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Testing for large extra dimensions with neutrino oscillations
Phys. Rev. D 84, 013003 – Published 5 July, 2011
DOI: https://doi.org/10.1103/PhysRevD.84.013003
Abstract
We consider a model where sterile neutrinos can propagate in a large compactified extra dimension giving rise to Kaluza-Klein (KK) modes and the standard model left-handed neutrinos are confined to a 4-dimensional spacetime brane. The KK modes mix with the standard neutrinos modifying their oscillation pattern. We examine former and current experiments such as CHOOZ, KamLAND, and MINOS to estimate the impact of the possible presence of such KK modes on the determination of the neutrino oscillation parameters and simultaneously obtain limits on the size of the largest extra dimension. We found that the presence of the KK modes does not essentially improve the quality of the fit compared to the case of the standard oscillation. By combining the results from CHOOZ, KamLAND, and MINOS, in the limit of a vanishing lightest neutrino mass, we obtain the stronger bound on the size of the extra dimension as at 99% C.L. for normal (inverted) mass hierarchy. If the lightest neutrino mass turns out to be larger, 0.2 eV, for example, we obtain the bound . We also discuss the expected sensitivities on the size of the extra dimension for future experiments such as Double CHOOZ, T2K, and NOνA.
Article Text
References (41)
- N. Arkani-Hamed, S. Dimopoulos, and G. Dvali, Phys. Lett. B 429, 263 (1998); I. Antoniadis, N. Arkani-Hamed, S. Dimopoulos, and G. Dvali, 436, 257 (1998); N. Arkani-Hamed, S. Dimopoulos, and G. Dvali, Phys. Rev. D 59, 086004 (1999).
- L. Randall and R. Sundrum, Phys. Rev. Lett. 83, 3370 (1999); 83, 4690 (1999).
- C. D. Hoyle et al., Phys. Rev. Lett. 86, 1418 (2001).
- S. Hannestad and G. G. Raffelt, Phys. Rev. D 67, 125008 (2003); 69, 029901(E) (2004).
- K. Lande et al. (Homestake Collaboration), Astrophys. J. 496, 505 (1998); Nucl. Phys. B, Proc. Suppl. 77, 13 (1999); Y. Fukuda et al. (Kamiokande Collaboration), Phys. Rev. Lett. 77, 1683 (1996); W. Hampel et al. (Gallex Collaboration), Phys. Lett. B 447, 127 (1999); M. Altmann et al. (GNO Collaboration), 490, 16 (2000); J. N. Abdurashitov et al. (SAGE Collaboration), Phys. Rev. C 60, 055801 (1999); V. N. Gavrin, Nucl. Phys. B, Proc. Suppl. 91, 36 (2001); Y. Fukuda et al. (Super-Kamiokande Collaboration), Phys. Rev. Lett. 81, 1158 (1998); 81, 4279(E) (1998); 82, 1810 (1999); 82, 2430 (1999); Y. Suzuki, Nucl. Phys. B, Proc. Suppl. 91, 29 (2001); J. P. Cravens et al., Phys. Rev. D 78, 032002 (2008); Q. R. Ahmad et al. (SNO Collaboration), Phys. Rev. Lett. 89, 011301 (2002); S. N. Ahmed et al., 92, 181301 (2004); B. Aharmim et al., 101, 111301 (2008); Phys. Rev. C 81, 055504 (2010); C. Arpesella et al. (The Borexino Collaboration), Phys. Rev. Lett. 101, 091302 (2008); L. Oberauer, J. Phys. Conf. Ser. 203, 012081 (2010).
- H. S. Hirata et al. (Kamiokande Collaboration), Phys. Lett. B 205, 416 (1988); 280, 146 (1992); Y. Fukuda et al., ibid. 335, 237 (1994); R. Becker-Szendy et al. (IMB Collaboration), Phys. Rev. D 46, 3720 (1992); W. W. M. Allison et al. (Soudan-2 Collaboration), Phys. Lett. B 391, 491 (1997); Y. Fukuda et al. (Super-Kamiokande Collaboration), Phys. Rev. Lett. 81, 1562 (1998); Phys. Lett. B 436, 33 (1998); Y. Ashie et al., Phys. Rev. Lett. 93, 101801 (2004); K. Abe et al., 97, 171801 (2006); Phys. Rev. D 77, 052001 (2008).
- M. H. Ahn et al. (K2K Collaboration), Phys. Rev. Lett. 90, 041801 (2003); E. Aliu et al. (K2K Collaboration), 94, 081802 (2005); M. H. Ahn et al., Phys. Rev. D 74, 072003 (2006).
- D. G. Michael et al. (MINOS Collaboration), Phys. Rev. Lett. 97, 191801 (2006).
- P. Adamson et al. (MINOS Collaboration), Phys. Rev. Lett. 101, 131802 (2008).
- P. Vahle (MINOS Collaboration), XXIV International Conference on Neutrino Physics and Astrophysics (Neutrino 2010), Athens, Greece, 2010, slides available at http://www.neutrino2010.gr/.
- K. Eguchi et al. (KamLAND Collaboration), Phys. Rev. Lett. 90, 021802 (2003).
- A. Gando et al. (KamLAND Collaboration), Phys. Rev. D 83, 052002 (2011).
- K. R. Dienes, E. Dudas, and T. Gherghetta, Nucl. Phys. B557, 25 (1999).
- N. Arkani-Hamed, S. Dimopoulos, G. R. Dvali et al., Phys. Rev. D 65, 024032 (2001).
- G. R. Dvali and A. Y. Smirnov, Nucl. Phys. B563, 63 (1999).
- R. Barbieri, P. Creminelli, and A. Strumia, Nucl. Phys. B585, 28 (2000).
- R. N. Mohapatra, S. Nandi, and A. Perez-Lorenzana, Phys. Lett. B 466, 115 (1999); R. N. Mohapatra and A. Perez-Lorenzana, Nucl. Phys. B576, 466 (2000); B593, 451 (2001).
- H. Davoudiasl, P. Langacker, and M. Perelstein, Phys. Rev. D 65, 105015 (2002).
- M. Apollonio et al. (CHOOZ Collaboration), Eur. Phys. J. C 27, 331 (2003).
- F. Ardellier et al. (Double CHOOZ Collaboration), arXiv:hep-ex/0606025.
- Y. Itow et al., arXiv:hep-ex/0106019; For an updated version, see http://neutrino.kek.jp/jhfnu/loi/loi.v2.030528.pdf.
- D. S. Ayres et al. (NOνA Collaboration), arXiv:hep-ex/0503053.
- T. Yang and S. Woijcicki (NOνA Collaboration), Off-Axis-Note-SIM-30, 2004.
- A. Aguilar et al. (LSND Collaboration), Phys. Rev. D 64, 112007 (2001).
- B. Armbruster et al. (KARMEN Collaboration), Phys. Rev. D 65, 112001 (2002).
- A. A. Aguilar-Arevalo et al. (MiniBooNE Collaboration), Phys. Rev. Lett. 103, 111801 (2009).
- T. A. Mueller et al., Phys. Rev. C 83, 054615 (2011).
- G. Mention et al., Phys. Rev. D 83, 073006 (2011).
- K. Nakamura et al. (Particle Data Group), J. Phys. G 37, 075021 (2010).
- R. Franceschini, G. F. Giudice, P. P. Giardino, P. Lodone, and A. Strumia, J. High Energy Phys. 05 (2011) 092.
- P. A. N. Machado et al. (work in progress).
- T. Hallgren, T. Ohlsson, and G. Seidl, J. High Energy Phys. 02 (2005) 049.
- P. Huber et al., Comput. Phys. Commun. 177, 432 (2007); see http://www.mpi-hd.mpg.de/~globes.
- M. C. Gonzalez-Garcia, M. Maltoni, and J. Salvado, J. High Energy Phys. 04 (2010) 056.
- H. Nunokawa, W. J. C. Teves, and R. Zukanovich Funchal, Phys. Lett. B 562, 28 (2003); H. Minakata, H. Nunokawa, W. J. C. Teves, and R. Zukanovich Funchal, Phys. Rev. D 71, 013005 (2005).
- J. Kopp, P. A. N. Machado, and S. J. Parke, Phys. Rev. D 82, 113002 (2010).
- M. Bishai (private communication).
- M. D. Messier, Report No. UMI-99-23965, 1999.
- E. A. Paschos and J. Y. Yu, Phys. Rev. D 65, 033002 (2002).
- P. Huber, M. Lindner, T. Schwetz, and W. Winter, J. High Energy Phys. 11 (2009) 044.
- K. Hiraide et al., Phys. Rev. D 73, 093008 (2006).