• [1]

    The LEP Collaborations, the LEP Electroweak Working Group, and the SLD Heavy Flavor and Electroweak Groups. CERN-EP/2003-091, arXiv: hep-ex/0312023[2] Filipuzzi A, Gonzalez-Alonso M, Portoles J. Phys. Rev. D, 2012, 85: 116010[3] Abada A, Das D, Teixeira A M, Vicente A, Weiland C. arXiv: 1211.3052[hep-ph][4] HOU Wei-Shu. Phys. Rev. D, 1993, 48: 2342[5] Lopez-Val D, Sola J. arXiv:1211.0311 [hep-ph][6] Masiero A, Paradisi P, Petronzio R. Phys. Rev. D, 2006, 74: 011701; Masiero A, Paradisi P, Petronzio R. JHEP, 2008, 0811: 042; Ellis J, Lola S, Raidal M, Nucl. Phys. B, 2009, 812: 128; Girrbach J, Nierste U. arXiv:1202.4906 [hep-ph]; Fonseca R M, Romao J C, Teixeira A M. Eur. Phys. J. C, 2012, 72: 2228[7] Minkowski P. Phys. Lett. B, 1977, 67: 421; Yanagida T. In: Proc. of the Workshop on Unifed Theory and the Baryon Number of the Universe. Sawada O Sugamoto A. Tsukuba: KEK, 1979. 95; Gell-Mann M, Ramond P, Slansky R. Supergravity. Amsterdam: North-Holland, 1979. 315; Glashow S L. Quarks and Leptons. New York: Plenum, 1980. 707; Mohapatra R N, Senjanovic G. Phys. Rev. Lett., 1980, 44: 912[8] XING Zhi-Zhong, ZHOU Shun. Neutrinos in Particle Physics, Astronomy and Cosmology. Zhejiang University Press and Springer-Verlag, 2011[9] Wyler D, Wolfenstein L. Nucl. Phys. B, 1983, 218: 205; Mohapatra R N, Valle J W F. Phys. Rev. D, 1986, 34: 1642; Ma E. Phys. Lett. B, 1987, 191: 287[10] Aguilar A et al. (LSND collaboration). Phys. Rev. D, 2001, 64: 112007[11] Aguilar-Arevalo A A et al. (MiniBooNE collaboration). Phys. Rev. Lett., 2010, 105: 181801[12] Mueller Th A et al. Phys. Rev. C, 2011, 83: 054615[13] Anselmann P et al. (GALLEX collaboration.). Phys. Lett. B, 1995, 342: 440; Hampel W et al. (GALLEX collaboration). Phys. Lett. B, 1998, 420: 114; Kaether F et al. Phys. Lett. B, 2010, 685: 47[14] Abdurashitov D et al. Phys. Rev. Lett., 1996, 77: 4708; Abdurashitov J et al. (SAGE collaboration). Phys. Rev. C, 1999, 59: 2246; Abdurashitov J et al. Phys. Rev. C, 2006, 73: 045805; Abdurashitov J et al. (SAGE collaboration). Phys. Rev. C, 2009, 80: 015807[15] ZHAO Gong-Bo et al. arXiv:1211.3741 [astro-ph.CO][16] Goudzovski E. (NA48/2 and NA62 collaborations). arXiv:1111.2818 [hep-ex][17] Balev S. arXiv:1006.1201 [hep-ex][18] Abazajian K N et al. arXiv:1204.5379 [hep-ph][19] Pontecorvo B. Zh. Eksp. Theor. Fiz., 1957, 33: 549; Pontecorvo B. Zh. Eksp. Theor. Fiz., 1958, 34: 247[20] Maki Z, Nakagawa M, Sakata S. Prog. Theor. Phys., 1962, 28: 870[21] Antusch S et al. JHEP, 2006, 0610: 084[22] XING Zhi-Zhong. arXiv: 1210.1523[hep-ph][23] Beringer J et al. (Particle Data Group). Phys. Rev. D, 2012, 86: 010001[24] Mohanta R. Eur. Phys. J. C, 2011, 71: 1625[25] Aubert B et al. (The BABAR collaboration). arXiv: 0912.2453 [hep-ex][26] Crivellin A, Kokulu A, Greub C. arXiv:1303.5877 [hep-ph][27] Heister A et al. (ALEPH collaboration). Phys. Lett. B, 2002, 528: 1[28] Abbiendi G et al. (OPAL collaboration). Phys. Lett. B, 2001, 516: 236[29] Acciarri M et al. (L3 collaboration). Phys. Lett. B, 1997, 396: 327[30] del Amo Sanchez P et al. (Babar collaboration). Phys. Rev. D, 2010, 82: 091103[31] Widhalm L et al. (BELLE collaboration). Phys. Rev. Lett., 2008, 100: 241801[32] Bonvicini G et al. (CLEO collaboration). Phys. Rev. D, 2004, 70: 112004; Artuso M et al. (CLEO collaboration). Phys. Rev. Lett., 2005, 95: 251801; Rubin P et al. (CLEO collaboration). Phys. Rev. D, 2006, 73: 112005; Pedlar T K et al. (CLEO collaboration). Phys. Rev. D, 2007, 76: 072002; Eisenstein B I et al. (CLEO collaboration). Phys. Rev. D, 2008, 78: 052003; Ecklund K M et al. (CLEO collaboration). Phys. Rev. Lett., 2008, 100: 161801; Alexander J P et al. (CLEO collaboration). Phys. Rev. D, 2009, 79: 052001; Onyisi P U E et al. (CLEO collaboration). Phys. Rev. D, 2009, 79: 052002; Naik P et al. (CLEO collaboration). Phys. Rev. D, 2009, 80: 112004[33] BAI J Z et al. (BES collaboration). Phys. Rev. Lett., 1995, 74: 4599; Bai J Z et al. (BES collaboration). Phys. Lett. B, 1998, 492: 188; Ablikim M et al. (BESIII collaboration). Phys. Lett. B, 2005, 610: 183[34] LI W D et al. The Offine Software for the BES Experiment. Proceeding of CHEP06. Mumbai, India 13-17 Febuary 2006[35] Agostinelli S et al. (Geant4 collaboration), Nucl. Instrum. Meth. A, 2003, 506: 250[36] DENG Z Y et al. High Energy Phys. Nucl. Phys., 2003, 30: 250[37] Ablikim M et al (BESIII collaboration). Nucl. Instrum. Methods A, 2010, 614: 345[38] Ablikim M et al. (BES collaboration). Phys. Lett. B, 2004, 603: 130[39] BAI J Z et al. (BES collaboration). Phys. Rev. D, 2000, 62: 012002[40] Feldman G J, Cousins R D. Phys. Rev. D, 1998, 57: 3873[41] Mohapatra R N, Smirnov A Yu. Ann. Rev. Nucl. Part. Sci., 2006, 56: 569; GE Shao-Feng, HE Hong-Jian, YIN Fu-Rong. JCAP, 2010, 1005: 017; HE Hong-Jian, YIN Fu-Rong. Phys. Rev. D, 2011, 84: 033009; Adhikary B, Ghosal A, Roy P. arXiv:1210.5328 [hep-ph]