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Volumn 35, Issue 9, 2004, Pages 2241-2248

Can one of three righthanded neutrinos be light enough to produce a small LSND effect?

Author keywords

[No Author keywords available]

Indexed keywords

LSND EFFECT; MASS MATRIX; MASS SPECTRUM; SOFT SEESAW MECHANISM;

EID: 4444383039     PISSN: 05874254     EISSN: None     Source Type: Conference Proceeding    
DOI: None     Document Type: Article
Times cited : (6)

References (24)
  • 1
    • 37649032191 scopus 로고    scopus 로고
    • nucl-ex/0309004
    • Q.R. Ahmad et al. (SNO Collaboration), Phys. Rev. Lett. 87, 071301 (2001); nucl-ex/0309004.
    • (2001) Phys. Rev. Lett. , vol.87 , pp. 071301
    • Ahmad, Q.R.1
  • 2
    • 4243741631 scopus 로고    scopus 로고
    • Y. Fukuda et al. (SuperKamiokande Collaboration), Phys. Rev. Lett. 81, 1562 (1998); Phys. Lett. B467, 185 (1999).
    • (1998) Phys. Rev. Lett. , vol.81 , pp. 1562
    • Fukuda, Y.1
  • 3
    • 0142146981 scopus 로고    scopus 로고
    • Y. Fukuda et al. (SuperKamiokande Collaboration), Phys. Rev. Lett. 81, 1562 (1998); Phys. Lett. B467, 185 (1999).
    • (1999) Phys. Lett. , vol.B467 , pp. 185
  • 4
    • 0037473863 scopus 로고    scopus 로고
    • M.H. Ahn et al. (K2K Collaboration), Phys. Rev. Lett. 90, 041801 (2003).
    • (2003) Phys. Rev. Lett. , vol.90 , pp. 041801
    • Ahn, M.H.1
  • 5
    • 0037449922 scopus 로고    scopus 로고
    • K. Eguchi et al. (KamLAND Collaboration), Phys. Rev. Lett. 90, 021802 (2003).
    • (2003) Phys. Rev. Lett. , vol.90 , pp. 021802
    • Eguchi, K.1
  • 7
    • 0346538980 scopus 로고    scopus 로고
    • M. Maltoni, hep-ph/0401042; and references therein
    • For a recent review cf. V. Barger, D. Marfatia, K. Whisnant, Int. J. Mod. Phys. E12, 569 (2003); M. Maltoni, hep-ph/0401042; and references therein.
  • 8
    • 0037397559 scopus 로고    scopus 로고
    • M. Apollonio et al (Chooz Collaboration), Eur. Phys. J. C27, 331 (2003).
    • (2003) Eur. Phys. J. , vol.C27 , pp. 331
    • Apollonio, M.1
  • 9
    • 4244086361 scopus 로고    scopus 로고
    • C. Athanassopoulos et al. (LSND Collaboration), Phys. Rev. Lett. 77, 3082 (1996); Phys. Rev. C58, 2489 (1998); A. Aguilar et al., Phys. Rev. D64, 112007 (2001).
    • (1996) Phys. Rev. Lett. , vol.77 , pp. 3082
    • Athanassopoulos, C.1
  • 10
    • 4244095288 scopus 로고    scopus 로고
    • C. Athanassopoulos et al. (LSND Collaboration), Phys. Rev. Lett. 77, 3082 (1996); Phys. Rev. C58, 2489 (1998); A. Aguilar et al., Phys. Rev. D64, 112007 (2001).
    • (1998) Phys. Rev. , vol.C58 , pp. 2489
  • 11
    • 0035584191 scopus 로고    scopus 로고
    • C. Athanassopoulos et al. (LSND Collaboration), Phys. Rev. Lett. 77, 3082 (1996); Phys. Rev. C58, 2489 (1998); A. Aguilar et al., Phys. Rev. D64, 112007 (2001).
    • (2001) Phys. Rev. , vol.D64 , pp. 112007
    • Aguilar, A.1
  • 12
    • 2442693707 scopus 로고    scopus 로고
    • H. Murayama, T. Yanagida, Phys. Rev. B52, 263 (2001); G. Borenboim, L. Borissov, J. Lykken, A.Y. Smirnov, J. High Energy Phys. 0210, 001 (2002); G. Borenboim, L. Borissov, J. Lykken, hep-ph/0212116.
    • (2001) Phys. Rev. , vol.B52 , pp. 263
    • Murayama, H.1    Yanagida, T.2
  • 14
    • 4444346503 scopus 로고    scopus 로고
    • G. Borenboim, L. Borissov, J. Lykken, hep-ph/0212116
    • H. Murayama, T. Yanagida, Phys. Rev. B52, 263 (2001); G. Borenboim, L. Borissov, J. Lykken, A.Y. Smirnov, J. High Energy Phys. 0210, 001 (2002); G. Borenboim, L. Borissov, J. Lykken, hep-ph/0212116.
  • 15
    • 4444338362 scopus 로고    scopus 로고
    • A.O. Bazarko et al., hep-ex/9906003
    • A.O. Bazarko et al., hep-ex/9906003.
  • 16
    • 1542575352 scopus 로고    scopus 로고
    • V. Barger, S. Pakvasa, T.J. Weiler, K. Whisnant, Phys. Rev. D58, 093016 (1998); Phys. Lett. B437, 107 (1998); M. Maltoni, T. Schwetz, M.A. Tortola, J.W. Valle, Nucl. Phys. B643, 321 (2002) and references therein.
    • (1998) Phys. Rev. , vol.D58 , pp. 093016
    • Barger, V.1    Pakvasa, S.2    Weiler, T.J.3    Whisnant, K.4
  • 17
    • 0000448373 scopus 로고    scopus 로고
    • V. Barger, S. Pakvasa, T.J. Weiler, K. Whisnant, Phys. Rev. D58, 093016 (1998); Phys. Lett. B437, 107 (1998); M. Maltoni, T. Schwetz, M.A. Tortola, J.W. Valle, Nucl. Phys. B643, 321 (2002) and references therein.
    • (1998) Phys. Lett. , vol.B437 , pp. 107
  • 18
    • 0037020777 scopus 로고    scopus 로고
    • and references therein
    • V. Barger, S. Pakvasa, T.J. Weiler, K. Whisnant, Phys. Rev. D58, 093016 (1998); Phys. Lett. B437, 107 (1998); M. Maltoni, T. Schwetz, M.A. Tortola, J.W. Valle, Nucl. Phys. B643, 321 (2002) and references therein.
    • (2002) Nucl. Phys. , vol.B643 , pp. 321
    • Maltoni, M.1    Schwetz, T.2    Tortola, M.A.3    Valle, J.W.4
  • 19
    • 4444310472 scopus 로고    scopus 로고
    • M. Sorel, J. Conrad, M. Shaevitz, hep-ph/0305255
    • M. Sorel, J. Conrad, M. Shaevitz, hep-ph/0305255.
  • 20
    • 2442698984 scopus 로고    scopus 로고
    • W. Królikowski, Acta Phys. Pol. B 35, 1675 (2004). This reference implies that in Nature, beside three generations of leptons and quarks (SM (15+1)-plets), there are exactly two light sterile neutrinos (extra SM singlets); for a theoretical background cf. W. Królikowski, Acta Phys. Pol. B 30, 227 (1999), Appendix; also Acta Phys. Pol. B 33, 2559 (2002), where a potential solution of the three-generation puzzle for leptons and quarks is described in some details. In the present paper that is an alternative for Ref. [12], these two singlets are assumed to be completely decoupled from the Standard Model and so, practically invisible, forming a kind of dark matter, observable only through gravitational interaction.
    • (2004) Acta Phys. Pol. B , vol.35 , pp. 1675
    • Królikowski, W.1
  • 21
    • 0000541758 scopus 로고    scopus 로고
    • Appendix
    • W. Królikowski, Acta Phys. Pol. B 35, 1675 (2004). This reference implies that in Nature, beside three generations of leptons and quarks (SM (15+1)-plets), there are exactly two light sterile neutrinos (extra SM singlets); for a theoretical background cf. W. Królikowski, Acta Phys. Pol. B 30, 227 (1999), Appendix; also Acta Phys. Pol. B 33, 2559 (2002), where a potential solution of the three-generation puzzle for leptons and quarks is described in some details. In the present paper that is an alternative for Ref. [12], these two singlets are assumed to be completely decoupled from the Standard Model and so, practically invisible, forming a kind of dark matter, observable only through gravitational interaction.
    • (1999) Acta Phys. Pol. B , vol.30 , pp. 227
    • Królikowski, W.1
  • 22
    • 31244433457 scopus 로고    scopus 로고
    • W. Królikowski, Acta Phys. Pol. B 35, 1675 (2004). This reference implies that in Nature, beside three generations of leptons and quarks (SM (15+1)-plets), there are exactly two light sterile neutrinos (extra SM singlets); for a theoretical background cf. W. Królikowski, Acta Phys. Pol. B 30, 227 (1999), Appendix; also Acta Phys. Pol. B 33, 2559 (2002), where a potential solution of the three-generation puzzle for leptons and quarks is described in some details. In the present paper that is an alternative for Ref. [12], these two singlets are assumed to be completely decoupled from the Standard Model and so, practically invisible, forming a kind of dark matter, observable only through gravitational interaction.
    • (2002) Acta Phys. Pol. B , vol.33 , pp. 2559
  • 23
    • 85037916911 scopus 로고    scopus 로고
    • R.N. Mohapatra, Phys. Rev. D64, 091301 (2001); B. Brahmachari, S. Choubey, R.N. Mohapatra Phys. Lett. B536, 94 (2002).
    • (2001) Phys. Rev. , vol.D64 , pp. 091301
    • Mohapatra, R.N.1


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