Scholar
  21. 21.
    H. Baer and J. O’ Farrill, JCAP0404, 005 (2004)ADSGoogle Scholar
  22. 22.
    H. Baer, A. Belyaev, T. Krupovnickas and J. O’Farrill, JCAP0408, 005 (2004); for related work, see J. Edsjo, M. Schelke and P. Ulio, astro-ph/0405414 (2004)ADSGoogle Scholar
  23. 23.
    H. Baer, A. Belyaev, T. Krupovnickas and A. Mustafayev, JHEP0406, 044 (2004)CrossRefADSGoogle Scholar

Copyright information

© Springer-Verlag Berlin Heidelberg 2006

Authors and Affiliations

  • Howard Baer
    • 1
  1. 1.Dep’t of PhysicsFlorida State UniversityTallahassee

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