Implications of 4 texture zeros mass matrices for neutrino anomalies

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 57, Issue 7, 1998, Pages 3971-3976

  Gill, P S ^a,b   Gupta, Manmohan ^a  

^a PANJAB UNIVERSITY   (India)

^b Sri Guru Gobind Singh College   (India)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0000309745     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.57.3971     Document Type: Article

References (80)

1. B. T. Cleveland, in Neutrino 94, Proceedings of the 16th International Conference on Neutrino Physics and Astrophysics, Eilat, Israel, edited by A. Dar et al. [Nucl. Phys. (Proc. Suppl.) 38, 47 (1995)].
2. Kamiokande Collaboration, Y. Suzuki, in Neutrino 94 1, p. 54.
3. Gallex Collaboration, P. Anselmann, Phys. Lett. B 327, 377 (1994).
4. SAGE Collaboration, J. N. Abdurashitov et al., in Neutrino 94 1, p. 60.
5. J. N. Bahcall and M. H. Pinsonneault, Rev. Mod. Phys. 64, 885 (1992).
6. S. Turck-Chieze and I. Lopes, Astrophys. J. 408, 347 (1993).
7. Kamiokande Collaboration, Y. Fukuda, Phys. Lett. B 335, 237 (1994).
8. IMB Collaboration, D. Casper, Phys. Rev. Lett. 66, 2561 (1991).
9. NUSEX Collaboration, M. Aglietta, Europhys. Lett. 8, 611 (1989).
10. SOUDAN 2 Collaboration, M. Goodman et al., in Neutrino 94 1, p. 337.
11. LSND Collaboration, C. Anthanassopoulos, Phys. Rev. Lett. 75, 2650 (1995);
12. C. Anthanassopoulosnucl-ex/965001 (1996).
13. J. E. Hill, Phys. Rev. Lett. 75, 2654 (1995).
14. J. N. Bahcall, Astrophys. J. 467, 475 (1996), and references therein.
15. A. Acker, Phys. Lett. B 372, 265 (1993);
16. Phys. Lett. BH. Fritzsch and Z. Z. Xing, 372, 265 (1996);
17. K. Kang, S. K. Kang, J. E. Kim, and P. Ko, Mod. Phys. Lett. A 12, 1175 (1997).
18. The term texture zeros has been used in the sense of P. Ramond, Nucl. Phys. B406, 19 (1993). For example, texture four zeros corresponds to the no. of diagonal zeros plus half of the symmetrically placed off diagonal zeros in U and D type mass matrices considered in Eq. (1).
19. P. S. Gill and M. Gupta, PU-PHY-
20. D. Du and Z. Z. Xing, Phys. Rev. D 48, 2349 (1993);
21. H. Fritzsch and Z. Z. Xing, Phys. Lett. B 353, 95 (1995);
22. P. S. Gill and M. Gupta, Pramana, J. Phys. 45, 333 (1995);
23. P. S. GillM. GuptaJ. Phys. G 23, 335 (1997);
24. P. S. GillM. GuptaPhys. Rev. D 56, 3143 (1997);
25. Phys. Rev. DK. Kang, S. K. Kang, J. E. Kim, and P. Ko, 56, 1511 (1997).
26. CDF Collaboration, F. Abe, Phys. Rev. D 50, 2966 (1994);
27. F. AbePhys. Rev. Lett. 73, 225 (1994);
28. Phys. Rev. Lett.F. Abe74, 2626 (1995);
29. Phys. Rev. Lett.D0 Collaboration, S. Abachi, 74, 2632 (1995).
30. Particle Data Group, R. M. Barnett, Phys. Rev. D 54, 1 (1996).
31. X. G. He, Phys. Rev. D 49, 567 (1994);
32. C. D. Froggatt, Nucl. Phys. B420, 3 (1994);
33. B. Dutta and S. Nandi, Oregon Univ.
34. C. H. Albright and S. Nandi, Phys. Rev. D 52, 410 (1995).
35. R. Peccei and K. Wang, Phys. Rev. D 53, 2712 (1996);
36. Phys. Rev. DK. Wang, 54, 5750 (1996).
37. J. N. Bahcall and P. I. Krastev, Phys. Rev. D 53, 4211 (1996).
38. S. P. Mikhayev and A. Yu. Smirnov, Sov. J. Nucl. Phys. 42, 913 (1985);
39. L. Wolfenstein, Phys. Rev. D 17, 2369 (1978);
40. Phys. Rev. DL. Wolfenstein20, 2634 (1979).
41. J. N. Bahcall and R. K. Ulrich, Rev. Mod. Phys. 60, 297 (1988); Ref. 5;
42. X. Shi and D. N. Schramm, Phys. Lett. B 283, 305 (1992);
43. X. Shi, D. N. Schramm, and J. N. Bahcall, Phys. Rev. Lett. 69, 717 (1992);
44. S. A. Bludmann, N. Hata, D. C. Kennedy, and P. Langacker, Phys. Rev. D 47, 2220 (1993);
45. Phys. Rev. DG. L. Fogli, E. Lisi, and D. Montanino, 49, 3626 (1994);
46. Phys. Rev. DG. Fiorenttini, M. Lissia, G. Mezzorani, M. Moretti, and D. Vignaud, 49, 6298 (1994);
47. Phys. Rev. DN. Hata and P. Langacker, 50, 632 (1994);
48. P. I. Krastev and S. T. Petcov, Phys. Lett. B 299, 99 (1993);
49. Phys. Lett. BP. I. Krastev and A. Y. Smirnov, 338, 282 (1994).
50. See, for example, Z. G. Berezhiani and R. N. Mohapatra, Phys. Rev. D 52, 6607 (1995).
51. L. Borodovsky, Phys. Rev. Lett. 68, 274 (1992).
52. B. Zeitnitz, Prog. Part. Nucl. Phys. 32, 351 (1994).
53. B. Ackar, Nucl. Phys. B434, 503 (1995).
54. N. Okada and O. Yasuda, Int. J. Mod. Phys. A 12, 3669 (1997).
55. S. M. Bilenky, C. Giunti, and W. Grimus, hep-ph/9607372.
56. G. L. Fogli, E. Lisi, and D. Montanino, Astropart. Phys. 4, 177 (1995);
57. G. L. Fogli, E. Lisi, and G. Scioscia, Phys. Rev. D 52, 5334 (1995);
58. Phys. Rev. DG. L. Fogli, E. Lisi, 52, 2775 (1995);
59. P. I. Krastev and S. T. Petcov, Nucl. Phys. B449, 605 (1995);
60. P. I. KrastevS. T. PetcovPhys. Rev. D 53, 1665 (1997);
61. Phys. Rev. DH. Minakata, 52, 6630 (1995);
62. Phys. Rev. DM. Narayan, M. V. N. Murthy, G. Rajasekaran, and S. Uma Sankar, 53, 2809 (1996);
63. Phys. Rev. DP. I. Krastev, S. T. Petcov, and L. Qiuyu, 54, 7057 (1996);
64. N. Okada and O. Yasuda, Int. J. Mod. Phys. A 12, 3669 (1997); O. Yasuda, Tokyo Metropolitan Univ. Report TMUP-HEL-9604.
65. C. Y. Cardall and G. M. Fuller, Phys. Rev. D 53, 4421 (1996).
66. G. L. Fogli, E. Lisi, and G. Scioscia, Phys. Rev. D 52, 5334 (1995);
67. K. S. Babu, J. Pati, and F. Wilczck, Phys. Lett. B 359, 351 (1995).
68. S. M. Bilenky and S. T. Petcov, Rev. Mod. Phys. 59, 671 (1987);
69. A. S. Joshipura, Z. Phys. C 64, 31 (1994);
70. A. Ionnaissyan and J. W. F. Valle, Phys. Lett. B 332, 93 (1994);
71. H. Minakata and O. Yasuda, Phys. Rev. D 56, 1692 (1997);
72. J. R. Primack, Phys. Rev. Lett. 74, 2160 (1995).
73. S. Barshay and P. Heiliger, Astropart. Phys. 6, 323 (1997); H. Minakata 31;
74. S. M. Bilenky, C. Giunti, C. W. Kim, and S. T. Petcov, Phys. Rev. D 54, 4432 (1996).
75. P. B. Pal, Int. J. Mod. Phys. A 7, 5387 (1992).
76. K. S. Babu and Q. Shafi, Phys. Lett. B 294, 235 (1994).
77. A. Acker and S. Pakvasa, Phys. Lett. B 397, 209 (1997).
78. T. Motoboyoshi, Phys. Rev. Lett. 73, 2680 (1994);
79. For a summary, see R. S. Raghvan, Science 267, 45 (1995).
80. G. Gelmini and E. Roulet, Rep. Prog. Phys. 58, 1207 (1995).