N. Tagg - MicroBooNE Collaboration

N. Tagg
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N. Tagg
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MicroBooNE Collaboration
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High Energy Physics - Experiment (49)
 
Physics - Instrumentation and Detectors (15)
 
Nuclear Experiment (7)
 
High Energy Physics - Phenomenology (6)
 
Instrumentation and Methods for Astrophysics (1)
 
Physics - Accelerator Physics (1)

Publications Authored By N. Tagg

2017May
Authors: MicroBooNE collaboration, R. Acciarri, C. Adams, R. An, J. Anthony, J. Asaadi, M. Auger, L. Bagby, S. Balasubramanian, B. Baller, C. Barnes, G. Barr, M. Bass, F. Bay, M. Bishai, A. Blake, T. Bolton, B. Bullard, L. Camilleri, D. Caratelli, B. Carls, R. Castillo Fernandez, F. Cavanna, H. Chen, E. Church, D. Cianci, E. Cohen, G. H. Collin, J. M. Conrad, M. Convery, J. I. Crespo-Anadon, G. De Geronimo, M. Del Tutto, D. Devitt, S. Dytman, B. Eberly, A. Ereditato, L. Escudero Sanchez, J. Esquivel, A. A. Fadeeva, B. T. Fleming, W. Foreman, A. P. Furmanski, D. Garcia-Gamez, G. T. Garvey, V. Genty, D. Goeldi, S. Gollapinni, N. Graf, E. Gramellini, H. Greenlee, R. Grosso, R. Guenette, A. Hackenburg, P. Hamilton, O. Hen, J. Hewes, C. Hill, J. Ho, G. Horton-Smith, A. Hourlier, E. -C. Huang, C. James, J. Jan de Vries, C. -M. Jen, L. Jiang, R. A. Johnson, J. Joshi, H. Jostlein, D. Kaleko, G. Karagiorgi, W. Ketchum, B. Kirby, M. Kirby, T. Kobilarcik, I. Kreslo, A. Laube, S. Li, Y. Li, A. Lister, B. R. Littlejohn, S. Lockwitz, D. Lorca, W. C. Louis, M. Luethi, B. Lundberg, X. Luo, A. Marchionni, C. Mariani, J. Marshall, D. A. Martinez Caicedo, V. Meddage, T. Miceli, G. B. Mills, J. Moon, M. Mooney, C. D. Moore, J. Mousseau, R. Murrells, D. Naples, P. Nienaber, J. Nowak, O. Palamara, V. Paolone, V. Papavassiliou, S. F. Pate, Z. Pavlovic, E. Piasetzky, D. Porzio, G. Pulliam, X. Qian, J. L. Raaf, V. Radeka, A. Rafique, S. Rescia, L. Rochester, C. Rudolf von Rohr, B. Russell, D. W. Schmitz, A. Schukraft, W. Seligman, M. H. Shaevitz, J. Sinclair, A. Smith, E. L. Snider, M. Soderberg, S. Soldner-Rembold, S. R. Soleti, P. Spentzouris, J. Spitz, J. St. John, T. Strauss, A. M. Szelc, N. Tagg, K. Terao, M. Thomson, C. Thorn, M. Toups, Y. -T. Tsai, S. Tufanli, T. Usher, W. Van De Pontseele, R. G. Van de Water, B. Viren, M. Weber, D. A. Wickremasinghe, S. Wolbers, T. Wongjirad, K. Woodruff, T. Yang, L. Yates, B. Yu, G. P. Zeller, J. Zennamo, C. Zhang

The low-noise operation of readout electronics in a liquid argon time projection chamber (LArTPC) is critical to properly extract the distribution of ionization charge deposited on the wire planes of the TPC, especially for the induction planes. This paper describes the characteristics and mitigation of the observed noise in the MicroBooNE detector. The MicroBooNE's single-phase LArTPC comprises two induction planes and one collection sense wire plane with a total of 8256 wires. Read More

2017Apr
Authors: MicroBooNE collaboration, R. Acciarri, C. Adams, R. An, J. Anthony, J. Asaadi, M. Auger, L. Bagby, S. Balasubramanian, B. Baller, C. Barnes, G. Barr, M. Bass, F. Bay, M. Bishai, A. Blake, T. Bolton, L. Bugel, L. Camilleri, D. Caratelli, B. Carls, R. Castillo Fernandez, F. Cavanna, H. Chen, E. Church, D. Cianci, E. Cohen, G. H. Collin, J. M. Conrad, M. Convery, J. I. Crespo-Anadon, M. Del Tutto, D. Devitt, S. Dytman, B. Eberly, A. Ereditato, L. Escudero Sanchez, J. Esquivel, B. T. Fleming, W. Foreman, A. P. Furmanski, D. Garcia-Gomez, G. T. Garvey, V. Genty, D. Goeldi, S. Gollapinni, N. Graf, E. Gramellini, H. Greenlee, R. Grosso, R. Guenette, A. Hackenburg, P. Hamilton, O. Hen, J. Hewes, C. Hill, J. Ho, G. Horton-Smith, E. -C. Huang, C. James, J. Jan de Vries, C. -M. Jen, L. Jiang, R. A. Johnson, J. Joshi, H. Jostlein, D. Kaleko, G. Karagiorgi, W. Ketchum, B. Kirby, M. Kirby, T. Kobilarcik, I. Kreslo, A. Laube, Y. Li, A. Lister, B. R. Littlejohn, S. Lockwitz, D. Lorca, W. C. Louis, M. Luethi, B. Lundberg, X. Luo, A. Marchionni, C. Mariani, J. Marshall, D. A. Martinez Caicedo, V. Meddage, T. Miceli, G. B. Mills, J. Moon, M. Mooney, C. D. Moore, J. Mousseau, R. Murrells, D. Naples, P. Nienaber, J. Nowak, O. Palamara, V. Paolone, V. Papavassiliou, S. F. Pate, Z. Pavlovic, E. Piasetzky, D. Porzio, G. Pulliam, X. Qian, J. L. Raaf, A. Rafique, L. Rochester, C. Rudolf von Rohr, B. Russell, D. W. Schmitz, A. Schukraft, W. Seligman, M. H. Shaevitz, J. Sinclair, E. L. Snider, M. Soderberg, S. Soldner-Rembold, S. R. Soleti, P. Spentzouris, J. Spitz, J. St. John, T. Strauss, K. A. Sutton, A. M. Szelc, N. Tagg, K. Terao, M. Thomson, M. Toups, Y. -T. Tsai, S. Tufanli, T. Usher, R. G. Van de Water, B. Viren, M. Weber, D. A. Wickremasinghe, S. Wolbers, T. Wongjirad, K. Woodruff, T. Yang, L. Yates, G. P. Zeller, J. Zennamo, C. Zhang

The MicroBooNE liquid argon time projection chamber (LArTPC) has been taking data at Fermilab since 2015 collecting, in addition to neutrino beam, cosmic-ray muons. Results are presented on the reconstruction of Michel electrons produced by the decay at rest of cosmic-ray muons. Michel electrons are abundantly produced in the TPC, and given their well known energy spectrum can be used to study MicroBooNE's detector response to low-energy electrons (electrons with energies up to ~50 MeV). Read More

2017Mar
Authors: MicroBooNE collaboration, P. Abratenko, R. Acciarri, C. Adams, R. An, J. Asaadi, M. Auger, L. Bagby, S. Balasubramanian, B. Baller, C. Barnes, G. Barr, M. Bass, F. Bay, M. Bishai, A. Blake, T. Bolton, L. Bugel, L. Camilleri, D. Caratelli, B. Carls, R. Castillo Fernandez, F. Cavanna, H. Chen, E. Church, D. Cianci, E. Cohen, G. H. Collin, J. M. Conrad, M. Convery, J. I. Crespo-Anadon, M. Del Tutto, D. Devitt, S. Dytman, B. Eberly, A. Ereditato, L. Escudero Sanchez, J. Esquivel, B. T. Fleming, W. Foreman, A. P. Furmanski, D. Garcia-Gomez, G. T. Garvey, V. Genty, D. Goeldi, S. Gollapinni, N. Graf, E. Gramellini, H. Greenlee, R. Grosso, R. Guenette, A. Hackenburg, P. Hamilton, O. Hen, J. Hewes, C. Hill, J. Ho, G. Horton-Smith, E. -C. Huang, C. James, J. Jan de Vries, C. -M. Jen, L. Jiang, R. A. Johnson, B. J. P. Jones, J. Joshi, H. Jostlein, D. Kaleko, L. N. Kalousis, G. Karagiorgi, W. Ketchum, B. Kirby, M. Kirby, T. Kobilarcik, I. Kreslo, A. Laube, Y. Li, A. Lister, B. R. Littlejohn, S. Lockwitz, D. Lorca, W. C. Louis, M. Luethi, B. Lundberg, X. Luo, A. Marchionni, C. Mariani, J. Marshall, D. A. Martinez Caicedo, V. Meddage, T. Miceli, G. B. Mills, J. Moon, M. Mooney, C. D. Moore, J. Mousseau, R. Murrells, D. Naples, P. Nienaber, J. Nowak, O. Palamara, V. Paolone, V. Papavassiliou, S. F. Pate, Z. Pavlovic, E. Piasetzky, D. Porzio, G. Pulliam, X. Qian, J. L. Raaf, A. Rafique, L. Rochester, C. Rudolf von Rohr, B. Russell, D. W. Schmitz, A. Schukraft, W. Seligman, M. H. Shaevitz, J. Sinclair, E. L. Snider, M. Soderberg, S. Soldner-Rembold, S. R. Soleti, P. Spentzouris, J. Spitz, J. St. John, T. Strauss, A. M. Szelc, N. Tagg, K. Terao, M. Thomson, M. Toups, Y. -T. Tsai, S. Tufanli, T. Usher, R. G. Van de Water, B. Viren, M. Weber, J. Weston, D. A. Wickremasinghe, S. Wolbers, T. Wongjirad, K. Woodruff, T. Yang, L. Yates, G. P. Zeller, J. Zennamo, C. Zhang

We discuss a technique for measuring a charged particle's momentum by means of multiple Coulomb scattering (MCS) in the MicroBooNE liquid argon time projection chamber (LArTPC). This method does not require the full particle ionization track to be contained inside of the detector volume as other track momentum reconstruction methods do (range-based momentum reconstruction and calorimetric momentum reconstruction). We motivate use of this technique, describe a tuning of the underlying phenomenological formula, quantify its performance on fully contained beam-neutrino-induced muon tracks both in simulation and in data, and quantify its performance on exiting muon tracks in simulation. Read More

2016Dec
Authors: MicroBooNE Collaboration, R. Acciarri, C. Adams, R. An, A. Aparicio, S. Aponte, J. Asaadi, M. Auger, N. Ayoub, L. Bagby, B. Baller, R. Barger, G. Barr, M. Bass, F. Bay, K. Biery, M. Bishai, A. Blake, V. Bocean, D. Boehnlein, V. D. Bogert, T. Bolton, L. Bugel, C. Callahan, L. Camilleri, D. Caratelli, B. Carls, R. Castillo Fernandez, F. Cavanna, S. Chappa, H. Chen, K. Chen, C. Y. Chi, C. S. Chiu, E. Church, D. Cianci, G. H. Collin, J. M. Conrad, M. Convery, J. Cornele, P. Cowan, J. I. Crespo-Anadon, G. Crutcher, C. Darve, R. Davis, M. Del Tutto, D. Devitt, S. Duffin, S. Dytman, B. Eberly, A. Ereditato, D. Erickson, L. Escudero Sanchez, J. Esquivel, S. Farooq, J. Farrell, D. Featherston, B. T. Fleming, W. Foreman, A. P. Furmanski, V. Genty, M. Geynisman, D. Goeldi, B. Goff, S. Gollapinni, N. Graf, E. Gramellini, J. Green, A. Greene, H. Greenlee, T. Griffin, R. Grosso, R. Guenette, A. Hackenburg, R. Haenni, P. Hamilton, P. Healey, O. Hen, E. Henderson, J. Hewes, C. Hill, K. Hill, L. Himes, J. Ho, G. Horton-Smith, D. Huffman, C. M. Ignarra, C. James, E. James, J. Jan de Vries, W. Jaskierny, C. M. Jen, L. Jiang, B. Johnson, M. Johnson, R. A. Johnson, B. J. P. Jones, J. Joshi, H. Jostlein, D. Kaleko, L. N. Kalousis, G. Karagiorgi, T. Katori, P. Kellogg, W. Ketchum, J. Kilmer, B. King, B. Kirby, M. Kirby, E. Klein, T. Kobilarcik, I. Kreslo, R. Krull, R. Kubinski, G. Lange, F. Lanni, A. Lathrop, A. Laube, W. M. Lee, Y. Li, D. Lissauer, A. Lister, B. R. Littlejohn, S. Lockwitz, D. Lorca, W. C. Louis, G. Lukhanin, M. Luethi, B. Lundberg, X. Luo, G. Mahler, I. Majoros, D. Makowiecki, A. Marchionni, C. Mariani, D. Markley, J. Marshall, D. A. Martinez Caicedo, K. T. McDonald, D. McKee, A. McLean, J. Mead, V. Meddage, T. Miceli, G. B. Mills, W. Miner, J. Moon, M. Mooney, C. D. Moore, Z. Moss, J. Mousseau, R. Murrells, D. Naples, P. Nienaber, B. Norris, N. Norton, J. Nowak, M. OBoyle, T. Olszanowski, O. Palamara, V. Paolone, V. Papavassiliou, S. F. Pate, Z. Pavlovic, R. Pelkey, M. Phipps, S. Pordes, D. Porzio, G. Pulliam, X. Qian, J. L. Raaf, V. Radeka, A. Rafique, R. A Rameika, B. Rebel, R. Rechenmacher, S. Rescia, L. Rochester, C. Rudolf von Rohr, A. Ruga, B. Russell, R. Sanders, W. R. Sands III, M. Sarychev, D. W. Schmitz, A. Schukraft, R. Scott, W. Seligman, M. H. Shaevitz, M. Shoun, J. Sinclair, W. Sippach, T. Smidt, A. Smith, E. L. Snider, M. Soderberg, M. Solano-Gonzalez, S. Soldner-Rembold, S. R. Soleti, J. Sondericker, P. Spentzouris, J. Spitz, J. St. John, T. Strauss, K. Sutton, A. M. Szelc, K. Taheri, N. Tagg, K. Tatum, J. Teng, K. Terao, M. Thomson, C. Thorn, J. Tillman, M. Toups, Y. T. Tsai, S. Tufanli, T. Usher, M. Utes, R. G. Van de Water, C. Vendetta, S. Vergani, E. Voirin, J. Voirin, B. Viren, P. Watkins, M. Weber, T. Wester, J. Weston, D. A. Wickremasinghe, S. Wolbers, T. Wongjirad, K. Woodruff, K. C. Wu, T. Yang, B. Yu, G. P. Zeller, J. Zennamo, C. Zhang, M. Zuckerbrot

This paper describes the design and construction of the MicroBooNE liquid argon time projection chamber and associated systems. MicroBooNE is the first phase of the Short Baseline Neutrino program, located at Fermilab, and will utilize the capabilities of liquid argon detectors to examine a rich assortment of physics topics. In this document details of design specifications, assembly procedures, and acceptance tests are reported. Read More

2016Nov
Authors: MicroBooNE collaboration, R. Acciarri, C. Adams, R. An, J. Asaadi, M. Auger, L. Bagby, B. Baller, G. Barr, M. Bass, F. Bay, M. Bishai, A. Blake, T. Bolton, L. Bugel, L. Camilleri, D. Caratelli, B. Carls, R. Castillo Fernandez, F. Cavanna, H. Chen, E. Church, D. Cianci, G. H. Collin, J. M. Conrad, M. Convery, J. I. Crespo-Anadón, M. Del Tutto, D. Devitt, S. Dytman, B. Eberly, A. Ereditato, L. Escudero Sanchez, J. Esquivel, B. T. Fleming, W. Foreman, A. P. Furmanski, G. T. Garvey, V. Genty, D. Goeldi, S. Gollapinni, N. Graf, E. Gramellini, H. Greenlee, R. Grosso, R. Guenette, A. Hackenburg, P. Hamilton, O. Hen, J. Hewes, C. Hill, J. Ho, G. Horton-Smith, C. James, J. Jan de Vries, C. -M. Jen, L. Jiang, R. A. Johnson, B. J. P. Jones, J. Joshi, H. Jostlein, D. Kaleko, G. Karagiorgi, W. Ketchum, B. Kirby, M. Kirby, T. Kobilarcik, I. Kreslo, A. Laube, Y. Li, A. Lister, B. R. Littlejohn, S. Lockwitz, D. Lorca, W. C. Louis, M. Luethi, B. Lundberg, X. Luo, A. Marchionni, C. Mariani, J. Marshall, D. A. Martinez Caicedo, V. Meddage, T. Miceli, G. B. Mills, J. Moon, M. Mooney, C. D. Moore, J. Mousseau, R. Murrells, D. Naples, P. Nienaber, J. Nowak, O. Palamara, V. Paolone, V. Papavassiliou, S. F. Pate, Z. Pavlovic, D. Porzio, G. Pulliam, X. Qian, J. L. Raaf, A. Rafique, L. Rochester, C. Rudolf von Rohr, B. Russell, D. W. Schmitz, A. Schukraft, W. Seligman, M. H. Shaevitz, J. Sinclair, E. L. Snider, M. Soderberg, S. Söldner-Rembold, S. R. Soleti, P. Spentzouris, J. Spitz, J. St. John, T. Strauss, A. M. Szelc, N. Tagg, K. Terao, M. Thomson, M. Toups, Y. -T. Tsai, S. Tufanli, T. Usher, R. G. Van de Water, B. Viren, M. Weber, J. Weston, D. A. Wickremasinghe, S. Wolbers, T. Wongjirad, K. Woodruff, T. Yang, G. P. Zeller, J. Zennamo, C. Zhang

We present several studies of convolutional neural networks applied to data coming from the MicroBooNE detector, a liquid argon time projection chamber (LArTPC). The algorithms studied include the classification of single particle images, the localization of single particle and neutrino interactions in an image, and the detection of a simulated neutrino event overlaid with cosmic ray backgrounds taken from real detector data. These studies demonstrate the potential of convolutional neural networks for particle identification or event detection on simulated neutrino interactions. Read More

2016Aug
Authors: P. Adamson, I. Anghel, A. Aurisano, G. Barr, M. Bishai, A. Blake, G. J. Bock, D. Bogert, S. V. Cao, T. J. Carroll, C. M. Castromonte, R. Chen, S. Childress, J. A. B. Coelho, L. Corwin, D. Cronin-Hennessy, J. K. de Jong, S. De Rijck, A. V. Devan, N. E. Devenish, M. V. Diwan, C. O. Escobar, J. J. Evans, E. Falk, G. J. Feldman, W. Flanagan, M. V. Frohne, M. Gabrielyan, H. R. Gallagher, S. Germani, R. A. Gomes, M. C. Goodman, P. Gouffon, N. Graf, R. Gran, K. Grzelak, A. Habig, S. R. Hahn, J. Hartnell, R. Hatcher, A. Holin, J. Huang, J. Hylen, G. M. Irwin, Z. Isvan, C. James, D. Jensen, T. Kafka, S. M. S. Kasahara, G. Koizumi, M. Kordosky, A. Kreymer, K. Lang, J. Ling, P. J. Litchfield, P. Lucas, W. A. Mann, M. L. Marshak, N. Mayer, C. McGivern, M. M. Medeiros, R. Mehdiyev, J. R. Meier, M. D. Messier, W. H. Miller, S. R. Mishra, S. Moed Sher, C. D. Moore, L. Mualem, J. Musser, D. Naples, J. K. Nelson, H. B. Newman, R. J. Nichol, J. A. Nowak, J. O'Connor, M. Orchanian, R. B. Pahlka, J. Paley, R. B. Patterson, G. Pawloski, A. Perch, M. M. Pfützner, D. D. Phan, S. Phan-Budd, R. K. Plunkett, N. Poonthottathil, X. Qiu, A. Radovic, B. Rebel, C. Rosenfeld, H. A. Rubin, P. Sail, M. C. Sanchez, J. Schneps, A. Schreckenberger, P. Schreiner, R. Sharma, A. Sousa, N. Tagg, R. L. Talaga, J. Thomas, M. A. Thomson, X. Tian, A. Timmons, J. Todd, S. C. Tognini, R. Toner, D. Torretta, G. Tzanakos, J. Urheim, P. Vahle, B. Viren, A. Weber, R. C. Webb, C. White, L. Whitehead, L. H. Whitehead, S. G. Wojcicki, R. Zwaska

We report new constraints on the size of large extra dimensions from data collected by the MINOS experiment between 2005 and 2012. Our analysis employs a model in which sterile neutrinos arise as Kaluza-Klein states in large extra dimensions and thus modify the neutrino oscillation probabilities due to mixing between active and sterile neutrino states. Using Fermilab's NuMI beam exposure of $10. Read More

2016Aug
Authors: P. Adamson, I. Anghel, A. Aurisano, G. Barr, M. Bishai, A. Blake, G. J. Bock, D. Bogert, S. V. Cao, T. J. Carroll, C. M. Castromonte, R. Chen, D. Cherdack, S. Childress, J. A. B. Coelho, L. Corwin, D. Cronin-Hennessy, J. K. de Jong, S. De Rijck, A. V. Devan, N. E. Devenish, M. V. Diwan, C. O. Escobar, J. J. Evans, E. Falk, G. J. Feldman, W. Flanagan, M. V. Frohne, M. Gabrielyan, H. R. Gallagher, S. Germani, R. A. Gomes, M. C. Goodman, P. Gouffon, N. Graf, R. Gran, K. Grzelak, A. Habig, S. R. Hahn, J. Hartnell, R. Hatcher, A. Holin, J. Huang, J. Hylen, G. M. Irwin, Z. Isvan, C. James, D. Jensen, T. Kafka, S. M. S. Kasahara, G. Koizumi, M. Kordosky, A. Kreymer, K. Lang, J. Ling, P. J. Litchfield, P. Lucas, W. A. Mann, M. L. Marshak, N. Mayer, C. McGivern, M. M. Medeiros, R. Mehdiyev, J. R. Meier, M. D. Messier, W. H. Miller, S. R. Mishra, S. Moed Sher, C. D. Moore, L. Mualem, J. Musser, D. Naples, J. K. Nelson, H. B. Newman, R. J. Nichol, J. A. Nowak, J. O'Connor, W. P. Oliver, M. Orchanian, R. B. Pahlka, J. Paley, R. B. Patterson, G. Pawloski, A. Perch, M. M. Pfutzner, D. D. Phan, S. Phan-Budd, R. K. Plunkett, N. Poonthottathil, X. Qiu, A. Radovic, B. Rebel, C. Rosenfeld, H. A. Rubin, P. Sail, M. C. Sanchez, J. Schneps, A. Schreckenberger, P. Schreiner, R. Sharma, A. Sousa, N. Tagg, R. L. Talaga, J. Thomas, M. A. Thomson, X. Tian, A. Timmons, J. Todd, S. C. Tognini, R. Toner, D. Torretta, G. Tzanakos, J. Urheim, P. Vahle, B. Viren, A. Weber, R. C. Webb, C. White, L. Whitehead, L. H. Whitehead, S. G. Wojcicki, R. Zwaska

Forward single $\pi^0$ production by coherent neutral-current interactions, $\nu \mathcal{A} \to \nu \mathcal{A} \pi^0$, is investigated using a 2.8$\times 10^{20}$ protons-on-target exposure of the MINOS Near Detector. For single-shower topologies, the event distribution in production angle exhibits a clear excess above the estimated background at very forward angles for visible energy in the range~1-8 GeV. Read More

2016Jul
Authors: P. Adamson, I. Anghel, A. Aurisano, G. Barr, M. Bishai, A. Blake, G. J. Bock, D. Bogert, S. V. Cao, T. J. Carroll, C. M. Castromonte, R. Chen, S. Childress, J. A. B. Coelho, L. Corwin, D. Cronin-Hennessy, J. K. de Jong, S. De Rijck, A. V. Devan, N. E. Devenish, M. V. Diwan, C. O. Escobar, J. J. Evans, E. Falk, G. J. Feldman, W. Flanagan, M. V. Frohne, M. Gabrielyan, H. R. Gallagher, S. Germani, R. A. Gomes, M. C. Goodman, P. Gouffon, N. Graf, R. Gran, K. Grzelak, A. Habig, S. R. Hahn, J. Hartnell, R. Hatcher, A. Holin, J. Huang, J. Hylen, G. M. Irwin, Z. Isvan, C. James, D. Jensen, T. Kafka, S. M. S. Kasahara, G. Koizumi, M. Kordosky, A. Kreymer, K. Lang, J. Ling, P. J. Litchfield, P. Lucas, W. A. Mann, M. L. Marshak, N. Mayer, C. McGivern, M. M. Medeiros, R. Mehdiyev, J. R. Meier, M. D. Messier, W. H. Miller, S. R. Mishra, S. Moed Sher, C. D. Moore, L. Mualem, J. Musser, D. Naples, J. K. Nelson, H. B. Newman, R. J. Nichol, J. A. Nowak, J. O'Connor, M. Orchanian, R. B. Pahlka, J. Paley, R. B. Patterson, G. Pawloski, A. Perch, M. M. Pfutzner, D. D. Phan, S. Phan-Budd, R. K. Plunkett, N. Poonthottathil, X. Qiu, A. Radovic, B. Rebel, C. Rosenfeld, H. A. Rubin, P. Sail, M. C. Sanchez, J. Schneps, A. Schreckenberger, P. Schreiner, R. Sharma, A. Sousa, N. Tagg, R. L. Talaga, J. Thomas, M. A. Thomson, X. Tian, A. Timmons, J. Todd, S. C. Tognini, R. Toner, D. Torretta, G. Tzanakos, J. Urheim, P. Vahle, B. Viren, A. Weber, R. C. Webb, C. White, L. Whitehead, L. H. Whitehead, S. G. Wojcicki, R. Zwaska

We report results of a search for oscillations involving a light sterile neutrino over distances of 1.04 and $735\,\mathrm{km}$ in a $\nu_{\mu}$-dominated beam with a peak energy of $3\,\mathrm{GeV}$. The data, from an exposure of $10. Read More

2016Jul
Authors: Daya Bay, MINOS Collaborations, :, P. Adamson, F. P. An, I. Anghel, A. Aurisano, A. B. Balantekin, H. R. Band, G. Barr, M. Bishai, A. Blake, S. Blyth G. J. Bock, D. Bogert, D. Cao, G. F. Cao, J. Cao, S. V. Cao, T. J. Carroll, C. M. Castromonte, W. R. Cen, Y. L. Chan, J. F. Chang, L. C. Chang, Y. Chang, H. S. Chen, Q. Y. Chen, R. Chen, S. M. Chen, Y. Chen, Y. X. Chen, J. Cheng, J. -H. Cheng, Y. P. Chen, Z. K. Cheng, J. J. Cherwinka, S. Childress, M. C. Chu, A. Chukanov, J. A. B. Coelho, L. Corwin, D. Cronin-Hennessy, J. P. Cummings, J. de Arcos, S. De Rijck, Z. Y. Deng, A. V. Devan, N. E. Devenish, X. F. Ding, Y. Y. Ding, M. V. Diwan, M. Dolgareva, J. Dove, D. A. Dwyer, W. R. Edwards, C. O. Escobar, J. J. Evans, E. Falk, G. J. Feldman, W. Flanagan, M. V. Frohne, M. Gabrielyan, H. R. Gallagher, S. Germani, R. Gill, R. A. Gomes, M. Gonchar, G. H. Gong, H. Gong, M. C. Goodman, P. Gouffon, N. Graf, R. Gran, M. Grassi, K. Grzelak, W. Q. Gu, M. Y. Guan, L. Guo, R. P. Guo, X. H. Guo, Z. Guo, A. Habig, R. W. Hackenburg, S. R. Hahn, R. Han, S. Hans, J. Hartnell, R. Hatcher, M. He, K. M. Heeger, Y. K. Heng, A. Higuera, A. Holin, Y. K. Hor, Y. B. Hsiung, B. Z. Hu, T. Hu, W. Hu, E. C. Huang, H. X. Huang, J. Huang, X. T. Huang, P. Huber, W. Huo, G. Hussain, J. Hylen, G. M. Irwin, Z. Isvan, D. E. Jaffe, P. Jaffke, C. James, K. L. Jen, D. Jensen, S. Jetter, X. L. Ji, X. P. Ji, J. B. Jiao, R. A. Johnson, J. K. de Jong, J. Joshi, T. Kafka, L. Kang, S. M. S. Kasahara, S. H. Kettell, S. Kohn, G. Koizumi, M. Kordosky, M. Kramer, A. Kreymer, 1 K. K. Kwan, M. W. Kwok, T. Kwok, K. Lang, T. J. Langford, K. Lau, L. Lebanowski, J. Lee, J. H. C. Lee, R. T. Lei, R. Leitner, J. K. C. Leung, C. Li, D. J. Li, F. Li, G. S. Li, Q. J. Li, S. Li, S. C. Li, W. D. Li, X. N. Li, Y. F. Li, Z. B. Li, H. Liang, C. J. Lin, G. L. Lin, S. Lin, S. K. Lin, Y. -C. Lin, J. J. Ling J. M. Link, P. J. Litchfield, L. Littenberg, B. R. Littlejohn, D. W. Liu, J. C. Liu, J. L. Liu, C. W. Loh, C. Lu, H. Q. Lu, J. S. Lu, P. Lucas, K. B. Luk, Z. Lv, Q. M. Ma, X. B. Ma, X. Y. Ma, Y. Q. Ma, Y. Malyshkin, W. A. Mann, M. L. Marshak, D. A. Martinez Caicedo, N. Mayer, K. T. McDonald, C. McGivern, R. D. McKeown, M. M. Medeiros, R. Mehdiyev, J. R. Meier, M. D. Messier, W. H. Miller, S. R. Mishra, I. Mitchell, M. Mooney, C. D. Moore, L. Mualem, J. Musser, Y. Nakajima, D. Naples, J. Napolitano, D. Naumov, E. Naumova, J. K. Nelson, H. B. Newman, H. Y. Ngai, R. J. Nichol, Z. Ning, A. Nowak, J. O'Connor, J. P. Ochoa-Ricoux, A. Olshevskiy, M. Orchanian, R., R. B. Pahlka, J. Paley, H. -R. Pan, J. Park, R. B. Patterson, S. Patton, G. Pawloski, V. Pec, J. C. Peng, A. Perch, M. M. Pfutzner, D. D. Phan, S. Phan-Budd, L. Pinsky, R. K. Plunkett, N. Poonthottathil, C. S. J. Pun, F. Z. Qi, M. Qi, X. Qian, X. Qiu, A. Radovic, N. Raper, B. Rebel, J. Ren, C. Rosenfeld, R. Rosero, B. Roskovec, X. C. Ruan, H. A. Rubin, P. Sail, M. C. Sanchez, J. Schneps, A. Schreckenberger, P. Schreiner, R. Sharma, S. Moed Sher, A. Sousa, H. Steiner, G. X. Sun, J. L. Sun, N. Tagg, R. L. Talaga, W. Tang, D. Taychenachev, J. Thomas, M. A. Thomson, X. Tian A. Timmons, J. Todd, S. C. Tognini, R. Toner, D. Torretta, K. Treskov, K. V. Tsang, C. E. Tull, G. Tzanakos, J. Urheim, P. Vahle, N. Viaux, B. Viren, V. Vorobel, C. H. Wang, M. Wang, N. Y. Wang, R. G. Wang, W. Wang, X. Wang, Y. F. Wang, Z. Wang, Z. M. Wang, R. C. Webb, A. Weber, H. Y. Wei, L. J. Wen, K. Whisnant, C. White, L. Whitehead L. H. Whitehead, T. Wise, S. G. Wojcicki, H. L. H. Wong, S. C. F. Wong, E. Worcester, C. -H. Wu, Q. Wu, W. J. Wu, D. M. Xia, J. K. Xia, Z. Z. Xing, J. L. Xu, J. Y. Xu, Y. Xu, T. Xue, C. G. Yang, H. Yang, L. Yang, M. S. Yang, M. T. Yang, M. Ye., Z. Ye, M. Yeh, B. L. Young, Z. Y. Yu, S. Zeng, L. ZhanC. Zhang, H. H. Zhang, J. W. Zhang, Q. M. Zhang, X. T. Zhang, Y. M. Zhang, Y. X. Zhang, Z. J. Zhang, Z. P. Zhang, Z. Y. Zhang, J. Zhao, Q. W. Zhao, Y. B. Zhao, W. L. Zhong, L. Zhou, N. Zhou, H. L. Zhuang, J. H. Zou

Searches for a light sterile neutrino have been performed independently by the MINOS and the Daya Bay experiments using the muon (anti)neutrino and electron antineutrino disappearance channels, respectively. In this Letter, results from both experiments are combined with those from the Bugey-3 reactor neutrino experiment to constrain oscillations into light sterile neutrinos. The three experiments are sensitive to complementary regions of parameter space, enabling the combined analysis to probe regions allowed by the LSND and MiniBooNE experiments in a minimally extended four-neutrino flavor framework. Read More

2016May
Authors: P. Adamson, I. Anghel, A. Aurisano, G. Barr, M. Bishai, A. Blake, G. J. Bock, D. Bogert, S. V. Cao, T. J. Carroll, C. M. Castromonte, R. Chen, S. Childress, J. A. B. Coelho, L. Corwin, D. Cronin-Hennessy, J. K. de Jong, S. de Rijck, A. V. Devan, N. E. Devenish, M. V. Diwan, C. O. Escobar, J. J. Evans, E. Falk, G. J. Feldman, W. Flanagan, M. V. Frohne, M. Gabrielyan, H. R. Gallagher, S. Germani, R. A. Gomes, M. C. Goodman, P. Gouffon, N. Graf, R. Gran, K. Grzelak, A. Habig, S. R. Hahn, J. Hartnell, R. Hatcher, A. Holin, J. Huang, J. Hylen, G. M. Irwin, Z. Isvan, C. James, D. Jensen, T. Kafka, S. M. S. Kasahara, G. Koizumi, M. Kordosky, A. Kreymer, K. Lang, J. Ling, P. J. Litchfield, P. Lucas, W. A. Mann, M. L. Marshak, N. Mayer, C. McGivern, M. M. Medeiros, R. Mehdiyev, J. R. Meier, M. D. Messier, W. H. Miller, S. R. Mishra, S. Moed Sher, C. D. Moore, L. Mualem, J. Musser, D. Naples, J. K. Nelson, H. B. Newman, R. J. Nichol, J. A. Nowak, J. O'Connor, M. Orchanian, R. B. Pahlka, J. Paley, R. B. Patterson, G. Pawloski, A. Perch, M. M. Pfützner, D. D. Phan, S. Phan-Budd, R. K. Plunkett, N. Poonthottathil, X. Qiu, A. Radovic, B. Rebel, C. Rosenfeld, H. A. Rubin, P. Sail, M. C. Sanchez, J. Schneps, A. Schreckenberger, P. Schreiner, R. Sharma, A. Sousa, N. Tagg, R. L. Talaga, J. Thomas, M. A. Thomson, X. Tian, A. Timmons, J. Todd, S. C. Tognini, R. Toner, D. Torretta, G. Tzanakos, J. Urheim, P. Vahle, B. Viren, A. Weber, R. C. Webb, C. White, L. Whitehead, L. H. Whitehead, S. G. Wojcicki, R. Zwaska

We report new constraints on flavor-changing non-standard neutrino interactions from the MINOS long-baseline experiment using $\nu_{e}$ and $\bar{\nu}_{e}$ appearance candidate events from predominantly $\nu_{\mu}$ and $\bar{\nu}_{\mu}$ beams. We used a statistical selection algorithm to separate $\nu_{e}$ candidates from background events, enabling an analysis of the combined MINOS neutrino and antineutrino data. We observe no deviations from standard neutrino mixing, and thus place constraints on the non-standard interaction matter effect, $|\varepsilon_{e\tau}|$, and phase, $(\delta_{CP}+\delta_{e\tau})$, using a thirty-bin likelihood fit. Read More

2016May
Authors: P. Adamson, I. Anghel, A. Aurisano, G. Barr, M. Bishai, A. Blake, G. J. Bock, D. Bogert, S. V. Cao, T. J. Carroll, C. M. Castromonte, R. Chen, S. Childress, J. A. B. Coelho, L. Corwin, D. Cronin-Hennessy, J. K. de Jong, S. de Rijck, A. V. Devan, N. E. Devenish, M. V. Diwan, C. O. Escobar, J. J. Evans, E. Falk, G. J. Feldman, W. Flanagan, M. V. Frohne, M. Gabrielyan, H. R. Gallagher, S. Germani, R. A. Gomes, M. C. Goodman, P. Gouffon, N. Graf, R. Gran, K. Grzelak, A. Habig, S. R. Hahn, J. Hartnell, R. Hatcher, A. Holin, J. Huang, J. Hylen, G. M. Irwin, Z. Isvan, C. James, D. Jensen, T. Kafka, S. M. S. Kasahara, G. Koizumi, M. Kordosky, A. Kreymer, K. Lang, J. Ling, P. J. Litchfield, P. Lucas, W. A. Mann, M. L. Marshak, N. Mayer, C. McGivern, M. M. Medeiros, R. Mehdiyev, J. R. Meier, M. D. Messier, W. H. Miller, S. R. Mishra, S. Moed Sher, C. D. Moore, L. Mualem, J. Musser, D. Naples, J. K. Nelson, H. B. Newman, R. J. Nichol, J. A. Nowak, J. O'Connor, M. Orchanian, R. B. Pahlka, J. Paley, R. B. Patterson, G. Pawloski, A. Perch, M. M. Pfützner, D. D. Phan, S. Phan-Budd, R. K. Plunkett, N. Poonthottathil, X. Qiu, A. Radovic, B. Rebel, C. Rosenfeld, H. A. Rubin, P. Sail, M. C. Sanchez, J. Schneps, A. Schreckenberger, P. Schreiner, R. Sharma, A. Sousa, N. Tagg, R. L. Talaga, J. Thomas, M. A. Thomson, X. Tian, A. Timmons, J. Todd, S. C. Tognini, R. Toner, D. Torretta, G. Tzanakos, J. Urheim, P. Vahle, B. Viren, A. Weber, R. C. Webb, C. White, L. Whitehead, L. H. Whitehead, S. G. Wojcicki, R. Zwaska

Data from the MINOS experiment has been used to search for mixing between muon neutrinos and muon antineutrinos using a time-independent Lorentz-violating formalism derived from the Standard-Model Extension (SME). MINOS is uniquely capable of searching for muon neutrino-antineutrino mixing given its long baseline and ability to distinguish between neutrinos and antineutrinos on an event-by-event basis. Neutrino and antineutrino interactions were observed in the MINOS Near and Far Detectors from an exposure of 10. Read More

The MINERvA experiment observes an excess of events containing electromagnetic showers relative to the expectation from Monte Carlo simulations in neutral-current neutrino interactions with mean beam energy of 4.5 GeV on a hydrocarbon target. The excess is characterized and found to be consistent with neutral-current neutral pion production with a broad energy distribution peaking at 7 GeV and a total cross section of 0. Read More

2016Feb
Authors: Minos Collaboration, P. Adamson, I. Anghel, A. Aurisano, G. Barr, M. Bishai, A. Blake, G. J. Bock, D. Bogert, S. V. Cao, T. J. Carroll, C. M. Castromonte, R. Chen, S. Childress, J. A. B. Coelho, L. Corwin, D. Cronin-Hennessy, J. K. de Jong, S. De Rijck, A. V. Devan, N. E. Devenish, M. V. Diwan, C. O. Escobar, J. J. Evans, E. Falk, G. J. Feldman, W. Flanagan, M. V. Frohne, M. Gabrielyan, H. R. Gallagher, S. Germani, R. A. Gomes, M. C. Goodman, P. Gouffon, N. Graf, R. Gran, K. Grzelak, A. Habig, S. R. Hahn, J. Hartnell, R. Hatcher, A. Holin, J. Huang, J. Hylen, G. M. Irwin, Z. Isvan, C. James, D. Jensen, T. Kafka, S. M. S. Kasahara, G. Koizumi, M. Kordosky, A. Kreymer, K. Lang, J. Ling, P. J. Litchfield, P. Lucas, W. A. Mann, M. L. Marshak, N. Mayer, C. McGivern, M. M. Medeiros, R. Mehdiyev, J. R. Meier, M. D. Messier, W. H. Miller, S. R. Mishra, S. Moed Sher, C. D. Moore, L. Mualem, J. Musser, D. Naples, J. K. Nelson, H. B. Newman, R. J. Nichol, J. A. Nowak, J. O'Connor, M. Orchanian, R. B. Pahlka, J. Paley, R. B. Patterson, G. Pawloski, A. Perch, M. Pfützner, D. D. Phan, S. Phan-Budd, R. K. Plunkett, N. Poonthottathil, X. Qiu, A. Radovic, B. Rebel, C. Rosenfeld, H. A. Rubin, P. Sail, M. C. Sanchez, J. Schneps, A. Schreckenberger, P. Schreiner, R. Sharma, A. Sousa, N. Tagg, R. L. Talaga, J. Thomas, M. A. Thomson, X. Tian, A. Timmons, J. Todd, S. C. Tognini, R. Toner, D. Torretta, G. Tzanakos, J. Urheim, P. Vahle, B. Viren, A. Weber, R. C. Webb, C. White, L. Whitehead, L. H. Whitehead, S. G. Wojcicki, R. Zwaska

The charge ratio, $R_\mu = N_{\mu^+}/N_{\mu^-}$, for cosmogenic multiple-muon events observed at an under- ground depth of 2070 mwe has been measured using the magnetized MINOS Far Detector. The multiple-muon events, recorded nearly continuously from August 2003 until April 2012, comprise two independent data sets imaged with opposite magnetic field polarities, the comparison of which allows the systematic uncertainties of the measurement to be minimized. The multiple-muon charge ratio is determined to be $R_\mu = 1. Read More

The MINERvA collaboration reports a novel study of neutrino-nucleus charged-current deep inelastic scattering (DIS) using the same neutrino beam incident on targets of polystyrene, graphite, iron, and lead. Results are presented as ratios of C, Fe, and Pb to CH. The ratios of total DIS cross sections as a function of neutrino energy and flux-integrated differential cross sections as a function of the Bjorken scaling variable x are presented in the neutrino-energy range of 5 - 50 GeV. Read More

Muon-neutrino elastic scattering on electrons is an observable neutrino process whose cross section is precisely known. Consequently a measurement of this process in an accelerator-based $\nu_\mu$ beam can improve the knowledge of the absolute neutrino flux impinging upon the detector; typically this knowledge is limited to $\sim$ 10% due to uncertainties in hadron production and focusing. We have isolated a sample of 135 $\pm$ 17 neutrino-electron elastic scattering candidates in the segmented scintillator detector of MINERvA, after subtracting backgrounds and correcting for efficiency. Read More

Two different nuclear-medium effects are isolated using a low three-momentum transfer subsample of neutrino-carbon scattering data from the MINERvA neutrino experiment. The observed hadronic energy in charged-current $\nu_\mu$ interactions is combined with muon kinematics to permit separation of the quasielastic and $\Delta$(1232) resonance processes. First, we observe a small cross section at very low energy transfer that matches the expected screening effect of long-range nucleon correlations. Read More

The first direct measurement of electron-neutrino quasielastic and quasielastic-like scattering on hydrocarbon in the few-GeV region of incident neutrino energy has been carried out using the MINERvA detector in the NuMI beam at Fermilab. The flux-integrated differential cross sections in electron production angle, electron energy and $Q^{2}$ are presented. The ratio of the quasielastic, flux-integrated differential cross section in $Q^{2}$ for $\nu_{e}$ with that of similarly-selected $\nu_{\mu}$-induced events from the same exposure is used to probe assumptions that underpin conventional treatments of charged-current $\nu_{e}$ interactions used by long-baseline neutrino oscillation experiments. Read More

2015Aug
Authors: F. P. An, J. Z. Bai, A. B. Balantekin, H. R. Band, D. Beavis, W. Beriguete, M. Bishai, S. Blyth, R. L. Brown, I. Butorov, D. Cao, G. F. Cao, J. Cao, R. Carr, W. R. Cen, W. T. Chan, Y. L. Chan, J. F. Chang, L. C. Chang, Y. Chang, C. Chasman, H. Y. Chen, H. S. Chen, M. J. Chen, Q. Y. Chen, S. J. Chen, S. M. Chen, X. C. Chen, X. H. Chen, X. S. Chen, Y. X. Chen, Y. Chen, J. H. Cheng, J. Cheng, Y. P. Cheng, J. J. Cherwinka, S. Chidzik, K. Chow, M. C. Chu, J. P. Cummings, J. de Arcos, Z. Y. Deng, X. F. Ding, Y. Y. Ding, M. V. Diwan, L. Dong, J. Dove, E. Draeger, X. F. Du, D. A. Dwyer, W. R. Edwards, S. R. Ely, S. D. Fang, J. Y. Fu, Z. W. Fu, L. Q. Ge, V. Ghazikhanian, R. Gill, J. Goett, M. Gonchar, G. H. Gong, H. Gong, Y. A. Gornushkin, M. Grassi, L. S. Greenler, W. Q. Gu, M. Y. Guan, R. P. Guo, X. H. Guo, R. W. Hackenburg, R. L. Hahn, R. Han, S. Hans, M. He, Q. He, W. S. He, K. M. Heeger, Y. K. Heng, A. Higuera, P. Hinrichs, T. H. Ho, M. Hoff, Y. K. Hor, Y. B. Hsiung, B. Z. Hu, L. M. Hu, L. J. Hu, T. Hu, W. Hu, E. C. Huang, H. Z. Huang, H. X. Huang, P. W. Huang, X. Huang, X. T. Huang, P. Huber, G. Hussain, Z. Isvan, D. E. Jaffe, P. Jaffke, K. L. Jen, S. Jetter, X. P. Ji, X. L. Ji, H. J. Jiang, W. Q. Jiang, J. B. Jiao, R. A. Johnson, J. Joseph, L. Kang, S. H. Kettell, S. Kohn, M. Kramer, K. K. Kwan, M. W. Kwok, T. Kwok, C. Y. Lai, W. C. Lai, W. H. Lai, T. J. Langford, K. Lau, L. Lebanowski, J. Lee, M. K. P. Lee, R. T. Lei, R. Leitner, J. K. C. Leung, K. Y. Leung, C. A. Lewis, B. Li, C. Li, D. J. Li, F. Li, G. S. Li, J. Li, N. Y. Li, Q. J. Li, S. F. Li, S. C. Li, W. D. Li, X. B. Li, X. N. Li, X. Q. Li, Y. Li, Y. F. Li, Z. B. Li, H. Liang, J. Liang, C. J. Lin, G. L. Lin, P. Y. Lin, S. X. Lin, S. K. Lin, Y. C. Lin, J. J. Ling, J. M. Link, L. Littenberg, B. R. Littlejohn, B. J. Liu, C. Liu, D. W. Liu, H. Liu, J. L. Liu, J. C. Liu, S. Liu, S. S. Liu, X. Liu, Y. B. Liu, C. Lu, H. Q. Lu, J. S. Lu, A. Luk, K. B. Luk, T. Luo, X. L. Luo, L. H. Ma, Q. M. Ma, X. Y. Ma, X. B. Ma, Y. Q. Ma, B. Mayes, K. T. McDonald, M. C. McFarlane, R. D. McKeown, Y. Meng, I. Mitchell, D. Mohapatra, J. Monari Kebwaro, J. E. Morgan, Y. Nakajima, J. Napolitano, D. Naumov, E. Naumova, C. Newsom, H. Y. Ngai, W. K. Ngai, Y. B. Nie, Z. Ning, J. P. Ochoa-Ricoux, A. Olshevskiy, A. Pagac, H. -R. Pan, S. Patton, C. Pearson, V. Pec, J. C. Peng, L. E. Piilonen, L. Pinsky, C. S. J. Pun, F. Z. Qi, M. Qi, X. Qian, N. Raper, B. Ren, J. Ren, R. Rosero, B. Roskovec, X. C. Ruan, W. R. Sands III, B. Seilhan, B. B. Shao, K. Shih, W. Y. Song, H. Steiner, P. Stoler, M. Stuart, G. X. Sun, J. L. Sun, N. Tagg, Y. H. Tam, H. K. Tanaka, W. Tang, X. Tang, D. Taychenachev, H. Themann, Y. Torun, S. Trentalange, O. Tsai, K. V. Tsang, R. H. M. Tsang, C. E. Tull, Y. C. Tung, N. Viaux, B. Viren, S. Virostek, V. Vorobel, C. H. Wang, L. S. Wang, L. Y. Wang, L. Z. Wang, M. Wang, N. Y. Wang, R. G. Wang, T. Wang, W. Wang, W. W. Wang, X. T. Wang, X. Wang, Y. F. Wang, Z. Wang, Z. Wang, Z. M. Wang, D. M. Webber, H. Y. Wei, Y. D. Wei, L. J. Wen, D. L. Wenman, K. Whisnant, C. G. White, L. Whitehead, C. A. Whitten Jr., J. Wilhelmi, T. Wise, H. C. Wong, H. L. H. Wong, J. Wong, S. C. F. Wong, E. Worcester, F. F. Wu, Q. Wu, D. M. Xia, J. K. Xia, S. T. Xiang, Q. Xiao, Z. Z. Xing, G. Xu, J. Y. Xu, J. L. Xu, J. Xu, W. Xu, Y. Xu, T. Xue, J. Yan, C. G. Yang, L. Yang, M. S. Yang, M. T. Yang, M. Ye, M. Yeh, Y. S. Yeh, K. Yip, B. L. Young, G. Y. Yu, Z. Y. Yu, S. Zeng, L. Zhan, C. Zhang, F. H. Zhang, H. H. Zhang, J. W. Zhang, K. Zhang, Q. X. Zhang, Q. M. Zhang, S. H. Zhang, X. T. Zhang, Y. C. Zhang, Y. H. Zhang, Y. M. Zhang, Y. X. Zhang, Y. M. Zhang, Z. J. Zhang, Z. Y. Zhang, Z. P. Zhang, J. Zhao, Q. W. Zhao, Y. F. Zhao, Y. B. Zhao, L. Zheng, W. L. Zhong, L. Zhou, N. Zhou, Z. Y. Zhou, H. L. Zhuang, S. Zimmerman, J. H. Zou

The Daya Bay experiment was the first to report simultaneous measurements of reactor antineutrinos at multiple baselines leading to the discovery of $\bar{\nu}_e$ oscillations over km-baselines. Subsequent data has provided the world's most precise measurement of $\rm{sin}^22\theta_{13}$ and the effective mass splitting $\Delta m_{ee}^2$. The experiment is located in Daya Bay, China where the cluster of six nuclear reactors is among the world's most prolific sources of electron antineutrinos. Read More

2015Jul
Authors: P. Adamson, K. Anderson, M. Andrews, R. Andrews, I. Anghel, D. Augustine, A. Aurisano, S. Avvakumov, D. S. Ayres, B. Baller, B. Barish, G. Barr, W. L. Barrett, R. H. Bernstein, J. Biggs, M. Bishai, A. Blake, V. Bocean, G. J. Bock, D. J. Boehnlein, D. Bogert, K. Bourkland, S. V. Cao, C. M. Castromonte, S. Childress, B. C. Choudhary, J. A. B. Coelho, J. H. Cobb, L. Corwin, D. Crane, J. P. Cravens, D. Cronin-Hennessy, R. J. Ducar, J. K. de Jong, A. V. Devan, N. E. Devenish, M. V. Diwan, A. R. Erwin, C. O. Escobar, J. J. Evans, E. Falk, G. J. Feldman, T. H. Fields, R. Ford, M. V. Frohne, H. R. Gallagher, V. Garkusha, R. A. Gomes, M. C. Goodman, P. Gouffon, N. Graf, R. Gran, N. Grossman, K. Grzelak, A. Habig, S. R. Hahn, D. Harding, D. Harris, P. G. Harris, J. Hartnell, R. Hatcher, S. Hays, K. Heller, A. Holin, J. Huang, J. Hylen, A. Ibrahim, D. Indurthy, G. M. Irwin, Z. Isvan, D. E. Jaffe, C. James, D. Jensen, J. Johnstone, T. Kafka, S. M. S. Kasahara, G. Koizumi, S. Kopp, M. Kordosky, A. Kreymer, K. Lang, C. Laughton, G. Lefeuvre, J. Ling, P. J. Litchfield, L. Loiacono, P. Lucas, W. A. Mann, A. Marchionni, M. L. Marshak, N. Mayer, C. McGivern, M. M. Medeiros, R. Mehdiyev, J. R. Meier, M. D. Messier, D. G. Michael, R. H. Milburn, J. L. Miller, W. H. Miller, S. R. Mishra, S. Moed Sher, C. D. Moore, J. Morfin, L. Mualem, S. Mufson, S. Murgia, M. Murtagh, J. Musser, D. Naples, J. K. Nelson, H. B. Newman, R. J. Nichol, J. A. Nowak, J. O Connor, W. P. Oliver, M. Olsen, M. Orchanian, S. Osprey, R. B. Pahlka, J. Paley, A. Para, R. B. Patterson, T. Patzak, Z. Pavlovic, G. Pawloski, A. Perch, E. A. Peterson, D. A. Petyt, M. M. Pfutzner, S. Phan-Budd, R. K. Plunkett, N. Poonthottathil, P. Prieto, D. Pushka, X. Qiu, A. Radovic, R. A. Rameika, J. Ratchford, B. Rebel, R. Reilly, C. Rosenfeld, H. A. Rubin, K. Ruddick, M. C. Sanchez, N. Saoulidou, L. Sauer, J. Schneps, D. Schoo, A. Schreckenberger, P. Schreiner, P. Shanahan, R. Sharma, W. Smart, C. Smith, A. Sousa, A. Stefanik, N. Tagg, R. L. Talaga, G. Tassotto, J. Thomas, J. Thompson, M. A. Thomson, X. Tian, A. Timmons, D. Tinsley, S. C. Tognini, R. Toner, D. Torretta, I. Trostin, G. Tzanakos, J. Urheim, P. Vahle, K. Vaziri, E. Villegas, B. Viren, G. Vogel, R. C. Webber, A. Weber, R. C. Webb, A. Wehmann, C. White, L. Whitehead, L. H. Whitehead, S. G. Wojcicki, M. L. Wong-Squires, T. Yang, F. X. Yumiceva, V. Zarucheisky, R. Zwaska

This paper describes the hardware and operations of the Neutrinos at the Main Injector (NuMI) beam at Fermilab. It elaborates on the design considerations for the beam as a whole and for individual elements. The most important design details of individual components are described. Read More

2015Jul
Authors: P. Adamson, I. Anghel, N. Ashby, A. Aurisano, G. Barr, M. Bishai, A. Blake, G. J. Bock, D. Bogert, R. Bumgarner, S. V. Cao, C. M. Castromonte, S. Childress, J. A. B. Coelho, L. Corwin, D. Cronin-Hennessy, J. K. de Jong, A. V. Devan, N. E. Devenish, M. V. Diwan, C. O. Escobar, J. J. Evans, E. Falk, G. J. Feldman, B. Fonville, M. V. Frohne, H. R. Gallagher, R. A. Gomes, M. C. Goodman, P. Gouffon, N. Graf, R. Gran, K. Grzelak, A. Habig, S. R. Hahn, J. Hartnell, R. Hatcher, J. Hirschauer, A. Holin, J. Huang, J. Hylen, G. M. Irwin, Z. Isvan, C. James, S. R. Jefferts, D. Jensen, T. Kafka, S. M. S. Kasahara, G. Koizumi, M. Kordosky, A. Kreymer, K. Lang, J. Ling, P. J. Litchfield, P. Lucas, W. A. Mann, M. L. Marshak, D. Matsakis, N. Mayer, A. McKinley, C. McGivern, M. M. Medeiros, R. Mehdiyev, J. R. Meier, M. D. Messier, W. H. Miller, S. R. Mishra, S. Mitchell, S. Moed Sher, C. D. Moore, L. Mualem, J. Musser, D. Naples, J. K. Nelson, H. B. Newman, R. J. Nichol, J. A. Nowak, J. O'Connor, M. Orchanian, R. B. Pahlka, J. Paley, T. E. Parker, R. B. Patterson, G. Pawloski, A. Perch, S. Phan-Budd, R. K. Plunkett, N. Poonthottathil, E. Powers, X. Qiu, A. Radovic, B. Rebel, K. Ridl, S. Römisch, C. Rosenfeld, H. A. Rubin, M. C. Sanchez, J. Schneps, A. Schreckenberger, P. Schreiner, R. Sharma, A. Sousa, N. Tagg, R. L. Talaga, J. Thomas, M. A. Thomson, X. Tian, A. Timmons, S. C. Tognini, R. Toner, D. Torretta, J. Urheim, P. Vahle, B. Viren, A. Weber, R. C. Webb, C. White, L. Whitehead, L. H. Whitehead, S. G. Wojcicki, J. Wright, V. Zhang, R. Zwaska

We report a two-detector measurement of the propagation speed of neutrinos over a baseline of 734 km. The measurement was made with the NuMI beam at Fermilab between the near and far MINOS detectors. The fractional difference between the neutrino speed and the speed of light is determined to be $(v/c-1) = (1. Read More

2015Mar

We report the first observation of seasonal modulations in the rates of cosmic ray multiple-muon events at two underground sites, the MINOS Near Detector with an overburden of 225 mwe, and the MINOS Far Detector site at 2100 mwe. At the deeper site, multiple-muon events with muons separated by more than 8 m exhibit a seasonal rate that peaks during the summer, similar to that of single-muon events. In contrast and unexpectedly, the rate of multiple-muon events with muons separated by less than 5-8 m, and the rate of multiple-muon events in the smaller, shallower Near Detector, exhibit a seasonal rate modulation that peaks in the winter. Read More

Single neutral pion production via muon antineutrino charged-current interactions in plastic scintillator (CH) is studied using the \minerva detector exposed to the NuMI low-energy, wideband antineutrino beam at Fermilab. Measurement of this process constrains models of neutral pion production in nuclei, which is important because the neutral-current analog is a background for $\bar{\nu}_e$ appearance oscillation experiments. The differential cross sections for $\pi^0$ momentum and production angle, for events with a single observed $\pi^0$ and no charged pions, are presented and compared to model predictions. Read More

2015Mar
Authors: R. Acciarri1, C. Adams2, R. An3, C. Andreopoulos4, A. M. Ankowski5, M. Antonello6, J. Asaadi7, W. Badgett8, L. Bagby9, B. Baibussinov10, B. Baller11, G. Barr12, N. Barros13, M. Bass14, V. Bellini15, P. Benetti16, S. Bertolucci17, K. Biery18, H. Bilokon19, M. Bishai20, A. Bitadze21, A. Blake22, F. Boffelli23, T. Bolton24, M. Bonesini25, J. Bremer26, S. J. Brice27, C. Bromberg28, L. Bugel29, E. Calligarich30, L. Camilleri31, D. Caratelli32, B. Carls33, F. Cavanna34, S. Centro35, H. Chen36, C. Chi37, E. Church38, D. Cianci39, A. G. Cocco40, G. H. Collin41, J. M. Conrad42, M. Convery43, G. De Geronimo44, A. Dermenev45, R. Dharmapalan46, S. Dixon47, Z. Djurcic48, S. Dytmam49, B. Eberly50, A. Ereditato51, J. Esquivel52, J. Evans53, A. Falcone54, C. Farnese55, A. Fava56, A. Ferrari57, B. T. Fleming58, W. M. Foreman59, J. Freestone60, T. Gamble61, G. Garvey62, V. Genty63, M. Geynisman64, D. Gibin65, S. Gninenko66, D. Göldi67, S. Gollapinni68, N. Golubev69, M. Graham70, E. Gramellini71, H. Greenlee72, R. Grosso73, R. Guenette74, A. Guglielmi75, A. Hackenburg76, R. Hänni77, O. Hen78, J. Hewes79, J. Ho80, G. Horton-Smith81, J. Howell82, A. Ivashkin83, C. James84, C. M. Jen85, R. A. Johnson86, B. J. P. Jones87, J. Joshi88, H. Jostlein89, D. Kaleko90, L. N. Kalousis91, G. Karagiorgi92, W. Ketchum93, B. Kirby94, M. Kirby95, M. Kirsanov96, J. Kisiel97, J. Klein98, J. Klinger99, T. Kobilarcik100, U. Kose101, I. Kreslo102, V. A. Kudryavtsev103, Y. Li104, B. Littlejohn105, D. Lissauer106, P. Livesly107, S. Lockwitz108, W. C. Louis109, M. Lüthi110, B. Lundberg111, F. Mammoliti112, G. Mannocchi113, A. Marchionni114, C. Mariani115, J. Marshall116, K. Mavrokoridis117, N. McCauley118, N. McConkey119, K. McDonald120, V. Meddage121, A. Menegolli122, G. Meng123, I. Mercer124, T. Miao125, T. Miceli126, G. B. Mills127, D. Mladenov128, C. Montanari129, D. Montanari130, J. Moon131, M. Mooney132, C. Moore133, Z. Moss134, M. H. Moulai135, S. Mufson136, R. Murrells137, D. Naples138, M. Nessi139, M. Nicoletto140, P. Nienaber141, B. Norris142, F. Noto143, J. Nowak144, S. Pal145, O. Palamara146, V. Paolone147, V. Papavassiliou148, S. Pate149, J. Pater150, Z. Pavlovic151, J. Perkin152, P. Picchi153, F. Pietropaolo154, P. Płoński155, S. Pordes156, R. Potenza157, G. Pulliam158, X. Qian159, L. Qiuguang160, J. L. Raaf161, V. Radeka162, R. Rameika163, A. Rappoldi164, G. L. Raselli165, P. N. Ratoff166, B. Rebel167, M. Richardson168, L. Rochester169, M. Rossella170, C. Rubbia171, C. Rudolf von Rohr172, B. Russell173, P. Sala174, A. Scaramelli175, D. W. Schmitz176, A. Schukraft177, W. Seligman178, M. H. Shaevitz179, B. Sippach180, E. Snider181, J. Sobczyk182, M. Soderberg183, S. Söldner-Rembold184, M. Spanu185, J. Spitz186, N. Spooner187, D. Stefan188, J. St. John189, T. Strauss190, R. Sulej191, C. M. Sutera192, A. M. Szelc193, N. Tagg194, C. E. Taylor195, K. Terao196, M. Thiesse197, L. Thompson198, M. Thomson199, C. Thorn200, M. Torti201, F. Tortorici202, M. Toups203, C. Touramanis204, Y. Tsai205, T. Usher206, R. Van de Water207, F. Varanini208, S. Ventura209, C. Vignoli210, T. Wachala211, M. Weber212, D. Whittington213, P. Wilson214, S. Wolbers215, T. Wongjirad216, K. Woodruff217, M. Xu218, T. Yang219, B. Yu220, A. Zani221, G. P. Zeller222, J. Zennamo223, C. Zhang224
Affiliations: 1MicroBooNE Collaboration, 2LAr1-ND Collaboration, 3MicroBooNE Collaboration, 4LAr1-ND Collaboration, 5LAr1-ND Collaboration, 6ICARUS-WA104 Collaboration, 7LAr1-ND Collaboration, 8LAr1-ND Collaboration, 9LAr1-ND Collaboration, 10ICARUS-WA104 Collaboration, 11LAr1-ND Collaboration, 12MicroBooNE Collaboration, 13LAr1-ND Collaboration, 14LAr1-ND Collaboration, 15ICARUS-WA104 Collaboration, 16ICARUS-WA104 Collaboration, 17ICARUS-WA104 Collaboration, 18ICARUS-WA104 Collaboration, 19ICARUS-WA104 Collaboration, 20LAr1-ND Collaboration, 21LAr1-ND Collaboration, 22MicroBooNE Collaboration, 23ICARUS-WA104 Collaboration, 24MicroBooNE Collaboration, 25ICARUS-WA104 Collaboration, 26ICARUS-WA104 Collaboration, 27MicroBooNE Collaboration, 28MicroBooNE Collaboration, 29LAr1-ND Collaboration, 30ICARUS-WA104 Collaboration, 31LAr1-ND Collaboration, 32MicroBooNE Collaboration, 33MicroBooNE Collaboration, 34LAr1-ND Collaboration, 35ICARUS-WA104 Collaboration, 36LAr1-ND Collaboration, 37LAr1-ND Collaboration, 38LAr1-ND Collaboration, 39LAr1-ND Collaboration, 40ICARUS-WA104 Collaboration, 41LAr1-ND Collaboration, 42LAr1-ND Collaboration, 43MicroBooNE Collaboration, 44LAr1-ND Collaboration, 45ICARUS-WA104 Collaboration, 46LAr1-ND Collaboration, 47LAr1-ND Collaboration, 48LAr1-ND Collaboration, 49MicroBooNE Collaboration, 50MicroBooNE Collaboration, 51LAr1-ND Collaboration, 52LAr1-ND Collaboration, 53LAr1-ND Collaboration, 54ICARUS-WA104 Collaboration, 55ICARUS-WA104 Collaboration, 56ICARUS-WA104 Collaboration, 57ICARUS-WA104 Collaboration, 58LAr1-ND Collaboration, 59LAr1-ND Collaboration, 60LAr1-ND Collaboration, 61LAr1-ND Collaboration, 62LAr1-ND Collaboration, 63LAr1-ND Collaboration, 64ICARUS-WA104 Collaboration, 65ICARUS-WA104 Collaboration, 66ICARUS-WA104 Collaboration, 67LAr1-ND Collaboration, 68MicroBooNE Collaboration, 69ICARUS-WA104 Collaboration, 70MicroBooNE Collaboration, 71LAr1-ND Collaboration, 72LAr1-ND Collaboration, 73MicroBooNE Collaboration, 74LAr1-ND Collaboration, 75ICARUS-WA104 Collaboration, 76LAr1-ND Collaboration, 77LAr1-ND Collaboration, 78MicroBooNE Collaboration, 79MicroBooNE Collaboration, 80LAr1-ND Collaboration, 81MicroBooNE Collaboration, 82LAr1-ND Collaboration, 83ICARUS-WA104 Collaboration, 84LAr1-ND Collaboration, 85LAr1-ND Collaboration, 86MicroBooNE Collaboration, 87LAr1-ND Collaboration, 88MicroBooNE Collaboration, 89MicroBooNE Collaboration, 90MicroBooNE Collaboration, 91LAr1-ND Collaboration, 92LAr1-ND Collaboration, 93LAr1-ND Collaboration, 94MicroBooNE Collaboration, 95MicroBooNE Collaboration, 96ICARUS-WA104 Collaboration, 97ICARUS-WA104 Collaboration, 98LAr1-ND Collaboration, 99LAr1-ND Collaboration, 100MicroBooNE Collaboration, 101ICARUS-WA104 Collaboration, 102LAr1-ND Collaboration, 103LAr1-ND Collaboration, 104MicroBooNE Collaboration, 105MicroBooNE Collaboration, 106LAr1-ND Collaboration, 107LAr1-ND Collaboration, 108MicroBooNE Collaboration, 109LAr1-ND Collaboration, 110LAr1-ND Collaboration, 111MicroBooNE Collaboration, 112ICARUS-WA104 Collaboration, 113ICARUS-WA104 Collaboration, 114MicroBooNE Collaboration, 115LAr1-ND Collaboration, 116MicroBooNE Collaboration, 117LAr1-ND Collaboration, 118LAr1-ND Collaboration, 119LAr1-ND Collaboration, 120MicroBooNE Collaboration, 121MicroBooNE Collaboration, 122ICARUS-WA104 Collaboration, 123ICARUS-WA104 Collaboration, 124LAr1-ND Collaboration, 125LAr1-ND Collaboration, 126MicroBooNE Collaboration, 127LAr1-ND Collaboration, 128ICARUS-WA104 Collaboration, 129ICARUS-WA104 Collaboration, 130LAr1-ND Collaboration, 131LAr1-ND Collaboration, 132MicroBooNE Collaboration, 133LAr1-ND Collaboration, 134LAr1-ND Collaboration, 135MicroBooNE Collaboration, 136LAr1-ND Collaboration, 137MicroBooNE Collaboration, 138MicroBooNE Collaboration, 139ICARUS-WA104 Collaboration, 140ICARUS-WA104 Collaboration, 141MicroBooNE Collaboration, 142LAr1-ND Collaboration, 143ICARUS-WA104 Collaboration, 144LAr1-ND Collaboration, 145LAr1-ND Collaboration, 146LAr1-ND Collaboration, 147MicroBooNE Collaboration, 148MicroBooNE Collaboration, 149MicroBooNE Collaboration, 150LAr1-ND Collaboration, 151LAr1-ND Collaboration, 152LAr1-ND Collaboration, 153ICARUS-WA104 Collaboration, 154ICARUS-WA104 Collaboration, 155ICARUS-WA104 Collaboration, 156MicroBooNE Collaboration, 157MicroBooNE Collaboration, 158LAr1-ND Collaboration, 159LAr1-ND Collaboration, 160LAr1-ND Collaboration, 161MicroBooNE Collaboration, 162LAr1-ND Collaboration, 163LAr1-ND Collaboration, 164ICARUS-WA104 Collaboration, 165ICARUS-WA104 Collaboration, 166LAr1-ND Collaboration, 167MicroBooNE Collaboration, 168LAr1-ND Collaboration, 169MicroBooNE Collaboration, 170ICARUS-WA104 Collaboration, 171ICARUS-WA104 Collaboration, 172LAr1-ND Collaboration, 173LAr1-ND Collaboration, 174ICARUS-WA104 Collaboration, 175ICARUS-WA104 Collaboration, 176LAr1-ND Collaboration, 177MicroBooNE Collaboration, 178MicroBooNE Collaboration, 179LAr1-ND Collaboration, 180LAr1-ND Collaboration, 181ICARUS-WA104 Collaboration, 182ICARUS-WA104 Collaboration, 183LAr1-ND Collaboration, 184LAr1-ND Collaboration, 185ICARUS-WA104 Collaboration, 186LAr1-ND Collaboration, 187LAr1-ND Collaboration, 188ICARUS-WA104 Collaboration, 189MicroBooNE Collaboration, 190LAr1-ND Collaboration, 191ICARUS-WA104 Collaboration, 192ICARUS-WA104 Collaboration, 193LAr1-ND Collaboration, 194MicroBooNE Collaboration, 195LAr1-ND Collaboration, 196LAr1-ND Collaboration, 197LAr1-ND Collaboration, 198LAr1-ND Collaboration, 199LAr1-ND Collaboration, 200LAr1-ND Collaboration, 201ICARUS-WA104 Collaboration, 202ICARUS-WA104 Collaboration, 203LAr1-ND Collaboration, 204LAr1-ND Collaboration, 205MicroBooNE Collaboration, 206MicroBooNE Collaboration, 207LAr1-ND Collaboration, 208ICARUS-WA104 Collaboration, 209ICARUS-WA104 Collaboration, 210ICARUS-WA104 Collaboration, 211ICARUS-WA104 Collaboration, 212LAr1-ND Collaboration, 213LAr1-ND Collaboration, 214MicroBooNE Collaboration, 215MicroBooNE Collaboration, 216LAr1-ND Collaboration, 217MicroBooNE Collaboration, 218MicroBooNE Collaboration, 219MicroBooNE Collaboration, 220LAr1-ND Collaboration, 221ICARUS-WA104 Collaboration, 222LAr1-ND Collaboration, 223LAr1-ND Collaboration, 224MicroBooNE Collaboration

A Short-Baseline Neutrino (SBN) physics program of three LAr-TPC detectors located along the Booster Neutrino Beam (BNB) at Fermilab is presented. This new SBN Program will deliver a rich and compelling physics opportunity, including the ability to resolve a class of experimental anomalies in neutrino physics and to perform the most sensitive search to date for sterile neutrinos at the eV mass-scale through both appearance and disappearance oscillation channels. Using data sets of 6. Read More

The MINERvA collaboration operated a scaled-down replica of the solid scintillator tracking and sampling calorimeter regions of the MINERvA detector in a hadron test beam at the Fermilab Test Beam Facility. This article reports measurements with samples of protons, pions, and electrons from 0.35 to 2. Read More

2014Oct

Kinematic distributions from an inclusive sample of 1.41 x 10^6 charged-current nu_mu interactions on iron, obtained using the MINOS Near Detector exposed to a wide-band beam with peak flux at 3 GeV, are compared to a conventional treatment of neutrino scattering within a Fermi gas nucleus. Results are used to guide the selection of a subsample enriched in quasielastic nu_mu Fe interactions, containing an estimated 123,000 quasielastic events of incident energies 1 < E_nu < 8 GeV, with = 2. Read More

A study of charged-current muon neutrino scattering on hydrocarbon in which the final state includes a muon and a proton and no pions is presented. Although this signature has the topology of neutrino quasielastic scattering from neutrons, the event sample contains contributions from both quasielastic and inelastic processes where pions are absorbed in the nucleus. The analysis accepts events with muon production angles up to 70$^{\circ}$ and proton kinetic energies greater than 110 MeV. Read More

Neutrino-induced coherent charged pion production on nuclei, $\stackrel{(-)}{\nu}_\mu A\to\mu^\pm\pi^\mp A$ is a rare, inelastic interaction in which a small squared four-momentum $| t|$ is transferred to the recoil nucleus leaving it intact in the reaction. In the scintillator tracker of MINERvA, we remove events with evidence of particles from nuclear breakup and reconstruct $| t|$ from the final state pion and muon. We select low $| t|$ events to isolate a sample rich in coherent candidates. Read More

2014Jun

A sample of 1.53$\times$10$^{9}$ cosmic-ray-induced single muon events has been recorded at 225 meters-water-equivalent using the MINOS Near Detector. The underground muon rate is observed to be highly correlated with the effective atmospheric temperature. Read More

2014Jun
Affiliations: 1The MINERvA Collaboration, 2The MINERvA Collaboration, 3The MINERvA Collaboration, 4The MINERvA Collaboration, 5The MINERvA Collaboration, 6The MINERvA Collaboration, 7The MINERvA Collaboration, 8The MINERvA Collaboration, 9The MINERvA Collaboration, 10The MINERvA Collaboration, 11The MINERvA Collaboration, 12The MINERvA Collaboration, 13The MINERvA Collaboration, 14The MINERvA Collaboration, 15The MINERvA Collaboration, 16The MINERvA Collaboration, 17The MINERvA Collaboration, 18The MINERvA Collaboration, 19The MINERvA Collaboration, 20The MINERvA Collaboration, 21The MINERvA Collaboration, 22The MINERvA Collaboration, 23The MINERvA Collaboration, 24The MINERvA Collaboration, 25The MINERvA Collaboration, 26The MINERvA Collaboration, 27The MINERvA Collaboration, 28The MINERvA Collaboration, 29The MINERvA Collaboration, 30The MINERvA Collaboration, 31The MINERvA Collaboration, 32The MINERvA Collaboration, 33The MINERvA Collaboration, 34The MINERvA Collaboration, 35The MINERvA Collaboration, 36The MINERvA Collaboration, 37The MINERvA Collaboration, 38The MINERvA Collaboration, 39The MINERvA Collaboration, 40The MINERvA Collaboration, 41The MINERvA Collaboration, 42The MINERvA Collaboration, 43The MINERvA Collaboration, 44The MINERvA Collaboration, 45The MINERvA Collaboration, 46The MINERvA Collaboration, 47The MINERvA Collaboration, 48The MINERvA Collaboration, 49The MINERvA Collaboration, 50The MINERvA Collaboration, 51The MINERvA Collaboration, 52The MINERvA Collaboration, 53The MINERvA Collaboration, 54The MINERvA Collaboration, 55The MINERvA Collaboration, 56The MINERvA Collaboration, 57The MINERvA Collaboration, 58The MINERvA Collaboration, 59The MINERvA Collaboration, 60The MINERvA Collaboration, 61The MINERvA Collaboration, 62The MINERvA Collaboration, 63The MINERvA Collaboration, 64The MINERvA Collaboration, 65The MINERvA Collaboration, 66The MINERvA Collaboration, 67The MINERvA Collaboration, 68The MINERvA Collaboration, 69The MINERvA Collaboration, 70The MINERvA Collaboration, 71The MINERvA Collaboration, 72The MINERvA Collaboration, 73The MINERvA Collaboration, 74The MINERvA Collaboration, 75The MINERvA Collaboration, 76The MINERvA Collaboration, 77The MINERvA Collaboration, 78The MINERvA Collaboration, 79The MINERvA Collaboration, 80The MINERvA Collaboration, 81The MINERvA Collaboration

Charged pion production via charged current $\nu_{\mu}$ interactions on plastic (CH) is studied using the MINERvA detector exposed to the NuMI wideband neutrino beam at Fermilab. Events with hadronic invariant mass W $<$ 1.4 GeV are selected to isolate single pion production, which is expected to occur primarily through the $\Delta(1232)$ resonance. Read More

2014Mar
Affiliations: 1The MINERvA Collaboration, 2The MINERvA Collaboration, 3The MINERvA Collaboration, 4The MINERvA Collaboration, 5The MINERvA Collaboration, 6The MINERvA Collaboration, 7The MINERvA Collaboration, 8The MINERvA Collaboration, 9The MINERvA Collaboration, 10The MINERvA Collaboration, 11The MINERvA Collaboration, 12The MINERvA Collaboration, 13The MINERvA Collaboration, 14The MINERvA Collaboration, 15The MINERvA Collaboration, 16The MINERvA Collaboration, 17The MINERvA Collaboration, 18The MINERvA Collaboration, 19The MINERvA Collaboration, 20The MINERvA Collaboration, 21The MINERvA Collaboration, 22The MINERvA Collaboration, 23The MINERvA Collaboration, 24The MINERvA Collaboration, 25The MINERvA Collaboration, 26The MINERvA Collaboration, 27The MINERvA Collaboration, 28The MINERvA Collaboration, 29The MINERvA Collaboration, 30The MINERvA Collaboration, 31The MINERvA Collaboration, 32The MINERvA Collaboration, 33The MINERvA Collaboration, 34The MINERvA Collaboration, 35The MINERvA Collaboration, 36The MINERvA Collaboration, 37The MINERvA Collaboration, 38The MINERvA Collaboration, 39The MINERvA Collaboration, 40The MINERvA Collaboration, 41The MINERvA Collaboration, 42The MINERvA Collaboration, 43The MINERvA Collaboration, 44The MINERvA Collaboration, 45The MINERvA Collaboration, 46The MINERvA Collaboration, 47The MINERvA Collaboration, 48The MINERvA Collaboration, 49The MINERvA Collaboration, 50The MINERvA Collaboration, 51The MINERvA Collaboration, 52The MINERvA Collaboration, 53The MINERvA Collaboration, 54The MINERvA Collaboration, 55The MINERvA Collaboration, 56The MINERvA Collaboration, 57The MINERvA Collaboration, 58The MINERvA Collaboration, 59The MINERvA Collaboration, 60The MINERvA Collaboration, 61The MINERvA Collaboration, 62The MINERvA Collaboration, 63The MINERvA Collaboration, 64The MINERvA Collaboration, 65The MINERvA Collaboration, 66The MINERvA Collaboration, 67The MINERvA Collaboration, 68The MINERvA Collaboration, 69The MINERvA Collaboration, 70The MINERvA Collaboration, 71The MINERvA Collaboration, 72The MINERvA Collaboration, 73The MINERvA Collaboration, 74The MINERvA Collaboration, 75The MINERvA Collaboration, 76The MINERvA Collaboration, 77The MINERvA Collaboration

We present measurements of $\nu_{\mu}$ charged-current cross section ratios on carbon, iron, and lead relative to a scintillator (CH) using the fine-grained MINERvA detector exposed to the NuMI neutrino beam at Fermilab. The measurements utilize events of energies $2=8~GeV$, which have a reconstructed $\mu^{-}$ scattering angle less than $17^\circ$ to extract ratios of inclusive total cross sections as a function of neutrino energy $E_{\nu}$ and flux-integrated differential cross sections with respect to the Bjorken scaling variable $x$. These results provide the first high-statistics direct measurements of nuclear effects in neutrino scattering using different targets in the same neutrino beam. Read More

2014Mar

We report on a new analysis of neutrino oscillations in MINOS using the complete set of accelerator and atmospheric data. The analysis combines the $\nu_{\mu}$ disappearance and $\nu_{e}$ appearance data using the three-flavor formalism. We measure $|\Delta m^{2}_{32}|=[2. Read More

2013May

The MINERvA experiment is designed to perform precision studies of neutrino-nucleus scattering using $\nu_\mu$ and ${\bar\nu}_\mu$ neutrinos incident at 1-20 GeV in the NuMI beam at Fermilab. This article presents a detailed description of the \minerva detector and describes the {\em ex situ} and {\em in situ} techniques employed to characterize the detector and monitor its performance. The detector is comprised of a finely-segmented scintillator-based inner tracking region surrounded by electromagnetic and hadronic sampling calorimetry. Read More

2013May
Authors: The MINERvA collaboration, L. Fields, J. Chvojka, L. Aliaga, O. Altinok, B. Baldin, A. Baumbaugh, A. Bodek, D. Boehnlein, S. Boyd, R. Bradford, W. K. Brooks, H. Budd, A. Butkevich, D. A. Martinez Caicedo, C. M. Castromonte, M. E. Christy, H. Chung, M. Clark, H. da Motta, D. S. Damiani, I. Danko, M. Datta, M. Day, R. DeMaat, J. Devan, E. Draeger, S. A. Dytman, G. A. Díaz, B. Eberly, D. A. Edmondson, J. Felix, T. Fitzpatrick, G. A. Fiorentini, A. M. Gago, H. Gallagher, C. A. George, J. A. Gielata, C. Gingu, B. Gobbi, R. Gran, N. Grossman, J. Hanson, D. A. Harris, J. Heaton, A. Higuera, I. J. Howley, K. Hurtado, M. Jerkins, T. Kafka, J. Kaisen, M. O. Kanter, C. E. Keppel, J. Kilmer, M. Kordosky, A. H. Krajeski, S. A. Kulagin, T. Le, H. Lee, A. G. Leister, G. Locke, G. Maggi, E. Maher, S. Manly, W. A. Mann, C. M. Marshall, K. S. McFarland, C. L. McGivern, A. M. McGowan, A. Mislivec, J. G. Morfín, J. Mousseau, D. Naples, J. K. Nelson, G. Niculescu, I. Niculescu, N. Ochoa, C. D. O'Connor, J. Olsen, B. Osmanov, J. Osta, J. L. Palomino, V. Paolone, J. Park, C. E. Patrick, G. N. Perdue, C. Peña, L. Rakotondravohitra, R. D. Ransome, H. Ray, L. Ren, P. A. Rodrigues, C. Rude, K. E. Sassin, H. Schellman, D. W. Schmitz, R. M. Schneider, E. C. Schulte, C. Simon, F. D. Snider, M. C. Snyder, J. T. Sobczyk, C. J. Solano Salinas, N. Tagg, W. Tan, B. G. Tice, G. Tzanakos, J. P. Velásquez, J. Walding, T. Walton, J. Wolcott, B. A. Wolthuis, N. Woodward, G. Zavala, H. B. Zeng, D. Zhang, L. Y. Zhu, B. P. Ziemer

We have isolated muon anti-neutrino charged-current quasi-elastic interactions occurring in the segmented scintillator tracking region of the MINERvA detector running in the NuMI neutrino beam at Fermilab. We measure the flux-averaged differential cross-section, d{\sigma}/dQ^2, and compare to several theoretical models of quasi-elastic scattering. Good agreement is obtained with a model where the nucleon axial mass, M_A, is set to 0. Read More

2013May
Authors: The MINERvA collaboration, G. A. Fiorentini, D. W. Schmitz, P. A. Rodrigues, L. Aliaga, O. Altinok, B. Baldin, A. Baumbaugh, A. Bodek, D. Boehnlein, S. Boyd, R. Bradford, W. K. Brooks, H. Budd, A. Butkevich, D. A. Martinez Caicedo, C. M. Castromonte, M. E. Christy, H. Chung, J. Chvojka, M. Clark, H. da Motta, D. S. Damiani, I. Danko, M. Datta, M. Day, R. DeMaat, J. Devan, E. Draeger, S. A. Dytman, G. A. Díaz, B. Eberly, D. A. Edmondson, J. Felix, T. Fitzpatrick, L. Fields, A. M. Gago, H. Gallagher, C. A. George, J. A. Gielata, C. Gingu, B. Gobbi, R. Gran, N. Grossman, J. Hanson, D. A. Harris, J. Heaton, A. Higuera, I. J. Howley, K. Hurtado, M. Jerkins, T. Kafka, J. Kaisen, M. O. Kanter, C. E. Keppel, J. Kilmer, M. Kordosky, A. H. Krajeski, S. A. Kulagin, T. Le, H. Lee, A. G. Leister, G. Locke, G. Maggi, E. Maher, S. Manly, W. A. Mann, C. M. Marshall, K. S. McFarland, C. L. McGivern, A. M. McGowan, A. Mislivec, J. G. Morfń, J. Mousseau, D. Naples, J. K. Nelson, G. Niculescu, I. Niculescu, N. Ochoa, C. D. O'Connor, J. Olsen, B. Osmanov, J. Osta, J. L. Palomino, V. Paolone, J. Park, C. E. Patrick, G. N. Perdue, C. Peña, L. Rakotondravohitra, R. D. Ransome, H. Ray, L. Ren, C. Rude, K. E. Sassin, H. Schellman, R. M. Schneider, E. C. Schulte, C. Simon, F. D. Snider, M. C. Snyder, J. T. Sobczyk, C. J. Solano Salinas, N. Tagg, W. Tan, B. G. Tice, G. Tzanakos, J. P. Velásquez, J. Walding, T. Walton, J. Wolcott, B. A. Wolthuis, N. Woodward, G. Zavala, H. B. Zeng, D. Zhang, L. Y. Zhu, B. P. Ziemer

We report a study of muon neutrino charged-current quasi-elastic events in the segmented scintillator inner tracker of the MINERvA experiment running in the NuMI neutrino beam at Fermilab. The events were selected by requiring a {\mu}^- and low calorimetric recoil energy separated from the interaction vertex. We measure the flux-averaged differential cross-section, d{\sigma}/dQ^2, and study the low energy particle content of the final state. Read More

2013Apr

We report measurements of oscillation parameters from $\nu_{mu}$ and $\bar{\nu}_{\mu}$ disappearance using beam and atmospheric data from MINOS. The data comprise exposures of \unit[$10.71 \times 10^{20}$]{protons on target (POT)} in the $\nu_{\mu}$-dominated beam, $\unit[3. Read More

We report new constraints on flavor-changing non-standard neutrino interactions (NSI) using data from the MINOS experiment. We analyzed a combined set of beam neutrino and antineutrino data, and found no evidence for deviations from standard neutrino mixing. The observed energy spectra constrain the NSI parameter to the range $-0. Read More

2013Jan

We report on $\nu_e$ and $\bar{\nu}_e$ appearance in $\nu_\mu$ and $\bar{\nu}_\mu$ beams using the full MINOS data sample. The comparison of these $\nu_e$ and $\bar{\nu}_e$ appearance data at a 735 km baseline with $\theta_{13}$ measurements by reactor experiments probes $\delta$, the $\theta_{23}$ octant degeneracy, and the mass hierarchy. This analysis is the first use of this technique and includes the first accelerator long-baseline search for $\bar{\nu}_\mu\rightarrow\bar{\nu}_e$. Read More

2012Oct
Authors: Daya Bay Collaboration, F. P. An, Q. An, J. Z. Bai, A. B. Balantekin, H. R. Band, W. Beriguete, M. Bishai, S. Blyth, R. L. Brown, G. F. Cao, J. Cao, R. Carr, W. T. Chan, J. F. Chang, Y. Chang, C. Chasman, H. S. Chen, H. Y. Chen, S. J. Chen, S. M. Chen, X. C. Chen, X. H. Chen, X. S. Chen, Y. Chen, Y. X. Chen, J. J. Cherwinka, M. C. Chu, J. P. Cummings, Z. Y. Deng, Y. Y. Ding, M. V. Diwan, E. Draeger, X. F. Du, D. Dwyer, W. R. Edwards, S. R. Ely, S. D. Fang, J. Y. Fu, Z. W. Fu, L. Q. Ge, R. L. Gill, M. Gonchar, G. H. Gong, H. Gong, Y. A. Gornushkin, W. Q. Gu, M. Y. Guan, X. H. Guo, R. W. Hackenburg, R. L. Hahn, S. Hans, H. F. Hao, M. He, Q. He, K. M. Heeger, Y. K. Heng, P. Hinrichs, Y. K. Hor, Y. B. Hsiung, B. Z. Hu, T. Hu, H. X. Huang, H. Z. Huang, X. T. Huang, P. Huber, V. Issakov, Z. Isvan, D. E. Jaffe, S. Jetter, X. L. Ji, X. P. Ji, H. J. Jiang, J. B. Jiao, R. A. Johnson, L. Kang, S. H. Kettell, M. Kramer, K. K. Kwan, M. W. Kwok, T. Kwok, C. Y. Lai, W. C. Lai, W. H. Lai, K. Lau, L. Lebanowski, J. Lee, R. T. Lei, R. Leitner, J. K. C. Leung, K. Y. Leung, C. A. Lewis, F. Li, G. S. Li, Q. J. Li, W. D. Li, X. B. Li, X. N. Li, X. Q. Li, Y. Li, Z. B. Li, H. Liang, C. J. Lin, G. L. Lin, S. K. Lin, Y. C. Lin, J. J. Ling, J. M. Link, L. Littenberg, B. R. Littlejohn, D. W. Liu, J. C. Liu, J. L. Liu, Y. B. Liu, C. Lu, H. Q. Lu, A. Luk, K. B. Luk, Q. M. Ma, X. B. Ma, X. Y. Ma, Y. Q. Ma, K. T. McDonald, M. C. McFarlane, R. D. McKeown, Y. Meng, D. Mohapatra, Y. Nakajima, J. Napolitano, D. Naumov, I. Nemchenok, H. Y. Ngai, W. K. Ngai, Y. B. Nie, Z. Ning, J. P. Ochoa-Ricoux, A. Olshevski, S. Patton, V. Pec, J. C. Peng, L. E. Piilonen, L. Pinsky, C. S. J. Pun, F. Z. Qi, M. Qi, X. Qian, N. Raper, J. Ren, R. Rosero, B. Roskovec, X. C. Ruan, B. B. Shao, K. Shih, H. Steiner, G. X. Sun, J. L. Sun, N. Tagg, Y. H. Tam, H. K. Tanaka, X. Tang, H. Themann, Y. Torun, S. Trentalange, O. Tsai, K. V. Tsang, R. H. M. Tsang, C. E. Tull, Y. C. Tung, B. Viren, V. Vorobel, C. H. Wang, L. S. Wang, L. Y. Wang, L. Z. Wang, M. Wang, N. Y. Wang, R. G. Wang, W. Wang, X. Wang, Y. F. Wang, Z. Wang, Z. Wang, Z. M. Wang, D. M. Webber, H. Y. Wei, Y. D. Wei, L. J. Wen, K. Whisnant, C. G. White, L. Whitehead, Y. Williamson, T. Wise, H. L. H. Wong, E. T. Worcester, F. F. Wu, Q. Wu, J. B. Xi, D. M. Xia, Z. Z. Xing, J. Xu, J. Xu, J. L. Xu, Y. Xu, T. Xue, C. G. Yang, L. Yang, M. Ye, M. Yeh, Y. S. Yeh, B. L. Young, Z. Y. Yu, L. Zhan, C. Zhang, F. H. Zhang, J. W. Zhang, Q. M. Zhang, S. H. Zhang, Y. C. Zhang, Y. H. Zhang, Y. X. Zhang, Z. J. Zhang, Z. P. Zhang, Z. Y. Zhang, J. Zhao, Q. W. Zhao, Y. B. Zhao, L. Zheng, W. L. Zhong, L. Zhou, Z. Y. Zhou, H. L. Zhuang, J. H. Zou

We report an improved measurement of the neutrino mixing angle $\theta_{13}$ from the Daya Bay Reactor Neutrino Experiment. We exclude a zero value for $\sin^22\theta_{13}$ with a significance of 7.7 standard deviations. Read More

2012Aug

This paper reports measurements of atmospheric neutrino and antineutrino interactions in the MINOS Far Detector, based on 2553 live-days (37.9 kton-years) of data. A total of 2072 candidate events are observed. Read More

2012Mar

Beams of neutrinos have been proposed as a vehicle for communications under unusual circumstances, such as direct point-to-point global communication, communication with submarines, secure communications and interstellar communication. We report on the performance of a low-rate communications link established using the NuMI beam line and the MINERvA detector at Fermilab. The link achieved a decoded data rate of 0. Read More

2012Feb

We report an improved measurement of muon anti-neutrino disappearance over a distance of 735km using the MINOS detectors and the Fermilab Main Injector neutrino beam in a muon anti-neutrino enhanced configuration. From a total exposure of 2.95e20 protons on target, of which 42% have not been previously analyzed, we make the most precise measurement of the anti-neutrino "atmospheric" delta-m squared = 2. Read More

2012Jan
Authors: P. Adamson1, D. S. Ayres2, G. Barr3, M. Bishai4, A. Blake5, G. J. Bock6, D. J. Boehnlein7, D. Bogert8, S. V. Cao9, S. Cavanaugh10, S. Childress11, J. A. B. Coelho12, L. Corwin13, D. Cronin-Hennessy14, I. Z. Danko15, J. K. de Jong16, N. E. Devenish17, M. V. Diwan18, C. O. Escobar19, J. J. Evans20, E. Falk21, G. J. Feldman22, M. V. Frohne23, H. R. Gallagher24, R. A. Gomes25, M. C. Goodman26, P. Gouffon27, N. Graf28, R. Gran29, K. Grzelak30, A. Habig31, J. Hartnell32, R. Hatcher33, A. Himmel34, A. Holin35, J. Hylen36, G. M. Irwin37, Z. Isvan38, C. James39, D. Jensen40, T. Kafka41, S. M. S. Kasahara42, G. Koizumi43, S. Kopp44, M. Kordosky45, A. Kreymer46, K. Lang47, J. Ling48, P. J. Litchfield49, L. Loiacono50, P. Lucas51, W. A. Mann52, M. L. Marshak53, M. Mathis54, N. Mayer55, R. Mehdiyev56, J. R. Meier57, M. D. Messier58, W. H. Miller59, S. R. Mishra60, J. Mitchell61, C. D. Moore62, L. Mualem63, S. Mufson64, J. Musser65, D. Naples66, J. K. Nelson67, H. B. Newman68, R. J. Nichol69, J. A. Nowak70, W. P. Oliver71, M. Orchanian72, R. B. Pahlka73, J. Paley74, R. B. Patterson75, G. Pawloski76, S. Phan-Budd77, R. K. Plunkett78, X. Qiu79, A. Radovic80, J. Ratchford81, B. Rebel82, C. Rosenfeld83, H. A. Rubin84, M. C. Sanchez85, J. Schneps86, A. Schreckenberger87, P. Schreiner88, R. Sharma89, A. Sousa90, M. Strait91, N. Tagg92, R. L. Talaga93, J. Thomas94, M. A. Thomson95, G. Tinti96, R. Toner97, D. Torretta98, G. Tzanakos99, J. Urheim100, P. Vahle101, B. Viren102, J. J. Walding103, A. Weber104, R. C. Webb105, C. White106, L. Whitehead107, S. G. Wojcicki108, R. Zwaska109
Affiliations: 1The MINOS Collaboration, 2The MINOS Collaboration, 3The MINOS Collaboration, 4The MINOS Collaboration, 5The MINOS Collaboration, 6The MINOS Collaboration, 7The MINOS Collaboration, 8The MINOS Collaboration, 9The MINOS Collaboration, 10The MINOS Collaboration, 11The MINOS Collaboration, 12The MINOS Collaboration, 13The MINOS Collaboration, 14The MINOS Collaboration, 15The MINOS Collaboration, 16The MINOS Collaboration, 17The MINOS Collaboration, 18The MINOS Collaboration, 19The MINOS Collaboration, 20The MINOS Collaboration, 21The MINOS Collaboration, 22The MINOS Collaboration, 23The MINOS Collaboration, 24The MINOS Collaboration, 25The MINOS Collaboration, 26The MINOS Collaboration, 27The MINOS Collaboration, 28The MINOS Collaboration, 29The MINOS Collaboration, 30The MINOS Collaboration, 31The MINOS Collaboration, 32The MINOS Collaboration, 33The MINOS Collaboration, 34The MINOS Collaboration, 35The MINOS Collaboration, 36The MINOS Collaboration, 37The MINOS Collaboration, 38The MINOS Collaboration, 39The MINOS Collaboration, 40The MINOS Collaboration, 41The MINOS Collaboration, 42The MINOS Collaboration, 43The MINOS Collaboration, 44The MINOS Collaboration, 45The MINOS Collaboration, 46The MINOS Collaboration, 47The MINOS Collaboration, 48The MINOS Collaboration, 49The MINOS Collaboration, 50The MINOS Collaboration, 51The MINOS Collaboration, 52The MINOS Collaboration, 53The MINOS Collaboration, 54The MINOS Collaboration, 55The MINOS Collaboration, 56The MINOS Collaboration, 57The MINOS Collaboration, 58The MINOS Collaboration, 59The MINOS Collaboration, 60The MINOS Collaboration, 61The MINOS Collaboration, 62The MINOS Collaboration, 63The MINOS Collaboration, 64The MINOS Collaboration, 65The MINOS Collaboration, 66The MINOS Collaboration, 67The MINOS Collaboration, 68The MINOS Collaboration, 69The MINOS Collaboration, 70The MINOS Collaboration, 71The MINOS Collaboration, 72The MINOS Collaboration, 73The MINOS Collaboration, 74The MINOS Collaboration, 75The MINOS Collaboration, 76The MINOS Collaboration, 77The MINOS Collaboration, 78The MINOS Collaboration, 79The MINOS Collaboration, 80The MINOS Collaboration, 81The MINOS Collaboration, 82The MINOS Collaboration, 83The MINOS Collaboration, 84The MINOS Collaboration, 85The MINOS Collaboration, 86The MINOS Collaboration, 87The MINOS Collaboration, 88The MINOS Collaboration, 89The MINOS Collaboration, 90The MINOS Collaboration, 91The MINOS Collaboration, 92The MINOS Collaboration, 93The MINOS Collaboration, 94The MINOS Collaboration, 95The MINOS Collaboration, 96The MINOS Collaboration, 97The MINOS Collaboration, 98The MINOS Collaboration, 99The MINOS Collaboration, 100The MINOS Collaboration, 101The MINOS Collaboration, 102The MINOS Collaboration, 103The MINOS Collaboration, 104The MINOS Collaboration, 105The MINOS Collaboration, 106The MINOS Collaboration, 107The MINOS Collaboration, 108The MINOS Collaboration, 109The MINOS Collaboration

We have searched for sidereal variations in the rate of antineutrino interactions in the MINOS Near Detector. Using antineutrinos produced by the NuMI beam, we find no statistically significant sidereal modulation in the rate. When this result is placed in the context of the Standard Model Extension theory we are able to place upper limits on the coefficients defining the theory. Read More