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Large-scale shell-model calculations of elastic and inelastic scattering rates of lightest supersymmetric particles (LSP) on I127, Xe129, Xe131, and Cs133 nuclei

P. Toivanen, M. Kortelainen, J. Suhonen, and J. Toivanen

  • Department of Physics, University of Jyväskylä, Post Office Box 35, FIN-40014 Jyväskylä, Finland

Phys. Rev. C 79, 044302 – Published 2 April, 2009

DOI: https://doi.org/10.1103/PhysRevC.79.044302

Abstract

We discuss the dark-matter detection rates for the elastic and inelastic scattering of the lightest supersymmetric particle (LSP) off nuclei. For this we use an easily accessible formalism where the underlying nuclear physics is condensed in structure coefficients multiplying the key parameters of supersymmetric theories. In this work we compute these coefficients for the stable iodine, xenon, and cesium nuclei by application of the nuclear shell model in a model space involving the 2s, 1d, 0g7/2, and 0h11/2 single-particle orbitals. As an interaction we use the renormalized Bonn-CD G matrix. By using fitted nuclear gyromagnetic factors we have successfully reproduced the relevant spectroscopic data on magnetic moments and M1 decays in the discussed nuclei.

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References (44)

  1. G. Jungman, M. Kamionkowski, and K. Griest, Phys. Rep. 267, 195 (1996).
  2. S. T. Lin et al., arXiv:0712.1645 [hep-ex].
  3. D. S. Akerib et al., Phys. Rev. Lett. 96, 011302 (2006); , Phys. Rev. D 73, 011102 (2006).
  4. V. Sanglard et al., Phys. Rev. D 71, 122002 (2005).
  5. G. Angloher et al., Astropart. Phys. 23, 325 (2005).
  6. G. J. Alner et al., Astropart. Phys. 23, 444 (2005).
  7. J. Angle et al., Phys. Rev. Lett. 100, 021303 (2008).
  8. P. Belli et al., Phys. Lett. B387, 222 (1996).
  9. R. Bernabei et al., Phys. Lett. B436, 379 (1998).
  10. R. Bernabei et al., New J. Phys. 2, 15 (2000).
  11. K. Ueshima et al., Nucl. Inst. Meth. A 594, 148 (2008).
  12. H. S. Lee et al., Phys. Rev. Lett. 99, 091301 (2007).
  13. N. J. C. Spooner et al., Phys. Lett. B473, 330 (2000).
  14. S. Cebrián et al., Astropart. Phys. 15, 79 (2001).
  15. T. A. Girard et al., Phys. Lett. B621, 233 (2005).
  16. M. Barnabe-Heider et al., Phys. Lett. B624, 186 (2005).
  17. E. Behnke et al., Science 319, 933 (2008).
  18. R. Bernabei et al., Phys. Lett. B424, 195 (1998); , ibid. B450, 448 (1999).
  19. R. Bernabei et al., Phys. Lett. B480, 23 (2000); R. Abusaidi et al., Phys. Rev. Lett. 84, 5699 (2000).
  20. R. Bernabei et al., Riv. Nuovo Cimento 26, 1 (2003).
  21. M. Kortelainen, T. S. Kosmas, J. Suhonen, and J. Toivanen, Phys. Lett. B632, 226 (2006).
  22. J. D. Vergados, Phys. Rev. Lett. 83, 3597 (1999); Phys. Rev. D 62, 023519 (2000); 67, 103003 (2003).
  23. M. E. Gomez and J. D. Vergados, Phys. Lett. B512, 252 (2001); M. E. Gomez, G. Lazarides, and C. Pallis, ibid. B487, 313 (2000); Phys. Rev. D 61, 123512 (2000).
  24. J. D. Vergados and H. Ejiri, Phys. Lett. B606, 313 (2005).
  25. T. S. Kosmas and J. D. Vergados, Phys. Rev. D 55, 1752 (1997); J. D. Vergados and T. S. Kosmas, Phys. At. Nucl. 61, 1066 (1998).
  26. P. Toivanen, M. Kortelainen, J. Suhonen, and J. Toivanen, Phys. Lett. B666, 1 (2008).
  27. A. K. Drukier, K. Freese, and D. N. Spergel, Phys. Rev. D 33, 3495 (1986); J. Ellis and R. A. Flores, Nucl. Phys. B307, 883 (1988).
  28. J. Engel and P. Vogel, Phys. Rev. D 40, 3132 (1989).
  29. J. Engel, Phys. Lett. B264, 114 (1991).
  30. F. Iachello, L. M. Krauss, and G. Maino, Phys. Lett. B254, 220 (1991).
  31. M. A. Nikolaev and H. V. Klapdor-Kleingrothaus, Z. Phys. A 345, 373 (1993).
  32. M. T. Ressell and D. J. Dean, Phys. Rev. C 56, 535 (1997).
  33. E. Holmlund, M. Kortelainen, T. S. Kosmas, J. Suhonen, and J. Toivanen, Phys. Lett. B584, 31 (2004).
  34. J. D. Vergados, P. Quentin, and D. Strottman, Int. J. Mod. Phys. E 14, 751 (2005).
  35. J. Ellis, R. A. Flores, and J. D. Lewin, Phys. Lett. B212, 375 (1988).
  36. J. Engel and P. Vogel, Phys. Rev. D 61, 063503 (2000).
  37. J. Toivanen, computer code EICODE, JYFL, Finland, 2004.
  38. M. Hjorth-Jensen, T. T. S. Kuo, and E. Osnes, Phys. Rep. 260, 125 (1995); M. Hjorth-Jensen (private communication).
  39. M. Horoi, B. A. Brown, and V. Zelevinsky, Phys. Rev. C 50, R2274 (1994).
  40. J. D. Vergados, J. Phys. G: Nucl. Part. Phys. 22, 253 (1996).
  41. J. Suhonen, From Nucleons to Nucleus: Concepts of Microscopic Nuclear Theory (Springer-Verlag, Berlin, 2007).
  42. R. Helm, Phys. Rev. 104, 1466 (1956).
  43. G. Duda, A. Kemper, and P. Gondolo, J. Cosmol. Astropart. Phys. 04 (2007) 012.
  44. G. L. Kane, C. Kolda, L. Roszkowski, and J. D. Wells, Phys. Rev. D 49, 6173 (1994).

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