First direct observation of muon antineutrino disappearance.
First direct observation of muon antineutrino disappearance.
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DOI:
10.1103/physrevlett.107.021801
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发表时间:
2011-04
影响因子:
8.6
通讯作者:
P. Adamson;C. Andreopoulos;D. Auty;D. Ayres;C. Backhouse;G. Barr;M. Bishai;A. Blake;G. Bock;D. Boehnlein;D. Bogert;S. Cavanaugh;D. Cherdack;S. Childress;B. Choudhary;J. Coelho;S. Coleman;L. Corwin;D. Cronin-Hennessy;I. Dankó;J. D. Jong;N. Devenish;M. Diwan;M. Dorman;C. Escobar;J. Evans;E. Falk;G. Feldman;M. Frohne;H. Gallagher;R. Gomes;M. Goodman;P. Gouffon;N. Graf;R. Gran;N. Grant;K. Grzelak;A. Habig;D. Harris;J. Hartnell;J. Hartnell;R. Hatcher;A. Himmel;A. Holin;C. Howcroft;X. Huang;J. Hylen;J. Ilic;G. Irwin;Z. Isvan;D. Jaffe;C. James;D. Jensen;T. Kafka;S. Amcix;G. Koizumi;S. Kopp;M. Kordosky;A. Kreymer;K. Lang;G. Lefeuvre;P. Litchfield;P. Litchfield;L. Loiacono;P. Lucas;W. A. Mann;M. Marshak;N. Mayer;A. McGowan;R. Mehdiyev;J. Meier;M. Messier;W. Miller;S. Mishra;J. Mitchell;C. Moore;J. Morfín;L. Mualem;S. Mufson;J. Musser;D. Naples;J. Nelson;H. Newman;R. Nichol;T. Nicholls;J. Nowak;J. Ochoa-Ricoux;W. Oliver;M. Orchanian;R. Ospanov;J. Paley;J. Paley;R. Patterson;G. Pawloski;G. Pearce;D. Petyt;S. Phan-Budd;R. Plunkett;X. Qiu;J. Ratchford;T. Raufer;B. Rebel;P. Rodrigues;C. Rosenfeld;H. Rubin;M. Sánchez;M. Sánchez;M. Sánchez;J. Schneps;P. Schreiner;P. Shanahan;A. Sousa;P. Stamoulis;M. Strait;N. Tagg;R. Talaga;E. Tetteh-Lartey;J. Thomas;M. Thomson;G. Tinti;R. Toner;G. Tzanakos;J. Urheim;P. Vahle;B. Viren;A. Weber;R. Webb;C. White;L. Whitehead;S. Wojcicki;T. Yang;R. Zwaska
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文献类型:
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作者:
P. Adamson;C. Andreopoulos;D. Auty;D. Ayres;C. Backhouse;G. Barr;M. Bishai;A. Blake;G. Bock;D. Boehnlein;D. Bogert;S. Cavanaugh;D. Cherdack;S. Childress;B. Choudhary;J. Coelho;S. Coleman;L. Corwin;D. Cronin-Hennessy;I. Dankó;J. D. Jong;N. Devenish;M. Diwan;M. Dorman;C. Escobar;J. Evans;E. Falk;G. Feldman;M. Frohne;H. Gallagher;R. Gomes;M. Goodman;P. Gouffon;N. Graf;R. Gran;N. Grant;K. Grzelak;A. Habig;D. Harris;J. Hartnell;J. Hartnell;R. Hatcher;A. Himmel;A. Holin;C. Howcroft;X. Huang;J. Hylen;J. Ilic;G. Irwin;Z. Isvan;D. Jaffe;C. James;D. Jensen;T. Kafka;S. Amcix;G. Koizumi;S. Kopp;M. Kordosky;A. Kreymer;K. Lang;G. Lefeuvre;P. Litchfield;P. Litchfield;L. Loiacono;P. Lucas;W. A. Mann;M. Marshak;N. Mayer;A. McGowan;R. Mehdiyev;J. Meier;M. Messier;W. Miller;S. Mishra;J. Mitchell;C. Moore;J. Morfín;L. Mualem;S. Mufson;J. Musser;D. Naples;J. Nelson;H. Newman;R. Nichol;T. Nicholls;J. Nowak;J. Ochoa-Ricoux;W. Oliver;M. Orchanian;R. Ospanov;J. Paley;J. Paley;R. Patterson;G. Pawloski;G. Pearce;D. Petyt;S. Phan-Budd;R. Plunkett;X. Qiu;J. Ratchford;T. Raufer;B. Rebel;P. Rodrigues;C. Rosenfeld;H. Rubin;M. Sánchez;M. Sánchez;M. Sánchez;J. Schneps;P. Schreiner;P. Shanahan;A. Sousa;P. Stamoulis;M. Strait;N. Tagg;R. Talaga;E. Tetteh-Lartey;J. Thomas;M. Thomson;G. Tinti;R. Toner;G. Tzanakos;J. Urheim;P. Vahle;B. Viren;A. Weber;R. Webb;C. White;L. Whitehead;S. Wojcicki;T. Yang;R. Zwaska
This Letter reports the first direct observation of muon antineutrino disappearance. The MINOS experiment has taken data with an accelerator beam optimized for ν(μ) production, accumulating an exposure of 1.71 × 10²⁰ protons on target. In the Far Detector, 97 charged current ν(μ) events are observed. The no-oscillation hypothesis predicts 156 events and is excluded at 6.3σ. The best fit to oscillation yields |Δm²| = [3.36(-0.40)(+0.46)(stat) ± 0.06(syst)] × 10⁻³ eV², sin²(2θ) = 0.86(-0.12)(+0.11)(stat) ± 0.01(syst). The MINOS ν(μ) and ν(μ) measurements are consistent at the 2.0% confidence level, assuming identical underlying oscillation parameters.