Testing Lorentz invariance and CPT conservation with NuMI neutrinos in the MINOS near detector.
Testing Lorentz invariance and CPT conservation with NuMI neutrinos in the MINOS near detector.
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DOI：
10.1103/physrevlett.101.151601
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发表时间：
2008-06
影响因子：
8.6
通讯作者：
P. Adamson;C. Andreopoulos;K. Arms;R. Armstrong;D. Auty;D. Ayres;B. Baller;G. Barr;W. Barrett;B. Becker;A. Belias;R. Bernstein;D. Bhattacharya;M. Bishai;A. Blake;G. Bock;J. Boehm;D. Boehnlein;D. Bogert;C. Bower;E. Buckley-Geer;S. Cavanaugh;J. D. Chapman;D. Cherdack;S. Childress;B. Choudhary;S. Coleman;A. Culling;J. D. Jong;M. Diwan;M. Dorman;M. Dorman;S. Dytman;C. Escobar;J. Evans;J. Evans;E. Harris;G. Feldman;M. Frohne;H. Gallagher;M. Goodman;P. Gouffon;R. Gran;E. Grashorn;N. Grossman;K. Grzelak;K. Grzelak;A. Habig;D. Harris;P. Harris;J. Hartnell;J. Hartnell;R. Hatcher;K. Heller;A. Himmel;A. Holin;J. Hylen;G. Irwin;M. Ishitsuka;D. Jaffe;C. James;D. Jensen;T. Kafka;S. Amcix;J. J. Kim-J.;G. Koizumi;S. Kopp;M. Kordosky;M. Kordosky;D. J. Koskinen;A. Kreymer;S. Kumaratunga;K. Lang;P. Litchfield;R. P. Litchfield;L. Loiacono;P. Lucas;J. Ma;W. A. Mann;M. Marshak;J. Marshall;N. Mayer;A. McGowan;A. McGowan;J. Meier;M. Messier;C. Metelko;D. Michael;J. Miller;W. Miller;S. Mishra;C. Moore;J. Morfín;L. Mualem;S. Mufson;S. Murgia;J. Musser;D. Naples;J. Nelson;H. Newman;R. Nichol;T. Nicholls;J. Ochoa-Ricoux;W. Oliver;R. Ospanov;J. Paley;V. Paolone;A. Para;T. Patzak;Z. Pavlovic;G. Pawloski;G. Pearce;C. Peck;D. Petyt;R. Pittam;R. Plunkett;A. Rahaman;R. Rameika;T. Raufer;B. Rebel;J. Reichenbacher;P. Rodrigues;C. Rosenfeld;H. Rubin;M. Sánchez;M. Sánchez;N. Saoulidou;J. Schneps;P. Schreiner;P. Shanahan;W. Smart;A. Sousa;B. Speakman;P. Stamoulis;M. Strait;N. Tagg;R. Talaga;M. Tavera;J. Thomas;J. Thompson;M. Thomson;J. Thron;G. Tinti;G. Tzanakos;J. Urheim;P. Vahle;P. Vahle;B. Viren;M. Watabe;A. Weber;R. Webb;A. Wehmann;N. West;C. White;S. Wojcicki;T. Yang;M. Zois;K. Zhang;R. Zwaska
中科院分区：
文献类型：
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作者：
P. Adamson;C. Andreopoulos;K. Arms;R. Armstrong;D. Auty;D. Ayres;B. Baller;G. Barr;W. Barrett;B. Becker;A. Belias;R. Bernstein;D. Bhattacharya;M. Bishai;A. Blake;G. Bock;J. Boehm;D. Boehnlein;D. Bogert;C. Bower;E. Buckley-Geer;S. Cavanaugh;J. D. Chapman;D. Cherdack;S. Childress;B. Choudhary;S. Coleman;A. Culling;J. D. Jong;M. Diwan;M. Dorman;M. Dorman;S. Dytman;C. Escobar;J. Evans;J. Evans;E. Harris;G. Feldman;M. Frohne;H. Gallagher;M. Goodman;P. Gouffon;R. Gran;E. Grashorn;N. Grossman;K. Grzelak;K. Grzelak;A. Habig;D. Harris;P. Harris;J. Hartnell;J. Hartnell;R. Hatcher;K. Heller;A. Himmel;A. Holin;J. Hylen;G. Irwin;M. Ishitsuka;D. Jaffe;C. James;D. Jensen;T. Kafka;S. Amcix;J. J. Kim-J.;G. Koizumi;S. Kopp;M. Kordosky;M. Kordosky;D. J. Koskinen;A. Kreymer;S. Kumaratunga;K. Lang;P. Litchfield;R. P. Litchfield;L. Loiacono;P. Lucas;J. Ma;W. A. Mann;M. Marshak;J. Marshall;N. Mayer;A. McGowan;A. McGowan;J. Meier;M. Messier;C. Metelko;D. Michael;J. Miller;W. Miller;S. Mishra;C. Moore;J. Morfín;L. Mualem;S. Mufson;S. Murgia;J. Musser;D. Naples;J. Nelson;H. Newman;R. Nichol;T. Nicholls;J. Ochoa-Ricoux;W. Oliver;R. Ospanov;J. Paley;V. Paolone;A. Para;T. Patzak;Z. Pavlovic;G. Pawloski;G. Pearce;C. Peck;D. Petyt;R. Pittam;R. Plunkett;A. Rahaman;R. Rameika;T. Raufer;B. Rebel;J. Reichenbacher;P. Rodrigues;C. Rosenfeld;H. Rubin;M. Sánchez;M. Sánchez;N. Saoulidou;J. Schneps;P. Schreiner;P. Shanahan;W. Smart;A. Sousa;B. Speakman;P. Stamoulis;M. Strait;N. Tagg;R. Talaga;M. Tavera;J. Thomas;J. Thompson;M. Thomson;J. Thron;G. Tinti;G. Tzanakos;J. Urheim;P. Vahle;P. Vahle;B. Viren;M. Watabe;A. Weber;R. Webb;A. Wehmann;N. West;C. White;S. Wojcicki;T. Yang;M. Zois;K. Zhang;R. Zwaska
在MINOS近探测器中微子数据中进行了恒星调制的搜索。如果存在的话，这个签名可能是洛伦兹和CPT破坏的结果，正如被称为标准模型扩展的有效场论所预测的那样。在数据集中没有发现恒星信号的证据，这意味着在太阳中心惯性系中，中微子传播没有显著的变化，这取决于中微子束的方向。在标准模型扩展中，洛伦兹和CPT违反项的幅度上限在最大预期值的10（-4）和10（-2）之间，假设这些特征被抑制10（-17）倍。
A search for a sidereal modulation in the MINOS near detector neutrino data was performed. If present, this signature could be a consequence of Lorentz and CPT violation as predicted by the effective field theory called the standard-model extension. No evidence for a sidereal signal in the data set was found, implying that there is no significant change in neutrino propagation that depends on the direction of the neutrino beam in a sun-centered inertial frame. Upper limits on the magnitudes of the Lorentz and CPT violating terms in the standard-model extension lie between 10(-4) and 10(-2) of the maximum expected, assuming a suppression of these signatures by a factor of 10(-17).