Indirect neutralino detection rates in neutrino telescopes

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 55, Issue 4, 1997, Pages 1765-1770

  Bergström, Lars ^a   Edsjö, Joakim ^a   Gondolo, Paolo ^b  

^a UPPSALA UNIVERSITY   (Sweden)

^b UNIVERSITY OF OXFORD   (United Kingdom)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0000858767     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.55.1765     Document Type: Article

References (43)

1. J. Silk, K. Olive, and M. Srednicki, Phys. Rev. Lett.55, 257 (1985);
2. T. Gaisser, G. Steigman, and S. Tilav, Phys. Rev. D34, 2206 (1986);
3. B.A. Campbell, J. Ellis, K. Enqvist, D.V. Nanopoulos, J. Hagelin, and K.A. Olive, Phys. Lett. B173, 270 (1986);
4. M. Srednicki, K. Olive, and J. Silk, Nucl. Phys.B279, 804 (1987);
5. K. Griest and S. Seckel, B283, 681 (1987);
6. J. Hagelin, K. Ng, and K. Olive, Phys. Lett. B180, 375 (1987);
7. K. Ng, K.A. Olive, and M. Srednicki, 188, 138 (1987).
8. K. Freese, Phys. Lett.167B, 295 (1986);
9. L. Krauss, M. Srednicki, and F. Wilczek, Phys. Rev. D33, 2079 (1986);
10. T. Gaisser, G. Steigman, and S. Tilav, 34, 2206 (1986).
11. W.H. Press and D.N. Spergel, Astrophys. J.296, 679 (1985).
12. H. Goldberg, Phys. Rev. Lett.50, 1419 (1983).
13. IMB Collaboration, J.M. Losecco et al., Phys. Lett. B188, 388 (1987);
14. Kamiokande Collaboration, M. Mori et al., 205, 416 (1988);
15. G. Gelmini, P. Gondolo, and E. Roulet, Nucl. Phys.B351, 623 (1991);
16. M. Kamionkowski, Phys. Rev. D44, 3021 (1991);
17. A. Bottino, V. de Alfaro, N. Fornengo, G. Mignola, and M. Pignone, Phys. Lett. B265, 57 (1991);
18. Kamiokande Collaboration, N. Sato et al., Phys. Rev. D44, 2220 (1991);
19. M. Mori et al., Phys. Lett. B270, 89 (1991);
20. 289, 463 (1992);
21. Phys. Rev. D48, 5505 (1993).
22. Baksan telescope, M.M. Boliev et al., in TAUP ’95, Proceedings of the 4th International Workshop on Theoretical and Phenomenological Aspects of Underground Physics, Toledo, Spain, edited by A. Morales Nucl. Phys. B (Proc. Suppl.)48, 83 (1996)].NPBSE7
23. S.W. Barwick, inTrends in Astroparticle Physics, Proceedings of the Workshop, Stockholm, Sweden, 1994, edited by L. Bergström, P. Carlson, P.O. Hulth, and H. Snellman [Nucl. Phys. B (Proc. Suppl.)43(1995)].NPBSE7
24. L. Bergström and P. Gondolo, Astropart. Phys.5, 263 (1996).
25. M. Carena, J.R. Espinosa, M. Quirós, and C.E.M. Wagner, Phys. Lett. B355, 209 (1995).
26. CLEO Collaboration, M.S. Alam et al., Phys. Rev. Lett.71, 674 (1993);
27. 74, 2885 (1995).
28. P. Gondolo and G. Gelmini, Nucl. Phys.B360, 145 (1991).
29. P. Gondolo (in preparation).
30. G. Jungman, M. Kamionkowski, and K. Griest, Phys. Rep.267, 195 (1996).
31. J. Edsjö, Diploma thesis, Uppsala University, 1993;in Trends in Astroparticle Physics 7, p. 265.
32. T. Sjöstrand, Comput. Phys. Commun.82, 74 (1994); “PYTHIA 5.7 and JETSET 7.4. Physics and Manual” (revised version), Report No. CERN-TH.7112/93, hep-ph/9508391 (unpublished).
33. Particle Data Group, L. Montanet et al., Phys. Rev. D50, 1173 (1994).
34. S. Ritz and D. Seckel, Nucl. Phys.B304, 877 (1988).
35. G.F. Giudice and E. Roulet, Nucl. Phys.B316, 429 (1989);
36. F. Halzen, T. Stelzer, and M. Kamionkowski, Phys. Rev. D45, 4439 (1992);
37. M. Drees, G. Jungman, M. Kamionkowski, and M.M. Nojiri, 49, 636 (1994);
38. R. Gandhi, J.L. Lopez, D.V. Nanopoulos, K. Yuan, and A. Zichichi, 49, 3691 (1994);
39. A. Bottino, N. Fornengo, G. Mignola, and L. Moscoso, Astropart. Phys.3, 65 (1995);
40. G. Jungman and M. Kamionkowski, Phys. Rev. D51, 328 (1995); V. Berezinsky, A. Bottino, J. Ellis, N. Fornengo, G. Mignola, and S. Scopel, Report No. hep-ph/9603342 (unpublished).
41. J. Edsjö and P. Gondolo, Phys. Lett. B357, 595 (1995).
42. D. Seckel, T. Stanev, and T. Gaisser, Astrophys. J.382, 652 (1991).
43. E. Accomando et al., “Higgs Physics at LEP2,” Report No. hep-ph/9602250, in “Report of the Workshop on Physics at LEP2,” edited by G. Altarelli, T. Sjöstrand, and F. Zwirner, Report No. CERN 96-01 (in press).