Variations on four-neutrino oscillations

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 58, Issue 9, 1998, Pages

  Barger, V ^a   Pakvasa, S ^b   Weiler, T J ^c   Whisnant, K ^d  

^a University of Wisconsin ^*  (United States)

^b UNIVERSITY OF HAWAII   (United States)

^c VANDERBILT UNIVERSITY   (United States)

^d IOWA STATE UNIVERSITY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 1542575352     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.58.093016     Document Type: Article

References (148)

1. J. N. Bahcall and M. H. Pinsonneault, Rev. Mod. Phys. 67, 781 (1995);
2. J. N. Bahcall, S. Basu, and M. H. Pinsonneault, Phys. Lett. B 433, 1 (1998); the new solar flux calculation in the second reference has not yet been implemented in the solar neutrino analyses.
3. B. T. Cleveland, Nucl. Phys. B (Proc. Suppl.) 38, 47 (1995);
4. Kamiokande Collaboration, Y. Fukuda, Phys. Rev. Lett. 77, 1683 (1996);
5. GALLEX Collaboration, W. Hampel, Phys. Lett. B 388, 384 (1996);
6. SAGE Collaboration, J. N. Abdurashitov, Phys. Rev. Lett. 77, 4708 (1996).
7. Kamiokande Collaboration, K. S. Hirata, Phys. Lett. B 280, 146 (1992);
8. Phys. Lett. BY. Fukuda, 335, 237 (1994);
9. IMB Collaboration, R. Becker-Szendy, Nucl. Phys. B (Proc. Suppl.) 38, 331 (1995);
10. Soudan-2 Collaboration, W. W. M. Allison, Phys. Lett. B 391, 491 (1997).
11. Super-Kamiokande Collaboration, talk by E. Kearns in Ref. 8 and hep-ex/9803007;
12. Y. Fukuda, hep-ex/9803006.
13. The Super-Kamiokande Collaboration, Y. Fukuda, hep-ex/9805006.
14. J. G. Learned, S. Pakvasa, and T. J. Weiler, Phys. Lett. B 207, 79 (1988);
15. Phys. Lett. BV. Barger and K. Whisnant, 209, 365 (1988);
16. K. Hidaka, M. Honda, and S. Midorikawa, Phys. Rev. Lett. 61, 1537 (1988).
17. Liquid Scintillator Neutrino Detector (LSND) Collaboration, C. Athanassopoulos, Phys. Rev. Lett. 75, 2650 (1995);
18. Phys. Rev. Lett.C. Athanassopoulos77, 3082 (1996);
19. C. AthanassopoulosPhys. Rev. C 58, 2489 (1998).
20. a recent review, see talks at the ITP Conference on Solar Neutrinos: News About SNUS, Santa Barbara, December 1997 at http://doug-pc.itp.ucsb.edu/online/snu/schedule.html
21. C. Y. Cardall and G. M. Fuller, Nucl. Phys. B (Proc. Suppl.) 51, 259 (1996);
22. G. L. Fogli, E. Lisi, D. Montanino, and G. Scioscia, Phys. Rev. D 56, 4365 (1997).
23. A. Acker, J. G. Learned, S. Pakvasa, and T. J. Weiler, Phys. Lett. B 298, 149 (1992);
24. Phys. Lett. BA. Acker and S. Pakvasa, 397, 209 (1997);
25. P. I. Krastev and S. T. Petcov, Phys. Lett. B 395, 69 (1997).
26. Y. Grossman, Phys. Lett. B 359, 141 (1995);
27. L. M. Johnson and D. McKay, Phys. Lett. B 433, 355 (1998); however, S. Bergmann and Y. Grossman, private communication and work in progress, argue that some lepton-flavor violating operators which would explain the LSND result are likely to be incompatible with the present muonium-antimuonium conversion limits.
28. KARMEN Collaboration, B. Bodmann, Nucl. Phys. A553, 831c (1993);
29. J. Kleinfeller, Nucl. Phys. B (Proc. Suppl.) 48, 207 (1996); talks by B. Armbruster at 33rd Rencontres de Moriond: Electroweak Interactions and Unified Theories, Les Arcs, France, 1998; B. Zeitnitz at Neutrino-98, Takayama, Japan, 1998, and G. Drexlin at 5th International WEIN Symposium, Sante Fe, NM, 1998.
30. V. Barger, P. Langacker, J. Leveille, and S. Pakvasa, Phys. Rev. Lett. 45, 692 (1980);
31. Z. G. Berezhiani and R. N. Mohapatra, Phys. Rev. D 52, 6607 (1995);
32. E. J. Chun, A. S. Joshipura, and A. Y. Smirnov, Phys. Lett. B 357, 608 (1995);
33. E. J. ChunA. S. JoshipuraA. Y. SmirnovPhys. Rev. D 54, 4654 (1996);
34. K. Benakli and A. Y. Smirnov, Phys. Rev. Lett. 79, 4314 (1997);
35. J. R. Espinosa, Nucl. Phys. B (Proc. Suppl.) 62, 187 (1998);
36. G. Cleaver, M. Cvetic, J. R. Espinosa, L. Everett, and P. Langacker, Phys. Rev. D 57, 2701 (1998);
37. P. Langacker, Phys. Rev. D (to be published), hep-ph/9805281.
38. LEP Electroweak Working Group and SLD Heavy Flavor Group, D. Abbaneo et al., CERN-PPE-96-183, 1996.
39. D. O. Caldwell and R. N. Mohapatra, Phys. Rev. D 48, 3259 (1993);
40. J. T. Peltoniemi and J. W. F. Valle, Nucl. Phys. B406, 409 (1993);
41. R. Foot and R. R. Volkas, Phys. Rev. D 52, 6595 (1995);
42. Phys. Rev. DErnest Ma and Probir Roy, 52, R4780 (1995);
43. J. J. Gomez-Cadenas and M. C. Gonzalez-Garcia, Z. Phys. C 71, 443 (1996);
44. N. Okada and O. Yasuda, Int. J. Mod. Phys. A 12, 3669 (1997);
45. S. M. Bilenky, C. Giunti, and W. Grimus, hep-ph/9711416;
46. R. N. Mohapatra, hep-ph/9711444;
47. N. Gaur, A. Ghosal, Ernest Ma, and Probir Roy, Phys. Rev. D 58, 071301 (1998);
48. particularly strong enthusiasm for the sterile neutrino is expressed by D. O. Caldwell, hep-ph/9804367.
49. R. Barbieri and A. Dolgov, Phys. Lett. B 237, 440 (1990);
50. K. Enqvist, K. Kainulainen, and M. Thomson, Nucl. Phys. B373, 498 (1992);
51. X. Shi, D. N. Schramm, and B. D. Fields, Phys. Rev. D 48, 2563 (1993);
52. Phys. Rev. DC. Y. Cardall and G. M. Fuller, 54, 1260 (1996);
53. Phys. Rev. DD. P. Kirilova and M. V. Chizhov, 58, 073004 (1998);
54. S. M. Bilenky, C. Giunti, W. Grimus, and T. Schwetz, hep-ph/9804421.
55. P. J. Kernan and S. Sarkar, Phys. Rev. D 54, R3681 (1996);
56. S. Sarkar, Rep. Prog. Phys. 59, 1 (1996); K. A. Olive, talk at 5th International Workshop on Topics in Astroparticle and Underground Physics (TAUP 97), Gran Sasso, Italy, 1997;K. A. Olive, proc. of 5th International Conference on Physics Beyond the Standard Model, Balholm, Norway, 1997;
57. C. J. Copi, D. N. Schramm and M. S. Turner, Phys. Rev. Lett. 75, 3981 (1995);
58. K. A. Olive and G. Steigman, Phys. Lett. B 354, 357 (1995).
59. R. Foot and R. R. Volkas, Phys. Rev. Lett. 75, 4350 (1995);
60. R. Foot, M. J. Thompson, and R. R. Volkas, Phys. Rev. D 53, 5349 (1996);
61. Phys. Rev. D53N. F. Bell, R. Foot, and R. R. Volkas, (to be published), hep-ph/9805259.
62. R. Foot and R. R. Volkas, Phys. Rev. D 55, 5147 (1997);
63. Q. Y. Liu and A. Yu. Smirnov, Nucl. Phys. B524, 505 (1998).
64. L. Wolfenstein, Phys. Rev. D 17, 2369 (1978);
65. S. P. Mikheyev and A. Smirnov, Yad. Fiz. 42, 1441 (1985);
66. S. P. MikheyevA. SmirnovNuovo Cimento C 9, 17 (1986).
67. S. P. Rosen and J. M. Gelb, Phys. Rev. D 34, 969 (1986).
68. S. J. Parke, Phys. Rev. Lett. 57, 1275 (1986);
69. Phys. Rev. Lett.S. J. Parke and T. P. Walker, 57, 2322 (1986);
70. Phys. Rev. Lett.W. C. Haxton, 57, 1271 (1986);
71. T. K. Kuo and J. Pantaleone, Rev. Mod. Phys. 61, 937 (1989).
72. H. Bethe, Phys. Rev. Lett. 56, 1305 (1986);
73. V. Barger, R. J. N. Phillips, and K. Whisnant, Phys. Rev. D 34, 980 (1986).
74. V. Barger, R. J. N. Phillips, and K. Whisnant, Phys. Rev. D 24, 538 (1981).
75. S. L. Glashow and L. M. Krauss, Phys. Lett. B 190, 199 (1987).
76. V. Barger, K. Whisnant, D. Cline, and R. J. N. Phillips, Phys. Lett. 93B, 194 (1980).
77. K. Zuber, talk at COSMO’97, Ambleside, England, 1997, hep-ph/9712378.
78. F. Dydak, Phys. Lett. 134B, 281 (1984).
79. I. E. Stockdale, Phys. Rev. Lett. 52, 1384 (1984).
80. Y. Declais, Nucl. Phys. B434, 503 (1995).
81. Y.-Z. Qian, Phys. Rev. Lett. 71, 1965 (1993).
82. J. T. Peltoniemi, hep-ph/9511323;
83. H. Nunokawa, A. Rossi, and J. Valle, Phys. Rev. D 56, 1704 (1997); D. O. Caldwell, G. Fuller, and Y. Z. Qian, private communication and work in progress.
84. C. Y. Cardall and G. M. Fuller, astro-ph/9701178.
85. L. Borodovsky, Phys. Rev. Lett. 68, 274 (1992).
86. A good discussion of the various statistics can be found in G. L. Fogli, E. Lisi, and G. Sciosia, Phys. Rev. D 56, 3081 (1997).
87. D. O. Caldwell, talk presented at the Aspen Center for Physics, 1998.
88. E. Church, nucl-ex/9706011.
89. G. Barr, T. K. Gaisser, and T. Stanev, Phys. Rev. D 39, 3532 (1989);
90. Phys. Rev. DM. Honda, T. Kajita, K. Kasahara, and S. Midorikawa, 52, 4985 (1995);
91. Phys. Rev. DV. Agrawal, T. K. Gaisser, P. Lipari, and T. Stanev, 53, 1314 (1996);
92. Phys. Rev. DT. K. Gaisser, 54, 5578 (1996).
93. M. C. Gonzalez-Garcia, H. Nunokawa, O. Peres, T. Stanev, and J. W. F. Valle, Phys. Rev. D 58, 033004 (1998).
94. CHOOZ Collaboration, M. Apollonio, Phys. Lett. B 420, 397 (1998).
95. E. Akhmedov, P. Lipari, and M. Lusignoli, Phys. Lett. B 300, 128 (1993);
96. P. Lipari and M. Lusignoli, Phys. Rev. D 57, 3842 (1998);
97. Phys. Rev. DP. LipariM. Lusignoli58073005 (1998);
98. Phys. Rev. DR. Foot, R. R. Volkas, and O. Yasuda, 58, 013006 (1998).
99. N. Hata and P. Langacker, Phys. Rev. D 56, 6107 (1997).
100. P. Krastev and S. T. Petcov, Phys. Rev. Lett. 72, 1960 (1994);
101. P. KrastevS. T. PetcovNucl. Phys. B449, 605 (1995).
102. Y. Suzuki, talk at Neutrino-98, Takayama, Japan, 1998.
103. V. Barger, K. Whisnant, S. Pakvasa, and R. J. N. Phillips, Phys. Rev. D 22, 2718 (1980).
104. P. Langacker, J. P. Leveille, and J. Sheiman, Phys. Rev. D 27, 1228 (1983).
105. V. Barger, N. Deshpande, P. B. Pal, R. J. N. Phillips, and K. Whisnant, Phys. Rev. D 43, 1759 (1991);
106. S. Bludman, D. C. Kennedy, and P. Langacker, Nucl. Phys. B374, 373 (1992).
107. C. Yanagisawa, talk given at Pheno 98, Madison, WI, 1998.
108. V. Barger, K. Whisnant, and T. J. Weiler, Phys. Lett. B 427, 97 (1998).
109. S. C. Gibbons, R. N. Mohapatra, S. Nandi, and A. Raychaudhuri, Phys. Lett. B 430, 296 (1998).
110. S. M. Bilenky, C. Giunti, and W. Grimus, Eur. J. Phys. C1, 247 (1998).
111. T. J. Weiler, Astropart. Phys. (to be published), hep-ph/9710431.
112. Solar Neutrino Observatory (SNO) Collaboration, E. Norman et al., in Proceedings of The Fermilab Conference: DPF 92, 1992, Batavia, IL, edited by C. H. Albright, P. H. Kasper, R. Raja, and J. Yoh (World Scientific, Singapore, 1993), p. 1450.
113. BOREXINO Collaboration, C. Arpesella et al., in INFN Borexino proposal, Vols. I and II, edited by G. Bellini et al. (Univ. of Milan, Milan, 1992);
114. J. Benziger, Proposal for Participation in the Borexino Solar Neutrino Experiment (Princeton University, Princeton, NJ, 1996).
115. HELLAZ Collaboration, F. Arzarello et al., CERN-LAA/94-19.
116. A. B. Balantekin, J. F. Beacom, and J. M. Fetter, Phys. Lett. B 427, 317 (1998).
117. M. Maris and S. T. Petcov, Phys. Rev. D (to be published).
118. Q. Y. Liu, S. P. Mikheyev, and A. Y. Smirnov, hep-ph/9803415.
119. Analytical derivations of the conditions required for resonant flavor-conversion in the earth’s mantle-core system are given in S. T Petcov, hep-ph/9805262;
120. E. K. Akhmedov, hep-ph/9805272.
121. J. Flanagan, J. G. Learned, and S. Pakvasa, Phys. Rev. D 57, R2649 (1998);
122. J. Bunn, R. Foot, and R. R. Volkas, Phys. Lett. B 413, 109 (1997).
123. J. G. Learned, S. Pakvasa, and J. Stone, Phys. Lett. B 435, 131 (1998).
124. F. Vissani and A. Smirnov, Phys. Lett. B 432, 376 (1998).
125. L. J. Hall and H. Murayama, hep-ph/9806218.
126. A. Curioni, hep-ph/9805249.
127. World Wide Web links to more information on these and other neutrino oscillation experiments, see the Neutrino Oscillation Industry web page at http://www.hep.anl.gov/NDK/Hypertext/nuindustry.html.
128. MINOS Collaboration, “Neutrino Oscillation Physics at Fermilab: The NuMI-MINOS Project,” NuMI-L-375, 1998.
129. S. Geer, Phys. Rev. D 57, 6989 (1998).
130. AMANDA Collaboration, S. Barwick et al., in Proceedings of the XXVIth International Conference on High Energy Physics, Dallas, TX, 1992, edited by James R. Sanford (AIP, New York, 1993), p. 1250;
131. F. Halzen, in Proceedings of the Workshop on Fundamental Particles and interactions: Frontiers in Contemporary Physics, Vanderbilt University, Tennessee, 1997, edited by R. S. Panvini and T. J. Weiler, AIP Conf. Proc. No. 23 (AIP, New York, 1998), p. 154.
132. H. V. Klapdor-Kleingrothaus, hep-ex/9802007;
133. H. V. Klapdor-KleingrothausJ. Phys. G 24, 483 (1998).
134. A. I. Belesev, Phys. Lett. B 350, 263 (1995);
135. V. M. Lobashev, in Proc. of Neutrino ’98, edited by K. Enqvist, K. Huitu, and J. Maalampi (World Scientific, Singapore, 1997).
136. a recent discussion see J. Primack, in Proceedings of the Jerusalem Winter School 1996, edited by A. Dekel and J. P. Ostriker (Cambridge University Press, Cambridge, England), Chap. 1 and astro-ph/9707285;
137. E. Gawiser and J. Silk, Science 280, 1405 (1998).
138. E. W. Kolb and M. S. Turner, The Early Universe (Addison-Wesley, Reading, MA, 1990).
139. W. Hu, D. J. Eisenstein, and M. Tegmark, Phys. Rev. Lett. 80, 5255 (1998).
140. See http://map.gsfc.nasa.gov for information on MAP.
141. See http://astro.estec.esa.nl/Planck/ for information on PLANCK.
142. C.-P. Ma and E. Bertschinger, Astrophys. J. 455, 7 (1995);
143. Astrophys. J.S. Dodelson, E. Gates, and A. Stebbins, 467, 10 (1996);
144. R. E. Lopez, S. Dodelson, A. Heckler, and M. S. Turner, astro-ph/9803095.
145. S. Hannestad and G. Raffelt, astro-ph/9805223.
146. B. Faid, G. L. Fogli, E. Lisi, and D. Montanino, hep-ph/9805293.
147. V. Barger, R. J. N. Phillips, and K. Whisnant, Phys. Rev. Lett. 65, 3084 (1990).
148. G. L. Fogli, E. Lisi, and D. Montanino, hep-ph/9803309.