Measurement of neutrino-induced neutral-current coherent π0 production in the NOvA near detector
The cross section of neutrino-induced neutral-current coherent π0 production on a carbon-dominated target is measured in the NOvA near detector. This measurement uses a narrow-band neutrino beam with an average neutrino energy of 2.7 GeV, which is of interest to ongoing and future long-baseline neut...
- Autores:
-
Acero, M. A.
- Tipo de recurso:
- Fecha de publicación:
- 2019
- Institución:
- Universidad del Atlántico
- Repositorio:
- Repositorio Uniatlantico
- Idioma:
- eng
- OAI Identifier:
- oai:repositorio.uniatlantico.edu.co:20.500.12834/935
- Acceso en línea:
- https://hdl.handle.net/20.500.12834/935
- Palabra clave:
- Rights
- openAccess
- License
- http://creativecommons.org/licenses/by-nc/4.0/
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Measurement of neutrino-induced neutral-current coherent π0 production in the NOvA near detector |
| title |
Measurement of neutrino-induced neutral-current coherent π0 production in the NOvA near detector |
| spellingShingle |
Measurement of neutrino-induced neutral-current coherent π0 production in the NOvA near detector |
| title_short |
Measurement of neutrino-induced neutral-current coherent π0 production in the NOvA near detector |
| title_full |
Measurement of neutrino-induced neutral-current coherent π0 production in the NOvA near detector |
| title_fullStr |
Measurement of neutrino-induced neutral-current coherent π0 production in the NOvA near detector |
| title_full_unstemmed |
Measurement of neutrino-induced neutral-current coherent π0 production in the NOvA near detector |
| title_sort |
Measurement of neutrino-induced neutral-current coherent π0 production in the NOvA near detector |
| dc.creator.fl_str_mv |
Acero, M. A. |
| dc.contributor.author.none.fl_str_mv |
Acero, M. A. |
| description |
The cross section of neutrino-induced neutral-current coherent π0 production on a carbon-dominated target is measured in the NOvA near detector. This measurement uses a narrow-band neutrino beam with an average neutrino energy of 2.7 GeV, which is of interest to ongoing and future long-baseline neutrino oscillation experiments. The measured, flux-averaged cross section is σ ¼ 13.8 0.9ðstatÞ 2.3ðsystÞ × 10−40 cm2=nucleus, consistent with model prediction. This result is the most precise measurement of neutral-current coherent π0 production in the few-GeV neutrino energy region. |
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2019 |
| dc.date.submitted.none.fl_str_mv |
2019-02-05 |
| dc.date.issued.none.fl_str_mv |
2020-07-09 |
| dc.date.accessioned.none.fl_str_mv |
2022-11-15T21:03:59Z |
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2022-11-15T21:03:59Z |
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http://purl.org/coar/version/c_970fb48d4fbd8a85 |
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http://purl.org/coar/resource_type/c_2df8fbb1 |
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Artículo |
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https://hdl.handle.net/20.500.12834/935 |
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: 10.1103/PhysRevD.102.012004 |
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Universidad del Atlántico |
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Repositorio Universidad del Atlántico |
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https://hdl.handle.net/20.500.12834/935 |
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: 10.1103/PhysRevD.102.012004 Universidad del Atlántico Repositorio Universidad del Atlántico |
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eng |
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eng |
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Attribution-NonCommercial 4.0 International |
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Sede Norte |
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Physical Review |
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Acero, M. A.979f9c6a-faae-415d-b017-8ea1e9afa74c2022-11-15T21:03:59Z2022-11-15T21:03:59Z2020-07-092019-02-05https://hdl.handle.net/20.500.12834/935: 10.1103/PhysRevD.102.012004Universidad del AtlánticoRepositorio Universidad del AtlánticoThe cross section of neutrino-induced neutral-current coherent π0 production on a carbon-dominated target is measured in the NOvA near detector. This measurement uses a narrow-band neutrino beam with an average neutrino energy of 2.7 GeV, which is of interest to ongoing and future long-baseline neutrino oscillation experiments. The measured, flux-averaged cross section is σ ¼ 13.8 0.9ðstatÞ 2.3ðsystÞ × 10−40 cm2=nucleus, consistent with model prediction. This result is the most precise measurement of neutral-current coherent π0 production in the few-GeV neutrino energy region.application/pdfenghttp://creativecommons.org/licenses/by-nc/4.0/Attribution-NonCommercial 4.0 Internationalinfo:eu-repo/semantics/openAccesshttp://purl.org/coar/access_right/c_abf2Physical ReviewMeasurement of neutrino-induced neutral-current coherent π0 production in the NOvA near detectorPúblico generalinfo:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArtículohttp://purl.org/coar/version/c_970fb48d4fbd8a85http://purl.org/coar/resource_type/c_2df8fbb1BarranquillaSede Norte[1] S. Adler, Phys. Rev. 135B, B963 (1964)[2] D. Rein and L. M. Sehgal, Nucl. Phys. B223, 29 (1983)[3] D. Rein and L. M. Sehgal, Phys. Lett. B 657, 207 (2007).[4] C. Andreopoulos et al., Nucl. Instrum. Methods Phys. Res., Sect. A 614, 87 (2010); arXiv:1510.05494v1.[5] C. Berger and L. M. Sehgal, Phys. Rev. D 79, 053003 (2009)[6] A. A. Belkov and B. Z. Kopeliovich, Sov. J. 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A 806, 279 (2016), FERMILAB-PUB-15-253-AD-FESSND.[29] The NOvA APD is a custom variant of the Hamamatsu S8550, http://www.hamamatsu.com/us/en/product/alpha/S/ 4112/S8550-02/index.html.[30] T. T. Bohlen, F. Cerutti, M. P. W. Chin, A. Fassò, A. Ferrari, P. G. Ortega, A. Mairani, P. R. Sala, G. Smirnov, and V. Vlachoudis, Nucl. Data Sheets 120, 211 (2014); A. Ferrari et al., CERN Reports No. CERN-2005-10, No. INFN/TC 05/11, and No. SLAC-R-773, 2005[31] M. Campanella et al., CERN Technical Report No. CERNATL-SOFT-99-004, 1999.[32] S. Agostinelli et al., Nucl. Instrum. Methods Phys. Res., Sect. A 506, 250 (2003); J. Allison et al., IEEE Trans. Nucl. Sci. 53, 270 (2006)[33] L. Aliaga et al. (MINERvA Collaboration), Phys. Rev. D 94, 092005 (2016[34] D. Rein and L. M. Sehgal, Ann. Phys. (N.Y.) 133, 79 (1981).[35] A. Bodek, I. Park, and U.-K. Yang, Nucl. Phys. B, Proc. Suppl. 139, 113 (2005)[36] D. Rein, Nucl. Phys. B278, 61 (1986)[37] B. Z. Kopeliovich, I. Schmidt, and M. Siddikov, Phys. Rev. D 85, 073003 (2012).[38] B. Z. Kopeliovich et al., Neutrinoproduction of pions off nuclei, http://atlas.fis.utfsm.cl/np/[39] A. Bodek and J. L. Ritchie, Phys. Rev. D 23, 1070 (1981)[40] A. Bodek and J. L. Ritchie, Phys. Rev. D 24, 1400 (1981).[41] L. Fernandes and M. Oliveira, Pattern Recognit. 41, 299 (2008).[42] E. Niner, Ph.D. thesis, Indiana University, 2015, FERMILABTHESIS-2015-16.[43] K. Sachdev, Ph.D. thesis, University of Minnesota, 2015, FERMILAB-THESIS-2015-20[44] P. Adamson et al. (NOvA Collaboration), Phys. Rev. D 96, 072006 (2017)[45] M. Tanabashi et al. (Particle Data Group), Phys. Rev. D 98, 030001 (2018)[46] A. Higuera et al. (MINERvA Collaboration) Phys. Rev. Lett. 113, 261802 (2014[47] A. Mislivec et al. (MINERvA Collaboration), Phys. Rev. D 97, 032014 (2018)[48] H. Duyang (NOvA Collaboration), arXiv:1511.00351.http://purl.org/coar/resource_type/c_6501ORIGINALPhysRevD.102.012004.pdfPhysRevD.102.012004.pdfapplication/pdf1733962https://repositorio.uniatlantico.edu.co/bitstream/20.500.12834/935/1/PhysRevD.102.012004.pdfaae5df65c90314705ad4ed8ce78e4e9dMD51CC-LICENSElicense_rdflicense_rdfapplication/rdf+xml; charset=utf-8914https://repositorio.uniatlantico.edu.co/bitstream/20.500.12834/935/2/license_rdf24013099e9e6abb1575dc6ce0855efd5MD52LICENSElicense.txtlicense.txttext/plain; charset=utf-81306https://repositorio.uniatlantico.edu.co/bitstream/20.500.12834/935/3/license.txt67e239713705720ef0b79c50b2ececcaMD5320.500.12834/935oai:repositorio.uniatlantico.edu.co:20.500.12834/9352022-11-15 16:04:00.631DSpace de la Universidad de Atlánticosysadmin@mail.uniatlantico.edu.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 |