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The goal of the Daya Bay reactor experiment is to determine unknown neutrino mixing angle θ13. The non-standard interactions (NSIs) of the neutrinos will affect the neutrino oscillation probability. In this paper we check the Daya Bay experimental sensitivity to θ13 in the presence of NSIs. Clearly, in this single experiment the values of θ13 and NSIs cannot be determined. The experimental observation of neutrino oscillation indicates a non-zero θ13. But if we do not observe the neutrino oscillation, it will not be meant that the value of θ13 must be zero.
[1] Cattadori C, Ferrari N, Pandola L 2005 Nucl. Phys. Proc. Suppl. 143 3
[2] Kamland Collaboration 2003 Phys. Rev. Lett. 90 021802
[3] Kamland Collaboration 2005 Phys. Rev. Lett. 94 081801
[4] Super-Kamiokande Collaboration 1998 Phys. Rev. Lett. 81 1562
[5] Super-Kamiokande Collaboration 2005 Phys. Rev. D 71 112005
[6] Minos Collaboration 2008 Phys.Rev.Lett.101 131802
[7] Huang X J, Li Z J, Wang Y J 2006 Chin. Phy. B 15 229
[8] Zhang J, Liu M Q, Wei B T, Luo Z Q 2008 Acta Phys. Sin. 57 5448 (in Chinese) [张 洁、刘门全、魏丙涛、罗志全 2005 57 5448]
[9] Cao J 2006 Nucl. Phys. Proc. Suppl. 155 229
[10] Daya Bay Collaboration 2007 arXIV:hep-ex/0701029
[11] Grossman Y, 1995 Phys. Lett.B 359 141
[12] Ota T, Sato J, Yamashita N A 2002 Phys. Rev. D 65 0903015
[13] Huber P, Schwetz T, Valle J W F 2002 Phys. Rev. D 66 013006
[14] Kopp J, Lindner M, Ota T, Sato S 2008 Phys. Rev. D 77 013007
[15] Bergmann S, Grossman Y, Pierce D M 2000 Phys. Rev. D 61 053005
[16] Gonzalez-Garcia M C, Grossman Y, Gusso A, Nir Y 2001 Phys. Rev. D 64 096006
[17] Antusch S, Biggio C, Fernandez-Martinez E, Gavela M B, Lopez-Pavon J 2006 Journal High Energy Physics 10 084
[18] Fernandez-Martinez E, Gavela M B, J. López-Pavón J, Yasuda O 2007 Phys. Lett. B 649 427
[19] Goswami S, Ota T 2008 Phys. Rev. D 78 033012
[20] Xing Z Z, Zhou S 2008 Phys. Lett. B 666 166
[21] Luo S 2008 Phys. Rev. D 78 016006
[22] Altarelli G, Meloni D 2008 arXiv:0809.1041
[23] Ohlsson T, Zhang H 2008 arXiv:0809.4835
[24] Maltoni M, Schwetz T, Tortola M A, Valle J W F 2004 New J. Phys. 6 122
[25] Fogli G L, Lisi E, Marrone A, Melchiorri A, Palazzo A, Serra P, Silk J, Slosar A 2007 Phys. Rev. D 75 053001
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[1] Cattadori C, Ferrari N, Pandola L 2005 Nucl. Phys. Proc. Suppl. 143 3
[2] Kamland Collaboration 2003 Phys. Rev. Lett. 90 021802
[3] Kamland Collaboration 2005 Phys. Rev. Lett. 94 081801
[4] Super-Kamiokande Collaboration 1998 Phys. Rev. Lett. 81 1562
[5] Super-Kamiokande Collaboration 2005 Phys. Rev. D 71 112005
[6] Minos Collaboration 2008 Phys.Rev.Lett.101 131802
[7] Huang X J, Li Z J, Wang Y J 2006 Chin. Phy. B 15 229
[8] Zhang J, Liu M Q, Wei B T, Luo Z Q 2008 Acta Phys. Sin. 57 5448 (in Chinese) [张 洁、刘门全、魏丙涛、罗志全 2005 57 5448]
[9] Cao J 2006 Nucl. Phys. Proc. Suppl. 155 229
[10] Daya Bay Collaboration 2007 arXIV:hep-ex/0701029
[11] Grossman Y, 1995 Phys. Lett.B 359 141
[12] Ota T, Sato J, Yamashita N A 2002 Phys. Rev. D 65 0903015
[13] Huber P, Schwetz T, Valle J W F 2002 Phys. Rev. D 66 013006
[14] Kopp J, Lindner M, Ota T, Sato S 2008 Phys. Rev. D 77 013007
[15] Bergmann S, Grossman Y, Pierce D M 2000 Phys. Rev. D 61 053005
[16] Gonzalez-Garcia M C, Grossman Y, Gusso A, Nir Y 2001 Phys. Rev. D 64 096006
[17] Antusch S, Biggio C, Fernandez-Martinez E, Gavela M B, Lopez-Pavon J 2006 Journal High Energy Physics 10 084
[18] Fernandez-Martinez E, Gavela M B, J. López-Pavón J, Yasuda O 2007 Phys. Lett. B 649 427
[19] Goswami S, Ota T 2008 Phys. Rev. D 78 033012
[20] Xing Z Z, Zhou S 2008 Phys. Lett. B 666 166
[21] Luo S 2008 Phys. Rev. D 78 016006
[22] Altarelli G, Meloni D 2008 arXiv:0809.1041
[23] Ohlsson T, Zhang H 2008 arXiv:0809.4835
[24] Maltoni M, Schwetz T, Tortola M A, Valle J W F 2004 New J. Phys. 6 122
[25] Fogli G L, Lisi E, Marrone A, Melchiorri A, Palazzo A, Serra P, Silk J, Slosar A 2007 Phys. Rev. D 75 053001
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