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arXiv:1403.0867v2 [hep-ex] 10 May 2014
FERMILAB-PUB-14-028-E-PPD
Combined analysis of ν
µ
disappearance and ν
µ
→ ν
e
appearance in MINOS using
accelerator and atmospheric neutrinos
P. Adamson,
8
I. Anghel,
15, 1
A. Aurisano,
7
G. Barr,
21
M. Bishai,
3
A. Blake,
5
G. J. Bock,
8
D. Bogert,
8
S. V. Cao,
29
C. M. Castromonte,
9
D. Cherdack,
30
S. Childre ss,
8
J. A. B. Coelho,
30, 6
L. Corwin,
14
D. Cronin-Hennessy,
18
J. K. de Jong,
21
A. V. Devan,
32
N. E. Devenish,
27
M. V. Diwan,
3
C. O. Escobar,
6
J. J. Evans,
17
E. Falk,
27
G. J. Feldman,
10
M. V. Frohne,
11
H. R. Gallagher,
30
R. A. Gomes,
9
M. C. Goodman,
1
P. Gouffon,
24
N. Graf,
22, 13
R. Gran,
19
K. Grzelak,
31
A. Habig,
19
S. R. Hahn,
8
J. Hartnell,
27
R. Hatcher,
8
A. Himmel,
4
A. Holin,
16
J. Huang,
29
J. Hylen,
8
G. M. Irwin,
26
Z. Isvan,
3, 22
C. James,
8
D. Jensen,
8
T. Kafka,
30
S. M. S. Kasahara,
18
G. Koizumi,
8
M. Kordosky,
32
A. Kreymer,
8
K. Lang,
29
J. Ling,
3
P. J. Litchfield,
18, 23
P. Lucas,
8
W. A. Mann,
30
M. L. Marshak,
18
N. Mayer,
30, 14
C. Mc Givern,
22
M. M. Medeiros,
9
R. Mehdiyev,
29
J. R. Meie r,
18
M. D. Messier,
14
D. G. Michael,
4, ∗
W. H. Miller,
18
S. R. Mishra,
25
S. Moed Sher,
8
C. D. Moore,
8
L. Mualem,
4
J. Musser,
14
D. Naples,
22
J. K. Nelson,
32
H. B. Newman,
4
R. J. Nichol,
16
J. A. Nowak,
18
J. O’Connor,
16
M. Orchanian,
4
R. B. Pahlka,
8
J. Paley,
1
R. B. Patterson,
4
G. Pawloski,
18, 26
A. Perch,
16
S. Phan-Budd,
1
R. K. Plunkett,
8
N. Poonthottathil,
8
X. Qiu,
26
A. Radovic,
32, 16
B. Rebel,
8
C. Rosenfeld,
25
H. A. Rubin,
13
M. C. Sanchez,
15, 1
J. Schneps,
30
A. Schreckenberger,
29, 18
P. Schreiner,
1
R. Sharma,
8
A. Sousa,
7, 10
N. Tagg,
20
R. L. Talaga,
1
J. Thomas,
16
M. A. Thomson,
5
X. Tian,
25
A. Timmons,
17
S. C. Tognini,
9
R. Toner,
10, 5
D. Torretta,
8
G. Tzanakos,
2, ∗
J. Urheim,
14
P. Vahle,
32
B. Viren,
3
A. Weber,
21, 23
R. C. Webb,
28
C. White,
13
L. Whitehead,
12, 3
L. H. Whitehead,
16
S. G. Wojcicki,
26
and R. Zwaska
8
(The MINOS Collaboration)
1
Argonne National Laboratory, Argonne, Illinois 60439, USA
2
Department of Physics, University of Athens, GR-15771 Athens, Greece
3
Brookhaven National Laboratory, Upton, New York 11973, USA
4
Lauritsen Laboratory, California I nstitute of Technology, Pasadena, California 91125, USA
5
Cavendish Laboratory, University of Cambridge, Madingley Road, Cambridge CB3 0HE, United Kingdom
6
Universidade Estadual de Campinas, I FGW-UNICAMP, CP 6165, 13083-970, Campinas, SP, Brazil
7
Department of Physics, University of Cincinnati, Cincinnati, Ohio 45221, USA
8
Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
9
Instituto de F´ısica, Universidade Federal de Goi´as, CP 131, 74001-970, Goiˆania, GO, Brazil
10
Department of Physics, Harvard University, Cambridge, Massachusetts 02138, USA
11
Holy Cross College, Notre Dame, Indiana 46556, USA
12
Department of Physics, University of Houston, Houston, Texas 77204, USA
13
Department of Physics, I llinois Institute of Technology, Chicago, Illinois 60616, USA
14
Indiana University, Bloomington, Indiana 47405, USA
15
Department of Physics and A stronomy, Iowa State University, Ames, Iowa 50011 USA
16
Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, United Kingdom
17
School of Physics and Astronomy, University of Manchester, Oxford Road, Manchester M13 9PL, United Kingdom
18
University of Minnesota, M inneapolis, Minnesota 55455, USA
19
Department of Physics, University of Minnesota Duluth, Duluth, Minnesota 55812, USA
20
Otterbein College, Westerville, Ohio 43081, USA
21
Subdepartment of Particle Physics, University of Oxford, Oxford OX1 3RH, United Kingdom
22
Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, Pennsylvania 15260, USA
23
Rutherford Appleton Laboratory, Science and Technologies Facilities Council, Didcot, OX11 0QX, United Kingdom
24
Instituto de F´ısica, Universidade de S˜ao Paulo, CP 66318, 05315-970, S˜ao Paulo, SP, Brazil
25
Department of Physics and Astronomy, University of South Carolina, Columbia, South Carolina 29208, USA
26
Department of Physics, Stanford University, Stanford, California 94305, USA
27
Department of Physics and Astronomy, University of Sussex, Falmer, Brighton BN1 9QH, United Kingdom
28
Physics Department, Texas A&M University, College Station, Texas 77843, USA
29
Department of Physics, University of Texas at Austin, 1 U niversity Station C1600, Austin, Texas 78712, USA
30
Physics Department, Tuf ts University, Medford, Massachusetts 02155, USA
31
Department of Physics, University of Warsaw, Ho˙za 69, PL-00-681 Warsaw, Poland
32
Department of Physics, Coll ege of William & Mary, Williamsburg, Virginia 23187, USA
(Dated: May 13, 2014)
We report on a new analysis of neu trino oscillations in MINOS using the complete set of accelerator
and atmospheric data. The an alysis combines the ν
µ
disappearance and ν
e
appearance data using
the three-flavor formalism. We measure |∆m
2
32
| = [2.28−2.46]×10
−3
eV
2
(68% C.L.) and sin
2
θ
23
=
0.35 − 0.65 (90% C.L.) in the normal hierarchy, and |∆m
2
32
| = [2.32 − 2.53] × 10
−3
eV
2
(68% C.L.)
and sin
2
θ
23
= 0.34 − 0.67 (90% C.L.) in the inverted hierarchy. The data also constrain δ
CP
, the
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