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P. f. Yin, Q. Yuan, J. Liu, J. Zhang, X. j. Bi and S. h. Zhu, arXiv:0811.0176 [hep-ph]; I. Gogoladze, R. Khalid, Q. Shafi and H. Yuksel, arXiv:0901.0923 [hep-ph]; K. Ishiwata, S. Matsumoto and T. Moroi, arXiv:0811.0250 [hep-ph]; C. R. Chen, F. Takahashi and T. T. Yanagida, arXiv:0811.0477 [hep-ph]; K. Hamaguchi, E. Nakamura, S. Shirai and T. T. Yanagida, arXiv:0811.0737 [hep-ph]; A. Ibarra and D. Tran, arXiv:0811.1555 [hep-ph]; C. R. Chen, F. Takahashi and T. T. Yanagida, arXiv:0811.3357 [astro-ph]; X. J. Bi, P. H. Gu, T. Li and X. Zhang, arXiv:0901.0176 [hep-ph]; A. Arvanitaki, S. Dimopoulos, S. Dubovsky, P. W. Graham, R. Harnik and S. Rajendran, arXiv:0812.2075 [hep-ph]

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2009

Type II Seesaw and the PAMELA/ATIC Signals

Gogoladze, Ilia, Okada, Nobuchika, Shafi, Qaisar

Understand

We discuss how the cosmic ray signals reported by the PAMELA and ATIC/PPB-BETS experiments may be understood in a Standard Model (SM) framework supplemented by type II seesaw and a stable SM singlet scalar boson as dark matter.

A particle physics explanation of the 'boost' factor can be provided by including an additional SM singlet scalar field.

Built on

G. Lazarides, Q. Shafi and C. Wetterich, Nucl. Phys. B181
1980
Earlier work this paper cites.
V. Silveira and A. Zee, Phys. Lett. B 161
1985
Earlier work this paper cites.
E. W. Kolb and M. S. Turner, The Early Universe,
1990
Earlier work this paper cites.
F. A. Aharonian, A. M. Atoyan and H. J. Volk, Astron. Astrophys. 294
Original
1995
Earlier work this paper cites.
C. P. Burgess, M. Pospelov and T. ter Veldhuis, Nucl. Phys. B 619
2001
Earlier work this paper cites.
C. L. Bennett et al
Original
2003
Earlier work this paper cites.