Electron neutrino and antineutrino appearance in the full MINOS data sample

P. Adamson; I. Anghel; C. Backhouse; G. Barr; M. Bishai; A. Blake; G. J. Bock; D. Bogert; S. V. Cao; D. Cherdack; S. Childress; J. A B Coelho; L. Corwin; D. Cronin-Hennessy; J. K. De Jong; A. V. Devan; N. E. Devenish; M. V. Diwan; C. O. Escobar; J. J. Evans; E. Falk; G. J. Feldman; M. V. Frohne; H. R. Gallagher; R. A. Gomes; M. C. Goodman; P. Gouffon; N. Graf; R. Gran; K. Grzelak; A. Habig; S. R. Hahn; J. Hartnell; R. Hatcher; A. Himmel; A. Holin; J. Hylen; G. M. Irwin; Z. Isvan; D. E. Jaffe; C. James; D. Jensen; T. Kafka; S. M S Kasahara; G. Koizumi; M. Kordosky; A. Kreymer; K. Lang; J. Ling; P. J. Litchfield; P. Lucas; W. A. Mann; M. L. Marshak; M. Mathis; N. Mayer; M. M. Medeiros; R. Mehdiyev; J. R. Meier; M. D. Messier; D. G. Michael; W. H. Miller; S. R. Mishra; S. Moed Sher; C. D. Moore; L. Mualem; J. Musser; D. Naples; J. K. Nelson; H. B. Newman; R. J. Nichol; J. A. Nowak; J. P. Ochoa-Ricoux; J. O'Connor; W. P. Oliver; M. Orchanian; R. B. Pahlka; J. Paley; R. B. Patterson; G. Pawloski; S. Phan-Budd; R. K. Plunkett; X. Qiu; A. Radovic; B. Rebel; C. Rosenfeld; H. A. Rubin; M. C. Sanchez; J. Schneps; A. Schreckenberger; P. Schreiner; R. Sharma; A. Sousa; N. Tagg; R. L. Talaga; J. Thomas; M. A. Thomson; G. Tinti; R. Toner; D. Torretta; G. Tzanakos; J. Urheim; P. Vahle; B. Viren; A. Weber; R. C. Webb; C. White; L. Whitehead; S. G. Wojcicki; T. Yang; R. Zwaska

doi:10.1103/PhysRevLett.110.171801

Electron neutrino and antineutrino appearance in the full MINOS data sample

P. Adamson, I. Anghel, C. Backhouse, G. Barr, M. Bishai, A. Blake, G. J. Bock, D. Bogert, S. V. Cao, D. Cherdack, S. Childress, J. A B Coelho, L. Corwin, D. Cronin-Hennessy, J. K. De Jong, A. V. Devan, N. E. Devenish, M. V. Diwan, C. O. Escobar, J. J. EvansE. Falk, G. J. Feldman, M. V. Frohne, H. R. Gallagher, R. A. Gomes, M. C. Goodman, P. Gouffon, N. Graf, R. Gran, K. Grzelak, A. Habig, S. R. Hahn, J. Hartnell, R. Hatcher, A. Himmel, A. Holin, J. Hylen, G. M. Irwin, Z. Isvan, D. E. Jaffe, C. James, D. Jensen, T. Kafka, S. M S Kasahara, G. Koizumi, M. Kordosky, A. Kreymer, K. Lang, J. Ling, P. J. Litchfield, P. Lucas, W. A. Mann, M. L. Marshak, M. Mathis, N. Mayer, M. M. Medeiros, R. Mehdiyev, J. R. Meier, M. D. Messier, D. G. Michael, W. H. Miller, S. R. Mishra, S. Moed Sher, C. D. Moore, L. Mualem, J. Musser, D. Naples, J. K. Nelson, H. B. Newman, R. J. Nichol, J. A. Nowak, J. P. Ochoa-Ricoux, J. O'Connor, W. P. Oliver, M. Orchanian, R. B. Pahlka, J. Paley, R. B. Patterson, G. Pawloski, S. Phan-Budd, R. K. Plunkett, X. Qiu, A. Radovic, B. Rebel, C. Rosenfeld, H. A. Rubin, M. C. Sanchez, J. Schneps, A. Schreckenberger, P. Schreiner, R. Sharma, A. Sousa, N. Tagg, R. L. Talaga, J. Thomas, M. A. Thomson, G. Tinti, R. Toner, D. Torretta, G. Tzanakos, J. Urheim, P. Vahle, B. Viren, A. Weber, R. C. Webb, C. White, L. Whitehead, S. G. Wojcicki, T. Yang, R. Zwaska

Research output: Contribution to journal › Article › peer-review

43 Downloads (Pure)

Abstract

We report on νe and ν̄e appearance in νμ and ν̄μ beams using the full MINOS data sample. The comparison of these νe and ν̄e appearance data at a 735 km baseline with θ13 measurements by reactor experiments probes δ, the θ23 octant degeneracy, and the mass hierarchy. This analysis is the first use of this technique and includes the first accelerator long-baseline search for ν ̄μ→ν̄e. Our data disfavor 31% (5%) of the three-parameter space defined by δ, the octant of the θ23, and the mass hierarchy at the 68% (90%) C.L. We measure a value of 2sin2(2θ13) sin2(θ23) that is consistent with reactor experiments. © 2013 American Physical Society.

Original language	English
Article number	171801
Journal	Physical Review Letters
Volume	110
Issue number	17
DOIs	https://doi.org/10.1103/PhysRevLett.110.171801
Publication status	Published - 22 Apr 2013

Access to Document

10.1103/PhysRevLett.110.171801

POST-PEER-REVIEW-NON-PUBLISHERS.PDFAccepted author manuscript, 326 KB

http://oai.aps.org/filefetch?identifier=10.1103/PhysRevLett.110.171801&component=fulltext&description=markup&format=xml

Cite this

Adamson, P., Anghel, I., Backhouse, C., Barr, G., Bishai, M., Blake, A., Bock, G. J., Bogert, D., Cao, S. V., Cherdack, D., Childress, S., Coelho, J. A. B., Corwin, L., Cronin-Hennessy, D., De Jong, J. K., Devan, A. V., Devenish, N. E., Diwan, M. V., Escobar, C. O., ... Zwaska, R. (2013). Electron neutrino and antineutrino appearance in the full MINOS data sample. Physical Review Letters, 110(17), Article 171801. https://doi.org/10.1103/PhysRevLett.110.171801

@article{5c305b0f7a6546b4a94c52763cf082d7,

title = "Electron neutrino and antineutrino appearance in the full MINOS data sample",

abstract = "We report on νe and {\=ν}e appearance in νμ and {\=ν}μ beams using the full MINOS data sample. The comparison of these νe and {\=ν}e appearance data at a 735 km baseline with θ13 measurements by reactor experiments probes δ, the θ23 octant degeneracy, and the mass hierarchy. This analysis is the first use of this technique and includes the first accelerator long-baseline search for ν{\= }μ→{\=ν}e. Our data disfavor 31% (5%) of the three-parameter space defined by δ, the octant of the θ23, and the mass hierarchy at the 68% (90%) C.L. We measure a value of 2sin2(2θ13) sin2(θ23) that is consistent with reactor experiments. {\textcopyright} 2013 American Physical Society.",

author = "P. Adamson and I. Anghel and C. Backhouse and G. Barr and M. Bishai and A. Blake and Bock, {G. J.} and D. Bogert and Cao, {S. V.} and D. Cherdack and S. Childress and Coelho, {J. A B} and L. Corwin and D. Cronin-Hennessy and {De Jong}, {J. K.} and Devan, {A. V.} and Devenish, {N. E.} and Diwan, {M. V.} and Escobar, {C. O.} and Evans, {J. J.} and E. Falk and Feldman, {G. J.} and Frohne, {M. V.} and Gallagher, {H. R.} and Gomes, {R. A.} and Goodman, {M. C.} and P. Gouffon and N. Graf and R. Gran and K. Grzelak and A. Habig and Hahn, {S. R.} and J. Hartnell and R. Hatcher and A. Himmel and A. Holin and J. Hylen and Irwin, {G. M.} and Z. Isvan and Jaffe, {D. E.} and C. James and D. Jensen and T. Kafka and Kasahara, {S. M S} and G. Koizumi and M. Kordosky and A. Kreymer and K. Lang and J. Ling and Litchfield, {P. J.} and P. Lucas and Mann, {W. A.} and Marshak, {M. L.} and M. Mathis and N. Mayer and Medeiros, {M. M.} and R. Mehdiyev and Meier, {J. R.} and Messier, {M. D.} and Michael, {D. G.} and Miller, {W. H.} and Mishra, {S. R.} and {Moed Sher}, S. and Moore, {C. D.} and L. Mualem and J. Musser and D. Naples and Nelson, {J. K.} and Newman, {H. B.} and Nichol, {R. J.} and Nowak, {J. A.} and Ochoa-Ricoux, {J. P.} and J. O'Connor and Oliver, {W. P.} and M. Orchanian and Pahlka, {R. B.} and J. Paley and Patterson, {R. B.} and G. Pawloski and S. Phan-Budd and Plunkett, {R. K.} and X. Qiu and A. Radovic and B. Rebel and C. Rosenfeld and Rubin, {H. A.} and Sanchez, {M. C.} and J. Schneps and A. Schreckenberger and P. Schreiner and R. Sharma and A. Sousa and N. Tagg and Talaga, {R. L.} and J. Thomas and Thomson, {M. A.} and G. Tinti and R. Toner and D. Torretta and G. Tzanakos and J. Urheim and P. Vahle and B. Viren and A. Weber and Webb, {R. C.} and C. White and L. Whitehead and Wojcicki, {S. G.} and T. Yang and R. Zwaska",

year = "2013",

month = apr,

day = "22",

doi = "10.1103/PhysRevLett.110.171801",

language = "English",

volume = "110",

journal = "Physical Review Letters",

issn = "0031-9007",

publisher = "American Physical Society",

number = "17",

}

Adamson, P, Anghel, I, Backhouse, C, Barr, G, Bishai, M, Blake, A, Bock, GJ, Bogert, D, Cao, SV, Cherdack, D, Childress, S, Coelho, JAB, Corwin, L, Cronin-Hennessy, D, De Jong, JK, Devan, AV, Devenish, NE, Diwan, MV, Escobar, CO, Evans, JJ, Falk, E, Feldman, GJ, Frohne, MV, Gallagher, HR, Gomes, RA, Goodman, MC, Gouffon, P, Graf, N, Gran, R, Grzelak, K, Habig, A, Hahn, SR, Hartnell, J, Hatcher, R, Himmel, A, Holin, A, Hylen, J, Irwin, GM, Isvan, Z, Jaffe, DE, James, C, Jensen, D, Kafka, T, Kasahara, SMS, Koizumi, G, Kordosky, M, Kreymer, A, Lang, K, Ling, J, Litchfield, PJ, Lucas, P, Mann, WA, Marshak, ML, Mathis, M, Mayer, N, Medeiros, MM, Mehdiyev, R, Meier, JR, Messier, MD, Michael, DG, Miller, WH, Mishra, SR, Moed Sher, S, Moore, CD, Mualem, L, Musser, J, Naples, D, Nelson, JK, Newman, HB, Nichol, RJ, Nowak, JA, Ochoa-Ricoux, JP, O'Connor, J, Oliver, WP, Orchanian, M, Pahlka, RB, Paley, J, Patterson, RB, Pawloski, G, Phan-Budd, S, Plunkett, RK, Qiu, X, Radovic, A, Rebel, B, Rosenfeld, C, Rubin, HA, Sanchez, MC, Schneps, J, Schreckenberger, A, Schreiner, P, Sharma, R, Sousa, A, Tagg, N, Talaga, RL, Thomas, J, Thomson, MA, Tinti, G, Toner, R, Torretta, D, Tzanakos, G, Urheim, J, Vahle, P, Viren, B, Weber, A, Webb, RC, White, C, Whitehead, L, Wojcicki, SG, Yang, T & Zwaska, R 2013, 'Electron neutrino and antineutrino appearance in the full MINOS data sample', Physical Review Letters, vol. 110, no. 17, 171801. https://doi.org/10.1103/PhysRevLett.110.171801

TY - JOUR

T1 - Electron neutrino and antineutrino appearance in the full MINOS data sample

AU - Adamson, P.

AU - Anghel, I.

AU - Backhouse, C.

AU - Barr, G.

AU - Bishai, M.

AU - Blake, A.

AU - Bock, G. J.

AU - Bogert, D.

AU - Cao, S. V.

AU - Cherdack, D.

AU - Childress, S.

AU - Coelho, J. A B

AU - Corwin, L.

AU - Cronin-Hennessy, D.

AU - De Jong, J. K.

AU - Devan, A. V.

AU - Devenish, N. E.

AU - Diwan, M. V.

AU - Escobar, C. O.

AU - Evans, J. J.

AU - Falk, E.

AU - Feldman, G. J.

AU - Frohne, M. V.

AU - Gallagher, H. R.

AU - Gomes, R. A.

AU - Goodman, M. C.

AU - Gouffon, P.

AU - Graf, N.

AU - Gran, R.

AU - Grzelak, K.

AU - Habig, A.

AU - Hahn, S. R.

AU - Hartnell, J.

AU - Hatcher, R.

AU - Himmel, A.

AU - Holin, A.

AU - Hylen, J.

AU - Irwin, G. M.

AU - Isvan, Z.

AU - Jaffe, D. E.

AU - James, C.

AU - Jensen, D.

AU - Kafka, T.

AU - Kasahara, S. M S

AU - Koizumi, G.

AU - Kordosky, M.

AU - Kreymer, A.

AU - Lang, K.

AU - Ling, J.

AU - Litchfield, P. J.

AU - Lucas, P.

AU - Mann, W. A.

AU - Marshak, M. L.

AU - Mathis, M.

AU - Mayer, N.

AU - Medeiros, M. M.

AU - Mehdiyev, R.

AU - Meier, J. R.

AU - Messier, M. D.

AU - Michael, D. G.

AU - Miller, W. H.

AU - Mishra, S. R.

AU - Moed Sher, S.

AU - Moore, C. D.

AU - Mualem, L.

AU - Musser, J.

AU - Naples, D.

AU - Nelson, J. K.

AU - Newman, H. B.

AU - Nichol, R. J.

AU - Nowak, J. A.

AU - Ochoa-Ricoux, J. P.

AU - O'Connor, J.

AU - Oliver, W. P.

AU - Orchanian, M.

AU - Pahlka, R. B.

AU - Paley, J.

AU - Patterson, R. B.

AU - Pawloski, G.

AU - Phan-Budd, S.

AU - Plunkett, R. K.

AU - Qiu, X.

AU - Radovic, A.

AU - Rebel, B.

AU - Rosenfeld, C.

AU - Rubin, H. A.

AU - Sanchez, M. C.

AU - Schneps, J.

AU - Schreckenberger, A.

AU - Schreiner, P.

AU - Sharma, R.

AU - Sousa, A.

AU - Tagg, N.

AU - Talaga, R. L.

AU - Thomas, J.

AU - Thomson, M. A.

AU - Tinti, G.

AU - Toner, R.

AU - Torretta, D.

AU - Tzanakos, G.

AU - Urheim, J.

AU - Vahle, P.

AU - Viren, B.

AU - Weber, A.

AU - Webb, R. C.

AU - White, C.

AU - Whitehead, L.

AU - Wojcicki, S. G.

AU - Yang, T.

AU - Zwaska, R.

PY - 2013/4/22

Y1 - 2013/4/22

N2 - We report on νe and ν̄e appearance in νμ and ν̄μ beams using the full MINOS data sample. The comparison of these νe and ν̄e appearance data at a 735 km baseline with θ13 measurements by reactor experiments probes δ, the θ23 octant degeneracy, and the mass hierarchy. This analysis is the first use of this technique and includes the first accelerator long-baseline search for ν ̄μ→ν̄e. Our data disfavor 31% (5%) of the three-parameter space defined by δ, the octant of the θ23, and the mass hierarchy at the 68% (90%) C.L. We measure a value of 2sin2(2θ13) sin2(θ23) that is consistent with reactor experiments. © 2013 American Physical Society.

AB - We report on νe and ν̄e appearance in νμ and ν̄μ beams using the full MINOS data sample. The comparison of these νe and ν̄e appearance data at a 735 km baseline with θ13 measurements by reactor experiments probes δ, the θ23 octant degeneracy, and the mass hierarchy. This analysis is the first use of this technique and includes the first accelerator long-baseline search for ν ̄μ→ν̄e. Our data disfavor 31% (5%) of the three-parameter space defined by δ, the octant of the θ23, and the mass hierarchy at the 68% (90%) C.L. We measure a value of 2sin2(2θ13) sin2(θ23) that is consistent with reactor experiments. © 2013 American Physical Society.

U2 - 10.1103/PhysRevLett.110.171801

DO - 10.1103/PhysRevLett.110.171801

M3 - Article

SN - 0031-9007

VL - 110

JO - Physical Review Letters

JF - Physical Review Letters

IS - 17

M1 - 171801

ER -

Electron neutrino and antineutrino appearance in the full MINOS data sample

Abstract

Access to Document

Fingerprint

Cite this