Possible lower bounds for the direct detection rate of SUSY dark matter

Physics of Atomic Nuclei

Volumn 66, Issue 3, 2003, Pages 490-493

  Bednyakov, V A ^a  

^a JOINT INSTITUTE FOR NUCLEAR RESEARCH   (Russian Federation)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0037659238     PISSN: 10637788     EISSN: None     Source Type: Journal    
DOI: 10.1134/1.1563711     Document Type: Conference Paper

References (33)

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15. R. Arnowitt and P. Nath, Phys. Rev. D 54, 2374 (1996); 56, 2820 (1997); Phys. Lett. B 437, 344 (1998); R. Arnowitt, Phys. At. Nucl. 61, 1098 (1998); V. Mandic, A. T. Pierce, P. Gondolo, and H. Murayama, hep-ph/0008022; R. Arnowitt, B. Dutta, and Y. Santoso, hep-ph/0008336; hep-ph/0005154; A. B. Lahanas, D. V. Nanopoulos, and V. C. Spanos, Mod. Phys. Lett. A 16, 1229 (2001); A. Bottino, F. Donato, N. Fornengo, and S. Scopel, Phys. Rev. D 59, 095004 (1999); V. Berezinsky et al., Astropart. Phys. 5, l (1996); A. Bottino, F. Donato, N. Fomengo, and S. Scopel, Phys. Rev. D 63, 125003 (2001); H. Baer and M. Brhlik, Phys. Rev. D 57, 567 (1998); J. L. Feng, K. T. Matchev, and F. Wilczek, Phys. Lett. B 482, 388 (2000); E. Gabrielli, S. Khalil, C. Munoz, and E. Torrente-Lujan, Phys. Rev. D 63, 025008 (2001); E. Accomando, R. Arnowitt, B. Dutta, and Y. Santoso, Nucl. Phys. B 585, 124 (2000); L. Bergström and P. Gondolo, Astropart. Phys. 6, 263 (1996); J. D. Vergados, Phys. Rev. Lett. 83, 3597 (1999); Phys. Rev. D 62, 023519 (2000); Part. Nucl. Lett. 106, 74 (2001).
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22. R. Arnowitt and P. Nath, Phys. Rev. D 54, 2374 (1996); 56, 2820 (1997); Phys. Lett. B 437, 344 (1998); R. Arnowitt, Phys. At. Nucl. 61, 1098 (1998); V. Mandic, A. T. Pierce, P. Gondolo, and H. Murayama, hep-ph/0008022; R. Arnowitt, B. Dutta, and Y. Santoso, hep-ph/0008336; hep-ph/0005154; A. B. Lahanas, D. V. Nanopoulos, and V. C. Spanos, Mod. Phys. Lett. A 16, 1229 (2001); A. Bottino, F. Donato, N. Fornengo, and S. Scopel, Phys. Rev. D 59, 095004 (1999); V. Berezinsky et al., Astropart. Phys. 5, l (1996); A. Bottino, F. Donato, N. Fomengo, and S. Scopel, Phys. Rev. D 63, 125003 (2001); H. Baer and M. Brhlik, Phys. Rev. D 57, 567 (1998); J. L. Feng, K. T. Matchev, and F. Wilczek, Phys. Lett. B 482, 388 (2000); E. Gabrielli, S. Khalil, C. Munoz, and E. Torrente-Lujan, Phys. Rev. D 63, 025008 (2001); E. Accomando, R. Arnowitt, B. Dutta, and Y. Santoso, Nucl. Phys. B 585, 124 (2000); L. Bergström and P. Gondolo, Astropart. Phys. 6, 263 (1996); J. D. Vergados, Phys. Rev. Lett. 83, 3597 (1999); Phys. Rev. D 62, 023519 (2000); Part. Nucl. Lett. 106, 74 (2001).
23. R. Arnowitt and P. Nath, Phys. Rev. D 54, 2374 (1996); 56, 2820 (1997); Phys. Lett. B 437, 344 (1998); R. Arnowitt, Phys. At. Nucl. 61, 1098 (1998); V. Mandic, A. T. Pierce, P. Gondolo, and H. Murayama, hep-ph/0008022; R. Arnowitt, B. Dutta, and Y. Santoso, hep-ph/0008336; hep-ph/0005154; A. B. Lahanas, D. V. Nanopoulos, and V. C. Spanos, Mod. Phys. Lett. A 16, 1229 (2001); A. Bottino, F. Donato, N. Fornengo, and S. Scopel, Phys. Rev. D 59, 095004 (1999); V. Berezinsky et al., Astropart. Phys. 5, l (1996); A. Bottino, F. Donato, N. Fomengo, and S. Scopel, Phys. Rev. D 63, 125003 (2001); H. Baer and M. Brhlik, Phys. Rev. D 57, 567 (1998); J. L. Feng, K. T. Matchev, and F. Wilczek, Phys. Lett. B 482, 388 (2000); E. Gabrielli, S. Khalil, C. Munoz, and E. Torrente-Lujan, Phys. Rev. D 63, 025008 (2001); E. Accomando, R. Arnowitt, B. Dutta, and Y. Santoso, Nucl. Phys. B 585, 124 (2000); L. Bergström and P. Gondolo, Astropart. Phys. 6, 263 (1996); J. D. Vergados, Phys. Rev. Lett. 83, 3597 (1999); Phys. Rev. D 62, 023519 (2000); Part. Nucl. Lett. 106, 74 (2001).
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