Three-flavor Lorentz-violating solution to the LSND anomaly?

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 74, Issue 9, 2006, Pages

  De Gouvêa, André ^a   Grossman, Yuval ^b  

^a NORTHWESTERN UNIVERSITY   (United States)

^b TECHNION ISRAEL INSTITUTE OF TECHNOLOGY   (Israel)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 33751347609     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.74.093008     Document Type: Article

References (40)

1. C. Athanassopoulos (LSND Collaboration), Phys. Rev. Lett. 77, 3082 (1996); PRLTAO 0031-9007 10.1103/PhysRevLett.77.3082
2. C. Athanassopoulos LSND Collaboration Phys. Rev. Lett. 81, 1774 (1998). PRLTAO 0031-9007 10.1103/PhysRevLett.81.1774
3. C. Athanassopoulos (LSND Collaboration), Phys. Rev. Lett. 81, 1774 (1998); PRLTAO 0031-9007 10.1103/PhysRevLett.81.1774
4. A. Aguilar (LSND Collaboration), Phys. Rev. D 64, 112007 (2001). PRVDAQ 0556-2821 10.1103/PhysRevD.64.112007
5. For a recent pedagogical discussion and many references, see A. de Gouvêa, hep-ph/0411274.
6. B. Armbruster (KARMEN Collaboration), Phys. Rev. D 65, 112001 (2002). PRVDAQ 0556-2821 10.1103/PhysRevD.65.112001
7. See, for example, M. Maltoni, T. Schwetz, M.A. Tortola, and J.W.F. Valle, New J. Phys. 6, 122 (2004). NJOPFM 1367-2630 10.1088/1367-2630/6/1/122
8. M. Sorel, J.M. Conrad, and M. Shaevitz, Phys. Rev. D 70, 073004 (2004). PRVDAQ 0556-2821 10.1103/PhysRevD.70.073004
9. M. Sorel and O. Yasuda (private communication).
10. See, for example, M. Cirelli, Nucl. Phys. NUPBBO 0550-3213 B708, 215 (2005). 10.1016/j.nuclphysb.2004.11.056
11. Solutions to the LSND anomaly that are currently ruled out include (see also): H. Murayama and T. Yanagida, Phys. Lett. B 520, 263 (2001); PYLBAJ 0370-2693 10.1016/S0370-2693(01)01136-4
12. G. Barenboim, L. Borissov, J.D. Lykken, and A.Y. Smirnov, J. High Energy Phys. JHEPFG 1029-8479 10 (2002) 001; 10.1088/1126-6708/2002/10/001
13. K.S. Babu and S. Pakvasa, hep-ph/0204236;
14. G. Barenboim, L. Borissov, and J.D. Lykken, hep-ph/0212116;
15. D.B. Kaplan, A.E. Nelson, and N. Weiner, Phys. Rev. Lett. 93, 091801 (2004). PRLTAO 0031-9007 10.1103/PhysRevLett.93.091801
16. Proposed solutions to the LSND anomaly that seem to accommodate the rest of the world neutrino data include V. Barger, D. Marfatia, and K. Whisnant, Phys. Lett. B 576, 303 (2003); PYLBAJ 0370-2693 10.1016/j.physletb.2003.10.004
17. S. Palomares-Ruiz, S. Pascoli, and T. Schwetz, J. High Energy Phys. JHEPFG 1029-8479 09 (2005) 048; 10.1088/1126-6708/2005/09/048
18. H. Päs, S. Pakvasa, and T.J. Weiler, Phys. Rev. D 72, 095017 (2005); PRVDAQ 0556-2821 10.1103/PhysRevD.72.095017
19. V. Barger, D. Marfatia, and K. Whisnant, Phys. Rev. D 73, 013005 (2006). All of them require the existence of sterile neutrinos, plus other "new physics." PRVDAQ 0556-2821 10.1103/PhysRevD.73.013005
20. G. Barenboim and N.E. Mavromatos, J. High Energy Phys. JHEPFG 1029-8479 01 (2005) 034. 10.1088/1126-6708/2005/01/034
21. V.A. Kostelecky and M. Mewes, Phys. Rev. D 70, 076002 (2004). PRVDAQ 0556-2821 10.1103/PhysRevD.70.076002
22. L.B. Auerbach (LSND Collaboration), Phys. Rev. D 72, 076004 (2005). PRVDAQ 0556-2821 10.1103/PhysRevD.72.076004
23. A. Strumia, Phys. Lett. B 539, 91 (2002). PYLBAJ 0370-2693 10.1016/S0370-2693(02)02042-7
24. Several "updates" included in the version present in the preprint archive, hep-ph/0201134.
25. M.C. Gonzalez-Garcia, M. Maltoni, and T. Schwetz, Phys. Rev. D 68, 053007 (2003). PRVDAQ 0556-2821 10.1103/PhysRevD.68.053007
26. V.A. Kostelecky and M. Mewes, Phys. Rev. D 69, 016005 (2004). PRVDAQ 0556-2821 10.1103/PhysRevD.69.016005
27. See, for example, R.N. Mohapatra, hep-ph/0510213;
28. A. de Gouvêa, Mod. Phys. Lett. A 19, 2799 (2004). MPLAEQ 0217-7323 10.1142/S0217732304016032
29. For a detailed, combined analysis of KARMEN and LSND data, see E.D. Church, K. Eitel, G.B. Mills, and M. Steidl, Phys. Rev. D 66, 013001 (2002). PRVDAQ 0556-2821 10.1103/PhysRevD.66.013001
30. P. Astier (NOMAD Collaboration), Phys. Lett. B 570, 19 (2003); PYLBAJ 0370-2693 10.1016/j.physletb.2003.07.029
31. B.A. Popov (NOMAD Collaboration), Phys. At. Nucl. PANUEO 1063-7788 67, 1942 (2004). 10.1134/1.1825509
32. P. Astier (NOMAD Collaboration), Nucl. Phys. NUPBBO 0550-3213 B611, 3 (2001).
33. A.M. Guler (CHORUS Collaboration), in Proceedings at 32nd International Conference on High-Energy Physics (ICHEP 04), Beijing, China, 2004 (unpublished);
34. see also http://ichep04.ihep.ac.cn/.
35. S. Avvakumov, Phys. Rev. Lett. 89, 011804 (2002). PRLTAO 0031-9007 10.1103/PhysRevLett.89.011804
36. A. de Gouvêa, Phys. Rev. D 66, 076005 (2002). PRVDAQ 0556-2821 10.1103/PhysRevD.66.076005
37. For a recent overview and update, see S.J. Brice (MiniBooNE Collaboration), Nucl. Phys. B, Proc. Suppl. NPBSE7 0920-5632 143, 115 (2005); 10.1016/j.nuclphysbps.2005.01.095
38. see also http://www-boone.fnal.gov/.
39. G.T. Garvey, Phys. Rev. D 72, 092001 (2005). PRVDAQ 0556-2821 10.1103/PhysRevD.72.092001
40. B. Armbruster, Phys. Rev. Lett. 90, 181804 (2003). PRLTAO 0031-9007 10.1103/PhysRevLett.90.181804