Built on

R. Foot, H. Lew, X.-G. He and G. C. Joshi, Z. Phys. C44 (1989) 441
1989
Earlier work this paper cites.
For a review, see, G. Jungman, M. Kamionkowski and K. Griest, Phys. Rept. 267
1996
Earlier work this paper cites.
R. R. Caldwell, R. Dave and P. J. Steinhardt, Phys. Rev. Lett
1999
Earlier work this paper cites.
B. Spokoiny, Phys. Lett. B
1999
Earlier work this paper cites.
C. H. Chen, M. Drees and J. F. Gunion, Phys. Rev. Lett. 76
1999
Earlier work this paper cites.
E. J. Chun, K. Y. Lee and S. C. Park, Phys. Lett. B 566
2003
Earlier work this paper cites.
P. Salati, Phys. Lett. B 571
2003
Earlier work this paper cites.
T. Asaka, K. Ishiwata and T. Moroi, Phys. Rev. D 73
2006
Earlier work this paper cites.

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2009

Minimal dark matter in type III seesaw

Chun, Eung Jin

Understand

We explore the possibility of a new dark matter candidate in the supersymmetric type III seesaw mechanism where a neutral scalar component of the Y=0 triplet can be the lightest supersymmetric particle.

Its thermal abundance can be in the right range if non-standard cosmology such as kination domination is assumed.
The enhanced cross-section of the dark matter annihilation to W+W- can leave detectable astrophysical and cosmological signals whose current observational data puts a lower bound on the dark matter mass.
The model predicts the existence of a charged scalar almost degenerate with the dark matter scalar and its lifetime lies between 5.5 cm and 6.3 m.

Built on

R. Foot, H. Lew, X.-G. He and G. C. Joshi, Z. Phys. C44 (1989) 441
1989
Earlier work this paper cites.
For a review, see, G. Jungman, M. Kamionkowski and K. Griest, Phys. Rept. 267
1996
Earlier work this paper cites.
R. R. Caldwell, R. Dave and P. J. Steinhardt, Phys. Rev. Lett
1999
Earlier work this paper cites.
B. Spokoiny, Phys. Lett. B
1999
Earlier work this paper cites.
C. H. Chen, M. Drees and J. F. Gunion, Phys. Rev. Lett. 76
1999
Earlier work this paper cites.
E. J. Chun, K. Y. Lee and S. C. Park, Phys. Lett. B 566
2003
Earlier work this paper cites.
P. Salati, Phys. Lett. B 571
2003
Earlier work this paper cites.
T. Asaka, K. Ishiwata and T. Moroi, Phys. Rev. D 73
2006
Earlier work this paper cites.

Similar

M. Cirelli, N. Fornengo and A. Strumia, Nucl. Phys. B 753
2006
Cited alongside, same era.
For a review, see, R. N. Mohapatra et al
2007
Cited alongside, same era.
H.-S. Lee, K. T. Matchev and S. Nasri, Phys. Rev. D 76
2007
Cited alongside, same era.
D. G. Cerdeno, C. Munoz and O. Seto, Phys. Rev. D 79
Original
2008
Cited alongside, same era.
M. Pospelov and A. Ritz, Phys. Rev. D 78
Original
2008
Cited alongside, same era.
R. Franceschini, T. Hambye and A. Strumia, Phys. Rev. D 78
Original
2008