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We propose an extended version of the standard model, in which neutrino oscillation, dark matter, and baryon asymmetry of the Universe can be simultaneously explained by the TeV-scale physics without assuming unnatural hierarchy among the mass scales.
A. D. Sakharov, Pisma Zh. Eksp. Teor. Fiz. 5
1967
Earlier work this paper cites.
T. Appelquist and J. Carazzone, Phys. Rev. D 11
1975
Earlier work this paper cites.
T. Yanagida, in Proceedings of Workshop on the Unified Theory and the Baryon Number in the Universe
1979
Earlier work this paper cites.
G. Passarino and M. J. G. Veltman, Nucl. Phys. B 160
1979
Earlier work this paper cites.
A. Zee, Phys. Lett. B 93
1985
Earlier work this paper cites.
S. L. Glashow and S. Weinberg, Phys. Rev. D 15
1990
Earlier work this paper cites.
J. F. Gunion, et al., “ The Higgs Hunters’s Guide
1990
Earlier work this paper cites.
E. W. Kolb and M. S. Turner, The Early Universe
1990
Earlier work this paper cites.
B. K. Bullock, K. Hagiwara and A. D. Martin, Phys. Rev. Lett. 67
1991
Cited alongside, same era.
G. W. Anderson and L. J. Hall, Phys. Rev. D 45
1992
Cited alongside, same era.
G. D. Moore, Phys. Lett. B 439
1998
Cited alongside, same era.
S. Kanemura, et al., Phys. Rev. D 64
2001
Cited alongside, same era.
L. M. Krauss, S. Nasri and M. Trodden, Phys. Rev. D 67
2003
Cited alongside, same era.
K. Cheung and O. Seto, Phys. Rev. D 69
2004
Cited alongside, same era.
S. Kanemura, et al., Phys. Lett. B 558
2004
Cited alongside, same era.
S. Kanemura, Y. Okada and E. Senaha, Phys. Lett. B 606
2005
Later among the works it cites.
W. M. Yao, et al., J. Phys. G 33
2006
Later among the works it cites.
J. M. Cline, K. Kainulainen and A. P. Vischer, Phys. Rev. D 54
2006
Later among the works it cites.
Y. D. Kim, Phys. Atom. Nucl. 69
2006
Later among the works it cites.
A. Baldini, Nucl. Phys. Proc. Suppl. 168
2007
Later among the works it cites.
J. McDonald, Phys. Rev. D 50
2008
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S. Kanemura and C. P. Yuan, Phys. Lett. B 530
2004
Cited alongside, same era.
E. Komatsu, et al., arXiv:0803.0547 [astro-ph]
Cited in the paper.
E. Barberio, et al., arXiv:hep-ex/0603003
Cited in the paper.
The unitarity bound for the scattering process h η → H + S − h\eta\rightarrow H^{+}S^{-} turns out to give κ ∼ < 25 \kappa\mbox{ \raisebox{-4.30554pt}{$\stackrel{{\scriptstyle\textstyle<}}{{\textstyle\sim}}$ }}25 , whereas tan β \tan\beta should not be too large for successful electroweak baryogenesis [ 6 ]
Cited in the paper.
M. Aoki, S. Kanemura and O. Seto, in preparation
Cited in the paper.
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