Search for Sterile Neutrinos Mixing with Muon Neutrinos in MINOS.

Search for Sterile Neutrinos Mixing with Muon Neutrinos in MINOS.
复制标题

DOI:
10.1103/physrevlett.117.151803
复制
发表时间:
2016-07
影响因子:
8.6
通讯作者:
P. Adamson;I. Anghel;I. Anghel;A. Aurisano;G. Barr;M. Bishai;A. Blake;A. Blake;G. Bock;D. Bogert;S. Cao;T. Carroll;C. Castromonte;R. Chen;S. Childress;J. Coelho;L. Corwin;L. Corwin;D. Cronin-Hennessy;J. D. Jong;S. Rijck;A. Devan;N. Devenish;M. Diwan;C. Escobar;J. Evans;E. Falk;G. Feldman;W. Flanagan;M. Frohne;M. Frohne;M. Gabrielyan;H. Gallagher;S. Germani;R. Gomes;M. Goodman;P. Gouffon;N. Graf;R. Gran;K. Grzelak;A. Habig;S. Hahn;J. Hartnell;R. Hatcher;A. Holin;J. Huang;J. Hylen;G. Irwin;Z. Isvan;C. James;D. Jensen;T. Kafka;S. Amcix;G. Koizumi;M. Kordosky;A. Kreymer;K. Lang;P. Litchfield;P. Litchfield;P. Lucas;W. A. Mann;M. Marshak;N. Mayer;C. Mcgivern;M. M. Medeiros-M.;R. Mehdiyev;J. Meier;M. Messier;W. Miller;S. Mishra;S. M. Sher;C. Moore;L. Mualem;J. Musser;D. Naples;J. Nelson;H. Newman;R. Nichol;J. Nowak;J. Nowak;J. O’Connor;M. Orchanian;R. Pahlka;J. Paley;R. Patterson;G. Pawloski;A. Perch;M. Pfützner;D. Phan;S. Phan-Budd;R. Plunkett;N. Poonthottathil;X. Qiu;A. Radovic;B. Rebel;C. Rosenfeld;H. Rubin;P. Sail;M. Sánchez;M. Sánchez;J. Schneps;A. Schreckenberger;P. Schreiner;R. Sharma;A. Sousa;N. Tagg;R. Talaga;J. Thomas;M. Thomson;X. Tian;A. Timmons;J. Todd;S. Tognini;R. Toner;D. Torretta;G. Tzanakos;J. Urheim;P. Vahle;B. Viren;A. Weber;A. Weber;R. Webb;C. White;L. Whitehead;L. Whitehead;S. Wojcicki;R. Zwaska
P. Adamson;I. Anghel;I. Anghel;A. Aurisano;G. Barr;M. Bishai;A. Blake;A. Blake;G. Bock;D. Bogert;S. Cao;T. Carroll;C. Castromonte;R. Chen;S. Childress;J. Coelho;L. Corwin;L. Corwin;D. Cronin-Hennessy;J. D. Jong;S. Rijck;A. Devan;N. Devenish;M. Diwan;C. Escobar;J. Evans;E. Falk;G. Feldman;W. Flanagan;M. Frohne;M. Frohne;M. Gabrielyan;H. Gallagher;S. Germani;R. Gomes;M. Goodman;P. Gouffon;N. Graf;R. Gran;K. Grzelak;A. Habig;S. Hahn;J. Hartnell;R. Hatcher;A. Holin;J. Huang;J. Hylen;G. Irwin;Z. Isvan;C. James;D. Jensen;T. Kafka;S. Amcix;G. Koizumi;M. Kordosky;A. Kreymer;K. Lang;P. Litchfield;P. Litchfield;P. Lucas;W. A. Mann;M. Marshak;N. Mayer;C. Mcgivern;M. M. Medeiros-M.;R. Mehdiyev;J. Meier;M. Messier;W. Miller;S. Mishra;S. M. Sher;C. Moore;L. Mualem;J. Musser;D. Naples;J. Nelson;H. Newman;R. Nichol;J. Nowak;J. Nowak;J. O’Connor;M. Orchanian;R. Pahlka;J. Paley;R. Patterson;G. Pawloski;A. Perch;M. Pfützner;D. Phan;S. Phan-Budd;R. Plunkett;N. Poonthottathil;X. Qiu;A. Radovic;B. Rebel;C. Rosenfeld;H. Rubin;P. Sail;M. Sánchez;M. Sánchez;J. Schneps;A. Schreckenberger;P. Schreiner;R. Sharma;A. Sousa;N. Tagg;R. Talaga;J. Thomas;M. Thomson;X. Tian;A. Timmons;J. Todd;S. Tognini;R. Toner;D. Torretta;G. Tzanakos;J. Urheim;P. Vahle;B. Viren;A. Weber;A. Weber;R. Webb;C. White;L. Whitehead;L. Whitehead;S. Wojcicki;R. Zwaska
中科院分区:
物理与天体物理1区
文献类型:
--
作者:
P. Adamson;I. Anghel;I. Anghel;A. Aurisano;G. Barr;M. Bishai;A. Blake;A. Blake;G. Bock;D. Bogert;S. Cao;T. Carroll;C. Castromonte;R. Chen;S. Childress;J. Coelho;L. Corwin;L. Corwin;D. Cronin-Hennessy;J. D. Jong;S. Rijck;A. Devan;N. Devenish;M. Diwan;C. Escobar;J. Evans;E. Falk;G. Feldman;W. Flanagan;M. Frohne;M. Frohne;M. Gabrielyan;H. Gallagher;S. Germani;R. Gomes;M. Goodman;P. Gouffon;N. Graf;R. Gran;K. Grzelak;A. Habig;S. Hahn;J. Hartnell;R. Hatcher;A. Holin;J. Huang;J. Hylen;G. Irwin;Z. Isvan;C. James;D. Jensen;T. Kafka;S. Amcix;G. Koizumi;M. Kordosky;A. Kreymer;K. Lang;P. Litchfield;P. Litchfield;P. Lucas;W. A. Mann;M. Marshak;N. Mayer;C. Mcgivern;M. M. Medeiros-M.;R. Mehdiyev;J. Meier;M. Messier;W. Miller;S. Mishra;S. M. Sher;C. Moore;L. Mualem;J. Musser;D. Naples;J. Nelson;H. Newman;R. Nichol;J. Nowak;J. Nowak;J. O’Connor;M. Orchanian;R. Pahlka;J. Paley;R. Patterson;G. Pawloski;A. Perch;M. Pfützner;D. Phan;S. Phan-Budd;R. Plunkett;N. Poonthottathil;X. Qiu;A. Radovic;B. Rebel;C. Rosenfeld;H. Rubin;P. Sail;M. Sánchez;M. Sánchez;J. Schneps;A. Schreckenberger;P. Schreiner;R. Sharma;A. Sousa;N. Tagg;R. Talaga;J. Thomas;M. Thomson;X. Tian;A. Timmons;J. Todd;S. Tognini;R. Toner;D. Torretta;G. Tzanakos;J. Urheim;P. Vahle;B. Viren;A. Weber;A. Weber;R. Webb;C. White;L. Whitehead;L. Whitehead;S. Wojcicki;R. Zwaska

文献摘要

被引文献

相似文献

我们报道了在峰值能量为3GeV的ν_{μ主控光束中,在1.04千米和735千米范围内涉及轻不育中微子的振荡的研究结果。用唯象模型对10.56×10^{20}质子在靶上的曝光数据进行了分析。我们约束了混合参数θ_{24}和Δm_{41}^{2},并对四维Pontecorvo-Maki-Nakagawa-Sakata矩阵|U_{μ4}|^{2}和|U_{τ4}|^{2}的参数进行了限制,假设ν_{e}和ν_{S}之间的混合可以忽略(|U_{e4}|^{2}=0)。没有发现ν_{μ}→ν_{S}转变的证据,我们在θ_{24}上设定了Δm_{41}^{2}≲1 ev^{2}的值的世界领先的限制。
We report results of a search for oscillations involving a light sterile neutrino over distances of 1.04 and 735 km in a ν_{μ}-dominated beam with a peak energy of 3 GeV. The data, from an exposure of 10.56×10^{20} protons on target, are analyzed using a phenomenological model with one sterile neutrino. We constrain the mixing parameters θ_{24} and Δm_{41}^{2} and set limits on parameters of the four-dimensional Pontecorvo-Maki-Nakagawa-Sakata matrix, |U_{μ4}|^{2} and |U_{τ4}|^{2}, under the assumption that mixing between ν_{e} and ν_{s} is negligible (|U_{e4}|^{2}=0). No evidence for ν_{μ}→ν_{s} transitions is found and we set a world-leading limit on θ_{24} for values of Δm_{41}^{2}≲1 eV^{2}.