-
1
-
-
33847037819
-
-
Atmospheric data: see. Super-Kamiokande Collaboration. hep-ex/0604011
-
Atmospheric data: see. Super-Kamiokande Collaboration. hep-ex/0604011
-
-
-
-
2
-
-
33847010105
-
-
K2K Collaboration. hep-ex/0606032
-
K2K Collaboration. hep-ex/0606032
-
-
-
-
3
-
-
33847027571
-
-
MINOS Collaboration. hep-ex/0607088
-
MINOS Collaboration. hep-ex/0607088
-
-
-
-
4
-
-
18144427171
-
-
Solar data: see. KamLAND Collaboration. hep-ex/0406035
-
Solar data: see. KamLAND Collaboration. Phys. Rev. Lett. 94 (2005) 081801. hep-ex/0406035
-
(2005)
Phys. Rev. Lett.
, vol.94
, pp. 081801
-
-
-
5
-
-
33847065765
-
-
SNO Collaboration. nucl-ex/0610020
-
SNO Collaboration. nucl-ex/0610020
-
-
-
-
6
-
-
33847079776
-
-
See-saw models with 2 right-handed neutrinos have been often considered because they are more predictive than models with 3 right-handed neutrinos. See A. Kleppe, in: Lohusalu 1995, Neutrino Physics, 118-125
-
-
-
-
13
-
-
1242271398
-
-
hep-ph/0310326
-
Guo W., and Xing Z. Phys. Lett. B 583 (2004) 163. hep-ph/0310326
-
(2004)
Phys. Lett. B
, vol.583
, pp. 163
-
-
Guo, W.1
Xing, Z.2
-
15
-
-
0037011685
-
-
hep-ph/0209020
-
Endoh T., Kaneko S., Kang S., Morozumi T., and Tanimoto M. Phys. Rev. Lett. 89 (2002) 231601. hep-ph/0209020
-
(2002)
Phys. Rev. Lett.
, vol.89
, pp. 231601
-
-
Endoh, T.1
Kaneko, S.2
Kang, S.3
Morozumi, T.4
Tanimoto, M.5
-
17
-
-
33845603076
-
-
hep-ph/0511136 In string models the number of right-handed neutrinos (defined as SM gauge singlets that couple to LH) is not generically equal to the number of generations, and right-handed neutrino masses (possibly generated by non-perturbative effects in supersymmetric models) can be anywhere below the string scale. However, the fact that the models we are considering arise in string theory could be simply due to the huge number of different string compactifications
-
Ibarra A. JHEP 0601 (2006) 064. hep-ph/0511136 In string models the number of right-handed neutrinos (defined as SM gauge singlets that couple to LH) is not generically equal to the number of generations, and right-handed neutrino masses (possibly generated by non-perturbative effects in supersymmetric models) can be anywhere below the string scale. However, the fact that the models we are considering arise in string theory could be simply due to the huge number of different string compactifications
-
(2006)
JHEP
, vol.601
, pp. 064
-
-
Ibarra, A.1
-
24
-
-
4243440412
-
-
explored the possibility that small neutrino masses arise radiatively from one weak-scale right-handed neutrino within a four-generation version of the SM
-
Babu K.S., and Ma E. Phys. Rev. Lett. 61 (1988) 674 explored the possibility that small neutrino masses arise radiatively from one weak-scale right-handed neutrino within a four-generation version of the SM
-
(1988)
Phys. Rev. Lett.
, vol.61
, pp. 674
-
-
Babu, K.S.1
Ma, E.2
-
28
-
-
0035500307
-
-
An error has been corrected in. hep-ph/0108005
-
An error has been corrected in. Antusch S., Drees M., Kersten J., Lindner M., and Ratz M. Phys. Lett. B 519 (2001) 238. hep-ph/0108005
-
(2001)
Phys. Lett. B
, vol.519
, pp. 238
-
-
Antusch, S.1
Drees, M.2
Kersten, J.3
Lindner, M.4
Ratz, M.5
-
31
-
-
27344455443
-
-
RGE equations in the MSSM are summarized in. hep-ph/0501272
-
RGE equations in the MSSM are summarized in. Antush S., Kersten J., Lindner M., Ratz M., and Schmidt M.A. JHEP 0503 (2005) 024. hep-ph/0501272
-
(2005)
JHEP
, vol.503
, pp. 024
-
-
Antush, S.1
Kersten, J.2
Lindner, M.3
Ratz, M.4
Schmidt, M.A.5
-
34
-
-
33646627507
-
-
hep-ph/9401241
-
Yamada Y. Phys. Rev. D 50 (1994) 3537. hep-ph/9401241
-
(1994)
Phys. Rev. D
, vol.50
, pp. 3537
-
-
Yamada, Y.1
-
37
-
-
0001244282
-
-
For a clear presentation of the superfield tecniques that we employ at one-loop level see. hep-ph/9709397
-
For a clear presentation of the superfield tecniques that we employ at one-loop level see. Avdeev L., Kazakov D., and Kondrashuk I. Nucl. Phys. B 510 (1998) 289. hep-ph/9709397
-
(1998)
Nucl. Phys. B
, vol.510
, pp. 289
-
-
Avdeev, L.1
Kazakov, D.2
Kondrashuk, I.3
-
38
-
-
0030599630
-
-
hep-ph/9604417
-
Strumia A. Nucl. Phys. B 482 (1996) 24. hep-ph/9604417
-
(1996)
Nucl. Phys. B
, vol.482
, pp. 24
-
-
Strumia, A.1
|