Home > Research > Publications & Outputs > Electron neutrino and antineutrino appearance i...

Electronic data

  • PhysRevLett.110.171801

    Rights statement: © 2013 American Physical Society

    Final published version, 369 KB, PDF document

Links

Text available via DOI:

View graph of relations

Electron neutrino and antineutrino appearance in the full MINOS data sample

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Published

Standard

Electron neutrino and antineutrino appearance in the full MINOS data sample. / MINOS Collaboration.
In: Physical review letters, Vol. 110, No. 17, 171801, 22.04.2013.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

MINOS Collaboration 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

APA

Vancouver

MINOS Collaboration. Electron neutrino and antineutrino appearance in the full MINOS data sample. Physical review letters. 2013 Apr 22;110(17):171801. doi: 10.1103/PhysRevLett.110.171801

Author

MINOS Collaboration. / Electron neutrino and antineutrino appearance in the full MINOS data sample. In: Physical review letters. 2013 ; Vol. 110, No. 17.

Bibtex

@article{f055aab7c678495aa5c496af689fe80d,
title = "Electron neutrino and antineutrino appearance in the full MINOS data sample",
abstract = "We report on νe and ν̅ e appearance in νμ and ν̅ μ beams using the full MINOS data sample. The comparison of these νe and ν̅ 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 ν̅ μ→ν̅ 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 2sin⁡2(2θ13)sin⁡2(θ23) that is consistent with reactor experiments.",
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 Nowak, {J. A.} and {MINOS Collaboration}",
note = "{\textcopyright} 2013 American Physical Society",
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",

}

RIS

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 - Nowak, J. A.

AU - MINOS Collaboration

N1 - © 2013 American Physical Society

PY - 2013/4/22

Y1 - 2013/4/22

N2 - We report on νe and ν̅ e appearance in νμ and ν̅ μ beams using the full MINOS data sample. The comparison of these νe and ν̅ 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 ν̅ μ→ν̅ 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 2sin⁡2(2θ13)sin⁡2(θ23) that is consistent with reactor experiments.

AB - We report on νe and ν̅ e appearance in νμ and ν̅ μ beams using the full MINOS data sample. The comparison of these νe and ν̅ 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 ν̅ μ→ν̅ 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 2sin⁡2(2θ13)sin⁡2(θ23) that is consistent with reactor experiments.

U2 - 10.1103/PhysRevLett.110.171801

DO - 10.1103/PhysRevLett.110.171801

M3 - Journal article

VL - 110

JO - Physical review letters

JF - Physical review letters

SN - 0031-9007

IS - 17

M1 - 171801

ER -