Constraining the NuMI neutrino flux using inverse muon decay reactions in MINERvA
Abstract
Inverse muon decay, vμe¯ → μ¯ve, is a reaction whose cross section can be predicted with very small uncertainties. It has a neutrino energy threshold of ≈ 11 GeV and can be used to constrain the high-energy part of the flux in the NuMI neutrino beam. This reaction is the dominant source of events which only contain high-energy muons nearly parallel to the direction of the neutrino beam. We have isolated a sample of hundreds of such events in neutrino and antineutrino enhanced beams, and have constrained the predicted high-energy flux.
- Authors:
- more »
- Publication Date:
- Research Org.:
- Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States); Univ. of Rochester, NY (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), High Energy Physics (HEP); National Science Foundation (NSF); NCN Opus
- Contributing Org.:
- MINERvA Collaboration; MINERVA Collaboration
- OSTI Identifier:
- 1832248
- Alternate Identifier(s):
- OSTI ID: 1824316; OSTI ID: 1838652
- Report Number(s):
- FERMILAB-PUB-21-312-E-SCD; arXiv:2107.01059
Journal ID: ISSN 2470-0010; PRVDAQ; 092010
- Grant/Contract Number:
- AC02-07CH11359; PHY-0619727; 3170845; 11130133; 216/21/B/ST2/01092; 27467; CHE2039044; SC0008475
- Resource Type:
- Published Article
- Journal Name:
- Physical Review D
- Additional Journal Information:
- Journal Name: Physical Review D Journal Volume: 104 Journal Issue: 9; Journal ID: ISSN 2470-0010
- Publisher:
- American Physical Society
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; lepton-lepton interactions; secondary beams; neutrino detectors; particle production
Citation Formats
Ruterbories, D., Ahmad Dar, Z., Akbar, F., Ascencio, M. V., Bashyal, A., Bercellie, A., Betancourt, M., Bodek, A., Bonilla, J. L., Bravar, A., Budd, H., Caceres, G., Cai, T., Carneiro, M. F., Díaz, G. A., da Motta, H., Felix, J., Fields, L., Filkins, A., Fine, R., Gago, A. M., Gallagher, H., Ghosh, A., Gran, R., Harris, D. A., Henry, S., Jena, D., Jena, S., Kleykamp, J., Kordosky, M., Last, D., Le, T., Lozano, A., Lu, X. -G., Maher, E., Manly, S., Mann, W. A., Mauger, C., McFarland, K. S., McGowan, A. M., Messerly, B., Miller, J., Morfín, J. G., Naples, D., Nelson, J. K., Nguyen, C., Norrick, A., Olivier, A., Paolone, V., Perdue, G. N., Plows, K. -J., Ramírez, M. A., Ray, H., Schellman, H., Solano Salinas, C. J., Su, H., Sultana, M., Syrotenko, V. S., Valencia, E., Vaughan, N. H., Waldron, A. V., Yaeggy, B., Yang, K., Zazueta, L., and The Collaboration. Constraining the NuMI neutrino flux using inverse muon decay reactions in MINERvA. United States: N. p., 2021.
Web. doi:10.1103/PhysRevD.104.092010.
Ruterbories, D., Ahmad Dar, Z., Akbar, F., Ascencio, M. V., Bashyal, A., Bercellie, A., Betancourt, M., Bodek, A., Bonilla, J. L., Bravar, A., Budd, H., Caceres, G., Cai, T., Carneiro, M. F., Díaz, G. A., da Motta, H., Felix, J., Fields, L., Filkins, A., Fine, R., Gago, A. M., Gallagher, H., Ghosh, A., Gran, R., Harris, D. A., Henry, S., Jena, D., Jena, S., Kleykamp, J., Kordosky, M., Last, D., Le, T., Lozano, A., Lu, X. -G., Maher, E., Manly, S., Mann, W. A., Mauger, C., McFarland, K. S., McGowan, A. M., Messerly, B., Miller, J., Morfín, J. G., Naples, D., Nelson, J. K., Nguyen, C., Norrick, A., Olivier, A., Paolone, V., Perdue, G. N., Plows, K. -J., Ramírez, M. A., Ray, H., Schellman, H., Solano Salinas, C. J., Su, H., Sultana, M., Syrotenko, V. S., Valencia, E., Vaughan, N. H., Waldron, A. V., Yaeggy, B., Yang, K., Zazueta, L., & The Collaboration. Constraining the NuMI neutrino flux using inverse muon decay reactions in MINERvA. United States. https://doi.org/10.1103/PhysRevD.104.092010
Ruterbories, D., Ahmad Dar, Z., Akbar, F., Ascencio, M. V., Bashyal, A., Bercellie, A., Betancourt, M., Bodek, A., Bonilla, J. L., Bravar, A., Budd, H., Caceres, G., Cai, T., Carneiro, M. F., Díaz, G. A., da Motta, H., Felix, J., Fields, L., Filkins, A., Fine, R., Gago, A. M., Gallagher, H., Ghosh, A., Gran, R., Harris, D. A., Henry, S., Jena, D., Jena, S., Kleykamp, J., Kordosky, M., Last, D., Le, T., Lozano, A., Lu, X. -G., Maher, E., Manly, S., Mann, W. A., Mauger, C., McFarland, K. S., McGowan, A. M., Messerly, B., Miller, J., Morfín, J. G., Naples, D., Nelson, J. K., Nguyen, C., Norrick, A., Olivier, A., Paolone, V., Perdue, G. N., Plows, K. -J., Ramírez, M. A., Ray, H., Schellman, H., Solano Salinas, C. J., Su, H., Sultana, M., Syrotenko, V. S., Valencia, E., Vaughan, N. H., Waldron, A. V., Yaeggy, B., Yang, K., Zazueta, L., and The Collaboration. Tue .
"Constraining the NuMI neutrino flux using inverse muon decay reactions in MINERvA". United States. https://doi.org/10.1103/PhysRevD.104.092010.
@article{osti_1832248,
title = {Constraining the NuMI neutrino flux using inverse muon decay reactions in MINERvA},
author = {Ruterbories, D. and Ahmad Dar, Z. and Akbar, F. and Ascencio, M. V. and Bashyal, A. and Bercellie, A. and Betancourt, M. and Bodek, A. and Bonilla, J. L. and Bravar, A. and Budd, H. and Caceres, G. and Cai, T. and Carneiro, M. F. and Díaz, G. A. and da Motta, H. and Felix, J. and Fields, L. and Filkins, A. and Fine, R. and Gago, A. M. and Gallagher, H. and Ghosh, A. and Gran, R. and Harris, D. A. and Henry, S. and Jena, D. and Jena, S. and Kleykamp, J. and Kordosky, M. and Last, D. and Le, T. and Lozano, A. and Lu, X. -G. and Maher, E. and Manly, S. and Mann, W. A. and Mauger, C. and McFarland, K. S. and McGowan, A. M. and Messerly, B. and Miller, J. and Morfín, J. G. and Naples, D. and Nelson, J. K. and Nguyen, C. and Norrick, A. and Olivier, A. and Paolone, V. and Perdue, G. N. and Plows, K. -J. and Ramírez, M. A. and Ray, H. and Schellman, H. and Solano Salinas, C. J. and Su, H. and Sultana, M. and Syrotenko, V. S. and Valencia, E. and Vaughan, N. H. and Waldron, A. V. and Yaeggy, B. and Yang, K. and Zazueta, L. and The Collaboration},
abstractNote = {Inverse muon decay, vμe¯ → μ¯ve, is a reaction whose cross section can be predicted with very small uncertainties. It has a neutrino energy threshold of ≈ 11 GeV and can be used to constrain the high-energy part of the flux in the NuMI neutrino beam. This reaction is the dominant source of events which only contain high-energy muons nearly parallel to the direction of the neutrino beam. We have isolated a sample of hundreds of such events in neutrino and antineutrino enhanced beams, and have constrained the predicted high-energy flux.},
doi = {10.1103/PhysRevD.104.092010},
journal = {Physical Review D},
number = 9,
volume = 104,
place = {United States},
year = {2021},
month = {11}
}
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