Hierarchical matrices in the see-saw mechanism, large neutrino mixing and leptogenesis

European Physical Journal C

Volumn 32, Issue 2, 2004, Pages 235-243

  Rodejohann, W ^a  

^a SEZIONE DI TRIESTE   (Italy)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 2442463541     PISSN: 14346044     EISSN: None     Source Type: Journal    
DOI: 10.1140/epjc/s2003-01400-5     Document Type: Article

References (70)

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44. CP has also been analyzed in C.W. Chiang, Phys. Rev. D 63, 076009 (2001)
45. CP has also been analyzed in C.W. Chiang, Phys. Rev. D 63, 076009 (2001)
46. CP has also been analyzed in C.W. Chiang, Phys. Rev. D 63, 076009 (2001)
47. CP has also been analyzed in C.W. Chiang, Phys. Rev. D 63, 076009 (2001)
48. See, e.g., M. Lindner, Invited talk at XXth International Conference on Neutrino Physics and Astrophysics (Neutrino 2002), Munich, Germany, 25-30 May 2002, hep-ph/0210377 and references therein
49. e3 through radiative corrections are in A.S. Joshipura, Phys. Lett. B 543, 276 (2002); R.N. Mohapatra, M.K. Parida, G. Rajasekaran, hep-ph/0301234; in the type II see-saw mechanism: H.S. Goh, R.N. Mohapatra, S.P. Ng, Phys. Lett. B 570, 215 (2003); for Fritzsch type mass matrices: M. Fukugita, M. Tanimoto, T. Yanagida, Phys. Lett. B 562, 273 (2003); from physics above the GUT scale: F. Vissani, M. Narayan, V. Berezinsky, hep-ph/0305233; see also the reviews S.M. Barr, I. Dorsner, Nucl. Phys. B 585, 79 (2000); M. Tanimoto, hep-ph/0305274 and references therein
50. e3 through radiative corrections are in A.S. Joshipura, Phys. Lett. B 543, 276 (2002); R.N. Mohapatra, M.K. Parida, G. Rajasekaran, hep-ph/0301234; in the type II see-saw mechanism: H.S. Goh, R.N. Mohapatra, S.P. Ng, Phys. Lett. B 570, 215 (2003); for Fritzsch type mass matrices: M. Fukugita, M. Tanimoto, T. Yanagida, Phys. Lett. B 562, 273 (2003); from physics above the GUT scale: F. Vissani, M. Narayan, V. Berezinsky, hep-ph/0305233; see also the reviews S.M. Barr, I. Dorsner, Nucl. Phys. B 585, 79 (2000); M. Tanimoto, hep-ph/0305274 and references therein
51. e3 through radiative corrections are in A.S. Joshipura, Phys. Lett. B 543, 276 (2002); R.N. Mohapatra, M.K. Parida, G. Rajasekaran, hep-ph/0301234; in the type II see-saw mechanism: H.S. Goh, R.N. Mohapatra, S.P. Ng, Phys. Lett. B 570, 215 (2003); for Fritzsch type mass matrices: M. Fukugita, M. Tanimoto, T. Yanagida, Phys. Lett. B 562, 273 (2003); from physics above the GUT scale: F. Vissani, M. Narayan, V. Berezinsky, hep-ph/0305233; see also the reviews S.M. Barr, I. Dorsner, Nucl. Phys. B 585, 79 (2000); M. Tanimoto, hep-ph/0305274 and references therein
52. e3 through radiative corrections are in A.S. Joshipura, Phys. Lett. B 543, 276 (2002); R.N. Mohapatra, M.K. Parida, G. Rajasekaran, hep-ph/0301234; in the type II see-saw mechanism: H.S. Goh, R.N. Mohapatra, S.P. Ng, Phys. Lett. B 570, 215 (2003); for Fritzsch type mass matrices: M. Fukugita, M. Tanimoto, T. Yanagida, Phys. Lett. B 562, 273 (2003); from physics above the GUT scale: F. Vissani, M. Narayan, V. Berezinsky, hep-ph/0305233; see also the reviews S.M. Barr, I. Dorsner, Nucl. Phys. B 585, 79 (2000); M. Tanimoto, hep-ph/0305274 and references therein
53. e3 through radiative corrections are in A.S. Joshipura, Phys. Lett. B 543, 276 (2002); R.N. Mohapatra, M.K. Parida, G. Rajasekaran, hep-ph/0301234; in the type II see-saw mechanism: H.S. Goh, R.N. Mohapatra, S.P. Ng, Phys. Lett. B 570, 215 (2003); for Fritzsch type mass matrices: M. Fukugita, M. Tanimoto, T. Yanagida, Phys. Lett. B 562, 273 (2003); from physics above the GUT scale: F. Vissani, M. Narayan, V. Berezinsky, hep-ph/0305233; see also the reviews S.M. Barr, I. Dorsner, Nucl. Phys. B 585, 79 (2000); M. Tanimoto, hep-ph/0305274 and references therein
54. e3 through radiative corrections are in A.S. Joshipura, Phys. Lett. B 543, 276 (2002); R.N. Mohapatra, M.K. Parida, G. Rajasekaran, hep-ph/0301234; in the type II see-saw mechanism: H.S. Goh, R.N. Mohapatra, S.P. Ng, Phys. Lett. B 570, 215 (2003); for Fritzsch type mass matrices: M. Fukugita, M. Tanimoto, T. Yanagida, Phys. Lett. B 562, 273 (2003); from physics above the GUT scale: F. Vissani, M. Narayan, V. Berezinsky, hep-ph/0305233; see also the reviews S.M. Barr, I. Dorsner, Nucl. Phys. B 585, 79 (2000); M. Tanimoto, hep-ph/0305274 and references therein
55. e3 through radiative corrections are in A.S. Joshipura, Phys. Lett. B 543, 276 (2002); R.N. Mohapatra, M.K. Parida, G. Rajasekaran, hep-ph/0301234; in the type II see-saw mechanism: H.S. Goh, R.N. Mohapatra, S.P. Ng, Phys. Lett. B 570, 215 (2003); for Fritzsch type mass matrices: M. Fukugita, M. Tanimoto, T. Yanagida, Phys. Lett. B 562, 273 (2003); from physics above the GUT scale: F. Vissani, M. Narayan, V. Berezinsky, hep-ph/0305233; see also the reviews S.M. Barr, I. Dorsner, Nucl. Phys. B 585, 79 (2000); M. Tanimoto, hep-ph/0305274 and references therein
56. See, e.g., A.S. Joshipura, E.A. Paschos, W. Rodejohann, JHEP 08, 029 (2001); W. Buchmüller, D. Wyler, Phys. Lett. B 521, 291 (2001); G.C. Branco et al., Nucl. Phys. B 640, 202 (2002); H.B. Nielsen, Y. Takanishi, Nucl. Phys. B 636, 305 (2002); J. Ellis, M. Raidal, Nucl. Phys. B 643, 229 (2002). Z.Z. Xing, Phys. Lett. B 545, 352 (2002); S. Davidson, A. Ibarra, Nucl. Phys. B 648, 345 (2003); W. Rodejohann, Phys. Lett. B 542, 100 (2002); T. Endoh et al., Phys. Rev. Lett. 89, 231601 (2002); S.F. King, Phys. Rev. D 67, 113010 (2003); S. Kaneko, M. Katsumata, M. Tanimoto, JHEP 0307, 025 (2003); L. Velasco-Sevilla, hep-ph/0307071.
57. See, e.g., A.S. Joshipura, E.A. Paschos, W. Rodejohann, JHEP 08, 029 (2001); W. Buchmüller, D. Wyler, Phys. Lett. B 521, 291 (2001); G.C. Branco et al., Nucl. Phys. B 640, 202 (2002); H.B. Nielsen, Y. Takanishi, Nucl. Phys. B 636, 305 (2002); J. Ellis, M. Raidal, Nucl. Phys. B 643, 229 (2002). Z.Z. Xing, Phys. Lett. B 545, 352 (2002); S. Davidson, A. Ibarra, Nucl. Phys. B 648, 345 (2003); W. Rodejohann, Phys. Lett. B 542, 100 (2002); T. Endoh et al., Phys. Rev. Lett. 89, 231601 (2002); S.F. King, Phys. Rev. D 67, 113010 (2003); S. Kaneko, M. Katsumata, M. Tanimoto, JHEP 0307, 025 (2003); L. Velasco-Sevilla, hep-ph/0307071.
58. See, e.g., A.S. Joshipura, E.A. Paschos, W. Rodejohann, JHEP 08, 029 (2001); W. Buchmüller, D. Wyler, Phys. Lett. B 521, 291 (2001); G.C. Branco et al., Nucl. Phys. B 640, 202 (2002); H.B. Nielsen, Y. Takanishi, Nucl. Phys. B 636, 305 (2002); J. Ellis, M. Raidal, Nucl. Phys. B 643, 229 (2002). Z.Z. Xing, Phys. Lett. B 545, 352 (2002); S. Davidson, A. Ibarra, Nucl. Phys. B 648, 345 (2003); W. Rodejohann, Phys. Lett. B 542, 100 (2002); T. Endoh et al., Phys. Rev. Lett. 89, 231601 (2002); S.F. King, Phys. Rev. D 67, 113010 (2003); S. Kaneko, M. Katsumata, M. Tanimoto, JHEP 0307, 025 (2003); L. Velasco-Sevilla, hep-ph/0307071.
59. See, e.g., A.S. Joshipura, E.A. Paschos, W. Rodejohann, JHEP 08, 029 (2001); W. Buchmüller, D. Wyler, Phys. Lett. B 521, 291 (2001); G.C. Branco et al., Nucl. Phys. B 640, 202 (2002); H.B. Nielsen, Y. Takanishi, Nucl. Phys. B 636, 305 (2002); J. Ellis, M. Raidal, Nucl. Phys. B 643, 229 (2002). Z.Z. Xing, Phys. Lett. B 545, 352 (2002); S. Davidson, A. Ibarra, Nucl. Phys. B 648, 345 (2003); W. Rodejohann, Phys. Lett. B 542, 100 (2002); T. Endoh et al., Phys. Rev. Lett. 89, 231601 (2002); S.F. King, Phys. Rev. D 67, 113010 (2003); S. Kaneko, M. Katsumata, M. Tanimoto, JHEP 0307, 025 (2003); L. Velasco-Sevilla, hep-ph/0307071.
60. See, e.g., A.S. Joshipura, E.A. Paschos, W. Rodejohann, JHEP 08, 029 (2001); W. Buchmüller, D. Wyler, Phys. Lett. B 521, 291 (2001); G.C. Branco et al., Nucl. Phys. B 640, 202 (2002); H.B. Nielsen, Y. Takanishi, Nucl. Phys. B 636, 305 (2002); J. Ellis, M. Raidal, Nucl. Phys. B 643, 229 (2002). Z.Z. Xing, Phys. Lett. B 545, 352 (2002); S. Davidson, A. Ibarra, Nucl. Phys. B 648, 345 (2003); W. Rodejohann, Phys. Lett. B 542, 100 (2002); T. Endoh et al., Phys. Rev. Lett. 89, 231601 (2002); S.F. King, Phys. Rev. D 67, 113010 (2003); S. Kaneko, M. Katsumata, M. Tanimoto, JHEP 0307, 025 (2003); L. Velasco-Sevilla, hep-ph/0307071.
61. See, e.g., A.S. Joshipura, E.A. Paschos, W. Rodejohann, JHEP 08, 029 (2001); W. Buchmüller, D. Wyler, Phys. Lett. B 521, 291 (2001); G.C. Branco et al., Nucl. Phys. B 640, 202 (2002); H.B. Nielsen, Y. Takanishi, Nucl. Phys. B 636, 305 (2002); J. Ellis, M. Raidal, Nucl. Phys. B 643, 229 (2002). Z.Z. Xing, Phys. Lett. B 545, 352 (2002); S. Davidson, A. Ibarra, Nucl. Phys. B 648, 345 (2003); W. Rodejohann, Phys. Lett. B 542, 100 (2002); T. Endoh et al., Phys. Rev. Lett. 89, 231601 (2002); S.F. King, Phys. Rev. D 67, 113010 (2003); S. Kaneko, M. Katsumata, M. Tanimoto, JHEP 0307, 025 (2003); L. Velasco-Sevilla, hep-ph/0307071.
62. See, e.g., A.S. Joshipura, E.A. Paschos, W. Rodejohann, JHEP 08, 029 (2001); W. Buchmüller, D. Wyler, Phys. Lett. B 521, 291 (2001); G.C. Branco et al., Nucl. Phys. B 640, 202 (2002); H.B. Nielsen, Y. Takanishi, Nucl. Phys. B 636, 305 (2002); J. Ellis, M. Raidal, Nucl. Phys. B 643, 229 (2002). Z.Z. Xing, Phys. Lett. B 545, 352 (2002); S. Davidson, A. Ibarra, Nucl. Phys. B 648, 345 (2003); W. Rodejohann, Phys. Lett. B 542, 100 (2002); T. Endoh et al., Phys. Rev. Lett. 89, 231601 (2002); S.F. King, Phys. Rev. D 67, 113010 (2003); S. Kaneko, M. Katsumata, M. Tanimoto, JHEP 0307, 025 (2003); L. Velasco-Sevilla, hep-ph/0307071.
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