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In addition to three active neutrinos, one or more light sterile neutrinos have been conjectured to account for the LSND, MiniBooNE and reactor antineutrino anomalies (at the sub-eV mass scale) or for warm dark matter in the Universe (at the keV mass scale).
Z. Maki, M. Nakagawa, and S. Sakata, Prog. Theor. Phys. 28
1968
Earlier work this paper cites.
P. Minkowski, Phys. Lett. B 67
1980
Earlier work this paper cites.
J. Schechter and J.W.F. Valle, Phys. Rev. D 22
1981
Earlier work this paper cites.
C. Jarlskog, Phys. Rev. Lett. 55
1985
Earlier work this paper cites.
M. Fukugita and T. Yanagida, Phys. Lett. B 174
1986
Earlier work this paper cites.
H. Fritzsch and Z.Z. Xing, Prog. Part. Nucl. Phys. 45
2000
Earlier work this paper cites.
A. Aguilar et al
2001
Earlier work this paper cites.
P. Bode, J.P. Ostriker, and N. Turok, Astrophys. J. 556
2001
Earlier work this paper cites.
For a detailed calculation of ε i α \varepsilon_{i\alpha} , see: Z.Z. Xing and S. Zhou, Neutrinos in Particle Physics, Astronomy and Cosmology
2004
Earlier work this paper cites.
S. Antusch, C. Biggio, E. Fernandez-Martinez, M.B. Gavela, and J. Lopez-Pavon, JHEP 0610
2006
Earlier work this paper cites.
A numerical reconstruction of the 3 × 3 3\times 3 Majorana neutrino mass matrix has been done by B. Dziewit, K. Kajda, J. Gluza, and M. Zralek, Phys. Rev. D 74
2006
Cited alongside, same era.
See, e.g., M. Maltoni and T. Schwetz, Phys. Rev. D 76
2007
Cited alongside, same era.
Z.Z. Xing, Phys. Lett. B 660
2008
Cited alongside, same era.
X.G. Wu, thesis for a bachelor’s degree, Peking University (2009)
2009
Cited alongside, same era.
M. Malinsky, T. Ohlsson, Z.Z. Xing, and H. Zhang, Phys. Lett. B 679
2009
Cited alongside, same era.
E. Fernandez-Martinez, M.B. Gavela, J. L o ´ \rm\acute{o} pez-Pav o ´ \rm\acute{o} n, and O. Yasuda, Phys. Lett. B 649
2009
Cited alongside, same era.
J. Kopp, M. Maltoni, and T. Schwetz, Phys. Rev. Lett. 107
2011
Closest in time.
J. Hamann et al
2011
Closest in time.
See, e.g., G. Mangano and P.D. Serpico, Phys. Lett. B 701
2011
Closest in time.
See, e.g., T. Asaka, S. Blanchet, and M. Shaposhnikov, Phys. Lett. B 631
2011
Closest in time.
See, e.g., D.K. Ghosh, G. Senjanovic, and Y. Zhang, Phys. Lett. B 698
2011
Closest in time.
Z.Z. Xing, invited plenary talk given at COSMO/CosPA 2010, September 2010, Tokyo; Y.F. Li and Z.Z. Xing, Phys. Lett. B 695
2011
Closest in time.
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A.A. Aguilar-Arevalo et al
2010
Cited alongside, same era.
Particle Data Group, K. Nakamura et al
2010
Cited alongside, same era.
Z.Z. Xing, Chin. Phys. C 34
2010
Cited alongside, same era.
G. Mention et al
2011
Cited alongside, same era.
Y.F. Li and S.S. Liu, arXiv:1110.5795
Cited in the paper.
A formally exact but very different parametrization of the 6 × 6 6\times 6 neutrino mixing matrix in the type-I seesaw framework has been done in: M. Blennow and E. Fernandez-Martinez, Phys. Lett. B 704
2011
Closest in time.
Z.Z. Xing, Phys. Rev. D 68
2011
Closest in time.
For a recent review, see: W. Rodejohann, Int. J. Mod. Phys. E 20
2011
Closest in time.