Built on

N. D. Christensen and C. Duhr, Comput. Phys. Commun. 180
Original
1921
Earlier work this paper cites.
S. Kanemura, T. Matsui and H. Sugiyama, Phys. Rev. D 90
Original
1935
Earlier work this paper cites.
S. Weinberg, Phys. Rev. Lett. 43
1979
Earlier work this paper cites.
P. Minkowski, Phys. Lett. B 67
1980
Earlier work this paper cites.
R. N. Mohapatra and G. Senjanovic, Phys, Rev. Lett. 44
1982
Earlier work this paper cites.
D. Weyler and L. Wolfenstein, Nucl. Phys. B 218
1987
Earlier work this paper cites.
A. Zee, Nucl. Phys. B 264
1988
Earlier work this paper cites.
A. Zee, Phys. Lett. B 93
1992
Earlier work this paper cites.
E. Akhmedov, M. Lindner, E. Schnapka, J. W. F. Valle, Phys. Lett. B 368
1996
Earlier work this paper cites.
J. Hisano, T. Moroi, K. Tobe and M. Yamaguchi, Phys. Rev. D 53
1996
Earlier work this paper cites.
E. Ma, Mod. Phys. Lett. A 17
2002
Earlier work this paper cites.
M. Malinsky, J. C. Romao, and J. W. F. Valle, Phys. Rev. Lett. 95, 161801 (2005)
2005
Earlier work this paper cites.
G. Bertone, D. Hooper and J. Silk, Phys. Rept. 405
2005
Earlier work this paper cites.
E. Ma, Phys. Rev. D 73
2006
Earlier work this paper cites.
G. Cacciapaglia, C. Csaki, G. Marandella and A. Strumia, Phys. Rev. D 74
2006
Earlier work this paper cites.
T. Han and B. Zhang, Phys. Rev. Lett. 97
2006
Earlier work this paper cites.
V. Barger, P. Langacker and G. Shaughnessy, Phys. Rev. D 75
2007
Earlier work this paper cites.
G. B¨¦langer, F. Boudjema, A. Pukhov and A. Semenov, Comput. Phys. Commun. 192
Original
2007
Earlier work this paper cites.
F. del Aguila, J. A. Aguilar-Saavedra and R. Pittau, JHEP 0710
2007
Earlier work this paper cites.
E. Ma, Phys. Lett. B 662
Original
2008
Earlier work this paper cites.
S. Khalil, J. Phys. G 35
2008
Earlier work this paper cites.
V. Barger, P. Langacker, M. McCaskey, M. J. Ramsey-Musolf and G. Shaughnessy, Phys. Rev. D 77
Original
2008
Earlier work this paper cites.

Similar

P. Langacker, Rev. Mod. Phys. 81
Original
2009
Cited alongside, same era.
E. Ma, Phys. Rev. D 80
Original
2009
Cited alongside, same era.
L. Basso, A. Belyaev, S. Moretti and C. H. Shepherd-Themistocleous, Phys. Rev. D 80
Original
2009
Cited alongside, same era.
A. Atre, T. Han, S. Pascoli and B. Zhang, JHEP 0905
Original
2009
Cited alongside, same era.
B. Aubert et al
Original
2010
Cited alongside, same era.

Then

J. Adam et al
Original
2013
Later among the works it cites.
A. Falkowski, F. Riva and A. Urbano, JHEP 1311
Original
2013
Later among the works it cites.
J. Baglio, A. Djouadi, R. Gröber, M. M. M¨¹hlleitner, J. Quevillon and M. Spira, JHEP 1304
Original
2013
Later among the works it cites.
M. Aoki and T. Toma, JCAP 1409
Original
2014
Later among the works it cites.
L. M. Krauss, S. Nasri and M. Trodden, Phys. Rev. D 67
2014
Later among the works it cites.

Beyond the bibliography

alphaXiv searches the wider corpus for related work and actual follow-ups.

Open on alphaXiv

alphaXiv is searching for related work…

Reading the bibliography…

2015

Radiative Linear Seesaw model, Dark Matter and $U(1)_{B-L}$

Wang, Weijian, Han, Zhi-Long

Understand

In this paper we propose a radiated linear seesaw model where the naturally small term $\mu_{L}$ are generated at one-loop level and its soft-breaking of lepton number symmetry attributes to the spontaneous breaking(SSB) of B-L gauge symmetry.

The value of $B-L$ charges for new particles are assigned to satisfy the anomalies cancelation.
It is founded that some new particles may have exotic values of $B-L$ charge such that there exists residual $Z_{2}\times Z_{2}^{\prime}$ symmetry even after SSB of $B-L$ gauge symmetry.
The $Z_{2}\times Z_{2}^{\prime}$ discrete symmetry stabilizes the these particles as dark matter candidates.

Built on

N. D. Christensen and C. Duhr, Comput. Phys. Commun. 180
Original
1921
Earlier work this paper cites.
S. Kanemura, T. Matsui and H. Sugiyama, Phys. Rev. D 90
Original
1935
Earlier work this paper cites.
S. Weinberg, Phys. Rev. Lett. 43
1979
Earlier work this paper cites.
P. Minkowski, Phys. Lett. B 67
1980
Earlier work this paper cites.
R. N. Mohapatra and G. Senjanovic, Phys, Rev. Lett. 44
1982
Earlier work this paper cites.
D. Weyler and L. Wolfenstein, Nucl. Phys. B 218
1987
Earlier work this paper cites.
A. Zee, Nucl. Phys. B 264
1988
Earlier work this paper cites.
A. Zee, Phys. Lett. B 93
1992
Earlier work this paper cites.
E. Akhmedov, M. Lindner, E. Schnapka, J. W. F. Valle, Phys. Lett. B 368
1996
Earlier work this paper cites.
J. Hisano, T. Moroi, K. Tobe and M. Yamaguchi, Phys. Rev. D 53
1996
Earlier work this paper cites.
E. Ma, Mod. Phys. Lett. A 17
2002
Earlier work this paper cites.
M. Malinsky, J. C. Romao, and J. W. F. Valle, Phys. Rev. Lett. 95, 161801 (2005)
2005
Earlier work this paper cites.
G. Bertone, D. Hooper and J. Silk, Phys. Rept. 405
2005
Earlier work this paper cites.
E. Ma, Phys. Rev. D 73
2006
Earlier work this paper cites.
G. Cacciapaglia, C. Csaki, G. Marandella and A. Strumia, Phys. Rev. D 74
2006
Earlier work this paper cites.
T. Han and B. Zhang, Phys. Rev. Lett. 97
2006
Earlier work this paper cites.
V. Barger, P. Langacker and G. Shaughnessy, Phys. Rev. D 75
2007
Earlier work this paper cites.
G. B¨¦langer, F. Boudjema, A. Pukhov and A. Semenov, Comput. Phys. Commun. 192
Original
2007
Earlier work this paper cites.
F. del Aguila, J. A. Aguilar-Saavedra and R. Pittau, JHEP 0710
2007
Earlier work this paper cites.
E. Ma, Phys. Lett. B 662
Original
2008
Earlier work this paper cites.
S. Khalil, J. Phys. G 35
2008
Earlier work this paper cites.
V. Barger, P. Langacker, M. McCaskey, M. J. Ramsey-Musolf and G. Shaughnessy, Phys. Rev. D 77
Original
2008
Earlier work this paper cites.