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2012

Fermionic Dark Matter in Radiative Inverse Seesaw Model with U(1)_{B-L}

Okada, Hiroshi, Toma, Takashi

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We construct a radiative inverse seesaw model with local B-L symmetry, and investigate the flavor structure of the lepton sector and the fermionic Dark Matter.

Neutrino masses are radiatively generated through a kind of inverse seesaw framework.
The PMNS matrix is derived from each mixing matrix of the neutrino and charged lepton sector with large Dirac CP phase.
We show that the annihilation processes via the interactions with Higgses which are independent on the lepton flavor violation, have to be dominant in order to satisfy the observed relic abundance by WMAP.

Fermionic Dark Matter in Radiative Inverse Seesaw Model with U(1)_{B-L} · Around

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Z. Maki, M. Nakagawa and S. Sakata, Prog. Theor. Phys. 28
1962
Earlier work this paper cites.
R. N. Mohapatra, Phys. Rev. Lett. 56
1986
Earlier work this paper cites.
R. N. Mohapatra and J. W. F. Valle, Phys. Rev. D 34
1986
Earlier work this paper cites.
A. Corsetti and P. Nath, Phys. Rev. D 64
2001
Earlier work this paper cites.
L. M. Krauss, S. Nasri and M. Trodden, Phys. Rev. D 67
2003
Earlier work this paper cites.
M. S. Carena, A. Daleo, B. A. Dobrescu and T. M. P. Tait, Phys. Rev. D 70
2004
Earlier work this paper cites.
S. Antusch and S. F. King, Phys. Lett. B 631
2005
Earlier work this paper cites.
E. Ma, Phys. Rev. D 73
2006
Earlier work this paper cites.
J. Kubo, E. Ma and D. Suematsu, Phys. Lett. B 642
2006
Earlier work this paper cites.
J. Kubo and D. Suematsu, Phys. Lett. B 643
2006
Earlier work this paper cites.
H. Ohki, H. Fukaya, S. Hashimoto, T. Kaneko, H. Matsufuru, J. Noaki, T. Onogi and E. Shintani et al
Original
2008
Earlier work this paper cites.

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