-
1
-
-
4244086361
-
-
LSND Collaboration
-
LSND Collaboration, C. Athanassopoulos et al., Phys. Rev. Lett. 77, 3082 (1996); Phys. Rev. C 58, 2489 (1998); LSND Collaboration, A. Aguilar et al., Phys. Rev. D 64, 112007 (2001).
-
(1996)
Phys. Rev. Lett.
, vol.77
, pp. 3082
-
-
Athanassopoulos, C.1
-
2
-
-
4244095288
-
-
LSND Collaboration, C. Athanassopoulos et al., Phys. Rev. Lett. 77, 3082 (1996); Phys. Rev. C 58, 2489 (1998); LSND Collaboration, A. Aguilar et al., Phys. Rev. D 64, 112007 (2001).
-
(1998)
Phys. Rev. C
, vol.58
, pp. 2489
-
-
-
3
-
-
0035584191
-
-
LSND Collaboration
-
LSND Collaboration, C. Athanassopoulos et al., Phys. Rev. Lett. 77, 3082 (1996); Phys. Rev. C 58, 2489 (1998); LSND Collaboration, A. Aguilar et al., Phys. Rev. D 64, 112007 (2001).
-
(2001)
Phys. Rev. D
, vol.64
, pp. 112007
-
-
Aguilar, A.1
-
5
-
-
17644448246
-
-
Particle Data Group Collaboration
-
Particle Data Group Collaboration, K. Hagiwara et al., Phys. Rev. D 66, 010001 (2002).
-
(2002)
Phys. Rev. D
, vol.66
, pp. 010001
-
-
Hagiwara, K.1
-
6
-
-
0003609959
-
-
North-Holland, Amsterdam
-
M. Gell-Mann, P. Ramond, and R. Slansky, in Supergravity (North-Holland, Amsterdam, 1979); T. Yanagida, in Proceedings of Workshop on Unified Theories and Baryon Number in the Universe (KEK, Tsukuba, 1979); R.N. Mohapatra and G. Senjanovic, Phys. Rev. Lett. 44, 912 (1980).
-
(1979)
Supergravity
-
-
Gell-Mann, M.1
Ramond, P.2
Slansky, R.3
-
7
-
-
18044384905
-
-
KEK, Tsukuba
-
M. Gell-Mann, P. Ramond, and R. Slansky, in Supergravity (North-Holland, Amsterdam, 1979); T. Yanagida, in Proceedings of Workshop on Unified Theories and Baryon Number in the Universe (KEK, Tsukuba, 1979); R.N. Mohapatra and G. Senjanovic, Phys. Rev. Lett. 44, 912 (1980).
-
(1979)
Proceedings of Workshop on Unified Theories and Baryon Number in the Universe
-
-
Yanagida, T.1
-
8
-
-
30244555405
-
-
M. Gell-Mann, P. Ramond, and R. Slansky, in Supergravity (North-Holland, Amsterdam, 1979); T. Yanagida, in Proceedings of Workshop on Unified Theories and Baryon Number in the Universe (KEK, Tsukuba, 1979); R.N. Mohapatra and G. Senjanovic, Phys. Rev. Lett. 44, 912 (1980).
-
(1980)
Phys. Rev. Lett.
, vol.44
, pp. 912
-
-
Mohapatra, R.N.1
Senjanovic, G.2
-
10
-
-
18044390752
-
-
A.D. Dolgov, hep-ph/0306154, and references therein
-
This conclusion can be avoided, however, in the presence of a non-negligible lepton asymmetry. See, for example, A.D. Dolgov, hep-ph/0306154, and references therein.
-
-
-
-
12
-
-
0037401124
-
-
K. N. Abazajian, Astropart. Phys. 19, 303 (2003); P. Di Bari, Phys. Rev. D 67, 127301 (2003); Phys. Rev. D 65, 043509 (2002).
-
(2003)
Astropart. Phys.
, vol.19
, pp. 303
-
-
Abazajian, K.N.1
-
13
-
-
0041626224
-
-
K. N. Abazajian, Astropart. Phys. 19, 303 (2003); P. Di Bari, Phys. Rev. D 67, 127301 (2003); Phys. Rev. D 65, 043509 (2002).
-
(2003)
Phys. Rev. D
, vol.67
, pp. 127301
-
-
Di Bari, P.1
-
14
-
-
0037084873
-
-
K. N. Abazajian, Astropart. Phys. 19, 303 (2003); P. Di Bari, Phys. Rev. D 67, 127301 (2003); Phys. Rev. D 65, 043509 (2002).
-
(2002)
Phys. Rev. D
, vol.65
, pp. 043509
-
-
-
15
-
-
1642441662
-
-
A. Pierce and H. Murayama, Phys. Lett. B 581, 218 (2004); M. Cirelli, G. Marandella, A. Strumia, and F. Vissani, Nucl. Phys. B 708, 215 (2005).
-
(2004)
Phys. Lett. B
, vol.581
, pp. 218
-
-
Pierce, A.1
Murayama, H.2
-
16
-
-
12744254726
-
-
A. Pierce and H. Murayama, Phys. Lett. B 581, 218 (2004); M. Cirelli, G. Marandella, A. Strumia, and F. Vissani, Nucl. Phys. B 708, 215 (2005).
-
(2005)
Nucl. Phys. B
, vol.708
, pp. 215
-
-
Cirelli, M.1
Marandella, G.2
Strumia, A.3
Vissani, F.4
-
17
-
-
17044381941
-
-
D. N. Spergel et al., Astrophys. J. Suppl. Ser. 148, 175 (2003); W.J. Percival et al., Mon. Not. R. Astron. Soc. 327, 1297 (2001).
-
(2003)
Astrophys. J. Suppl. Ser.
, vol.148
, pp. 175
-
-
Spergel, D.N.1
-
18
-
-
0000990243
-
-
D. N. Spergel et al., Astrophys. J. Suppl. Ser. 148, 175 (2003); W.J. Percival et al., Mon. Not. R. Astron. Soc. 327, 1297 (2001).
-
(2001)
Mon. Not. R. Astron. Soc.
, vol.327
, pp. 1297
-
-
Percival, W.J.1
-
19
-
-
33646661523
-
-
SDSS Collaboration
-
eV to 1.7 eV; see SDSS Collaboration, M. Tegmark et al., Phys. Rev. D 69, 103501 (2004).
-
(2004)
Phys. Rev. D
, vol.69
, pp. 103501
-
-
Tegmark, M.1
-
20
-
-
84927759376
-
-
Z. Chacko, L.J. Hall, T. Okui, and S. J. Oliver, Phys. Rev. D 70, 085008 (2004).
-
(2004)
Phys. Rev. D
, vol.70
, pp. 085008
-
-
Chacko, Z.1
Hall, L.J.2
Okui, T.3
Oliver, S.J.4
-
21
-
-
0038842334
-
-
Models with global symmetry breaking at the weak scale have been proposed in Y. Chikashige, R.N. Mohapatra, and R. D. Peccei, Phys. Lett. B 98, 265 (1981); G. Gelmini and M. Roncadelli, Phys. Lett. B 99, 411 (1981); H. Georgi, S. Glashow, and S. Nussinov, Nucl. Phys. B 193, 297 (1981). Global symmetries have been exploited to ensure the lightness of a sterile neutrino in R.N. Mohapatra, Phys. Rev. D 64, 091301 (2001); B. Brahmachari, S. Choubey, and R.N. Mohapatra, Phys. Lett. B 536, 94 (2002).
-
(1981)
Phys. Lett. B
, vol.98
, pp. 265
-
-
Chikashige, Y.1
Mohapatra, R.N.2
Peccei, R.D.3
-
22
-
-
4243616343
-
-
Models with global symmetry breaking at the weak scale have been proposed in Y. Chikashige, R.N. Mohapatra, and R. D. Peccei, Phys. Lett. B 98, 265 (1981); G. Gelmini and M. Roncadelli, Phys. Lett. B 99, 411 (1981); H. Georgi, S. Glashow, and S. Nussinov, Nucl. Phys. B 193, 297 (1981). Global symmetries have been exploited to ensure the lightness of a sterile neutrino in R.N. Mohapatra, Phys. Rev. D 64, 091301 (2001); B. Brahmachari, S. Choubey, and R.N. Mohapatra, Phys. Lett. B 536, 94 (2002).
-
(1981)
Phys. Lett. B
, vol.99
, pp. 411
-
-
Gelmini, G.1
Roncadelli, M.2
-
23
-
-
33744734276
-
-
Models with global symmetry breaking at the weak scale have been proposed in Y. Chikashige, R.N. Mohapatra, and R. D. Peccei, Phys. Lett. B 98, 265 (1981); G. Gelmini and M. Roncadelli, Phys. Lett. B 99, 411 (1981); H. Georgi, S. Glashow, and S. Nussinov, Nucl. Phys. B 193, 297 (1981). Global symmetries have been exploited to ensure the lightness of a sterile neutrino in R.N. Mohapatra, Phys. Rev. D 64, 091301 (2001); B. Brahmachari, S. Choubey, and R.N. Mohapatra, Phys. Lett. B 536, 94 (2002).
-
(1981)
Nucl. Phys. B
, vol.193
, pp. 297
-
-
Georgi, H.1
Glashow, S.2
Nussinov, S.3
-
24
-
-
85037916911
-
-
Models with global symmetry breaking at the weak scale have been proposed in Y. Chikashige, R.N. Mohapatra, and R. D. Peccei, Phys. Lett. B 98, 265 (1981); G. Gelmini and M. Roncadelli, Phys. Lett. B 99, 411 (1981); H. Georgi, S. Glashow, and S. Nussinov, Nucl. Phys. B 193, 297 (1981). Global symmetries have been exploited to ensure the lightness of a sterile neutrino in R.N. Mohapatra, Phys. Rev. D 64, 091301 (2001); B. Brahmachari, S. Choubey, and R.N. Mohapatra, Phys. Lett. B 536, 94 (2002).
-
(2001)
Phys. Rev. D
, vol.64
, pp. 091301
-
-
Mohapatra, R.N.1
-
25
-
-
0037198613
-
-
Models with global symmetry breaking at the weak scale have been proposed in Y. Chikashige, R.N. Mohapatra, and R. D. Peccei, Phys. Lett. B 98, 265 (1981); G. Gelmini and M. Roncadelli, Phys. Lett. B 99, 411 (1981); H. Georgi, S. Glashow, and S. Nussinov, Nucl. Phys. B 193, 297 (1981). Global symmetries have been exploited to ensure the lightness of a sterile neutrino in R.N. Mohapatra, Phys. Rev. D 64, 091301 (2001); B. Brahmachari, S. Choubey, and R.N. Mohapatra, Phys. Lett. B 536, 94 (2002).
-
(2002)
Phys. Lett. B
, vol.536
, pp. 94
-
-
Brahmachari, B.1
Choubey, S.2
Mohapatra, R.N.3
-
26
-
-
18144382622
-
-
See, for example, M. Kachelriess, R. Tomas, and J. W. F. Valle, Phys. Rev. D 62, 023004 (2000).
-
(2000)
Phys. Rev. D
, vol.62
, pp. 023004
-
-
Kachelriess, M.1
Tomas, R.2
Valle, J.W.F.3
-
27
-
-
10844291885
-
-
The possibility of lepton flavor violation as an additional, non-CMB, signal is also discussed in L. J. Hall and S. J. Oliver, Nucl. Phys. B, Proc. Suppl. 137, 269 (2004).
-
(2004)
Nucl. Phys. B, Proc. Suppl.
, vol.137
, pp. 269
-
-
Hall, L.J.1
Oliver, S.J.2
-
28
-
-
0042128542
-
-
P. Crotty, J. Lesgourgues, and S. Pastor, Phys. Rev. D 67, 123005 (2003); S. Hannestad, J. Cosmol. Astropart. Phys. 05 (2003), 004; E. Pierpaoli, Mon. Not. R. Astron. Soc. 342, L63 (2003); V. Barger et al., Phys. Lett. B 566, 8 (2003).
-
(2003)
Phys. Rev. D
, vol.67
, pp. 123005
-
-
Crotty, P.1
Lesgourgues, J.2
Pastor, S.3
-
29
-
-
0042128542
-
-
P. Crotty, J. Lesgourgues, and S. Pastor, Phys. Rev. D 67, 123005 (2003); S. Hannestad, J. Cosmol. Astropart. Phys. 05 (2003), 004; E. Pierpaoli, Mon. Not. R. Astron. Soc. 342, L63 (2003); V. Barger et al., Phys. Lett. B 566, 8 (2003).
-
(2003)
J. Cosmol. Astropart. Phys.
, vol.5
, pp. 004
-
-
Hannestad, S.1
-
30
-
-
0142073748
-
-
P. Crotty, J. Lesgourgues, and S. Pastor, Phys. Rev. D 67, 123005 (2003); S. Hannestad, J. Cosmol. Astropart. Phys. 05 (2003), 004; E. Pierpaoli, Mon. Not. R. Astron. Soc. 342, L63 (2003); V. Barger et al., Phys. Lett. B 566, 8 (2003).
-
(2003)
Mon. Not. R. Astron. Soc.
, vol.342
-
-
Pierpaoli, E.1
-
31
-
-
0037819320
-
-
P. Crotty, J. Lesgourgues, and S. Pastor, Phys. Rev. D 67, 123005 (2003); S. Hannestad, J. Cosmol. Astropart. Phys. 05 (2003), 004; E. Pierpaoli, Mon. Not. R. Astron. Soc. 342, L63 (2003); V. Barger et al., Phys. Lett. B 566, 8 (2003).
-
(2003)
Phys. Lett. B
, vol.566
, pp. 8
-
-
Barger, V.1
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