The DOI matches its Crossref record; 30 of the 30 references it cites were found in a registry or an index.
New results on ν μ → ν τ appearance with the OPERA experiment in the CNGS beam
Open accessAbstract
The OPERA neutrino experiment is designed to perform the first observation of neutrino oscillations in direct appearance mode in the ν μ → ν τ channel, via the detection of the τ-leptons created in charged current ν τ interactions. The detector, located in the underground Gran Sasso Laboratory, consists of an emulsion/lead target with an average mass of about 1.2 kt, complemented by electronic detectors. It is exposed to the CERN Neutrinos to Gran Sasso beam, with a baseline of 730 km and a mean energy of 17 GeV. The observation of the first ν τ candidate event and the analysis of the 2008-2009 neutrino sample have been reported in previous publications. This work describes substantial improvements in the analysis and in the evaluation of the detection efficiencies and backgrounds using new simulation tools. The analysis is extended to a sub-sample of 2010 and 2011 data, resulting from an electronic detector-based pre-selection, in which an additional ν τ candidate has been observed. The significance of the two events in terms of a ν μ → ν τ oscillation signal is of 2.40 σ.
Overview
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Integrity signals
Registry
Cites
Statistics
Verification
Claims the paper makes
The claims and statistics of this paper haven’t been checked yet.
Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.
Self-check
Percentages, sums and reported differences re-computed from the paper’s own numbers.
The self-check needs the paper’s full text.
Citations
Cites
Olive, K. A. (2016) · Chinese Physics C · doi:10.1088/1674-1137/40/10/100001 · Cited by 7,334
Nakamura, K. (2010) · Journal of Physics G: Nuclear and Particle Physics · doi:10.1088/0954-3899/37/7a/075021 · Cited by 5,797
Evidence for Oscillation of Atmospheric Neutrinos
Fukuda, Y., Hayakawa, T., Ichihara, E., Inoue, K., Ishihara, K., Ishino, H., Itow, Y., Kajita, T., Kameda, J., Kasuga, S., et al. (1998) · Physical Review Letters · doi:10.1103/physrevlett.81.1562 · Cited by 5,067
Self-citationRemarks on the unified model of elementary particles
Maki, Z., Nakagawa, M., & Sakata, S. (1962) · Progress of Theoretical Physics · doi:10.1143/ptp.28.870 · Cited by 3,355
FLUKA: A Multi-Particle Transport Code
Ferrari, A., Sala, P. R., Fasso, A., & Ranft, J. (2005) · doi:10.2172/877507 · Cited by 2,536
Observation of Electron-Antineutrino Disappearance at Daya Bay
An, F. P., Bai, J. Z., Balantekin, A. B., Band, H. R., Beavis, D., Beriguete, W., Bishai, M., Blyth, S., Boddy, K., Brown, R. L., et al. (2012) · Physical Review Letters · doi:10.1103/physrevlett.108.171803 · Cited by 2,189
Self-citationAhmad, Q. R., Allen, R. C., Andersen, T. C., Anglin, J. D., Bühler, G., Barton, J. C., Beier, E. W., Bercovitch, M., Bigu, J., Biller, S., et al. (2001) · Physical Review Letters · doi:10.1103/physrevlett.87.071301 · Cited by 1,936
Observation of Reactor Electron Antineutrinos Disappearance in the RENO Experiment
Ahn, J. K., Chebotaryov, S., Choi, J. H., Choi, S., Choi, W., Choi, Y., Jang, H. I., Jang, J. S., Jeon, E. J., Jeong, I. S., et al. (2012) · Physical Review Letters · doi:10.1103/physrevlett.108.191802 · Cited by 1,869
Self-citationIndication of Electron Neutrino Appearance from an Accelerator-Produced Off-Axis Muon Neutrino Beam
Abe, K., Abgrall, N., Ajima, Y., Aihara, H., Albert, J. B., Andreopoulos, C., Andrieu, B., Aoki, S., Araoka, O., Argyriades, J., et al. (2011) · Physical Review Letters · doi:10.1103/physrevlett.107.041801 · Cited by 1,330
Self-citationGALLEX solar neutrino observations: results for GALLEX IV
Hampel, W., Handt, J., Heusser, G., Kiko, J., Kirsten, T., Laubenstein, M., Pernicka, E., Rau, W., Wojcik, M., Zakharov, Y., et al. (1999) · Physics Letters B · doi:10.1016/s0370-2693(98)01579-2 · Cited by 1,329
Cited by
Conformal symmetry and its breaking in two-dimensional nearly anti-de Sitter space
Maldacena, J., Stanford, D., & Yang, Z. (2016) · Progress of Theoretical and Experimental Physics · doi:10.1093/ptep/ptw124 · Cited by 1,068
Replica wormholes and the entropy of Hawking radiation
Almheiri, A., Hartman, T., Maldacena, J., Shaghoulian, E., & Tajdini, A. (2020) · Journal of High Energy Physics · doi:10.1007/jhep05(2020)013 · Cited by 910
The spectrum in the Sachdev-Ye-Kitaev model
Polchinski, J., & Rosenhaus, V. (2016) · Journal of High Energy Physics · doi:10.1007/jhep04(2016)001 · Cited by 699
An investigation of AdS2 backreaction and holography
Engelsöy, J., Mertens, T. G., & Verlinde, H. (2016) · Journal of High Energy Physics · doi:10.1007/jhep07(2016)139 · Cited by 622
(2017) · Institutional Repositories DataBase (IRDB) · Cited by 323
Metadata
- Authors
- The OPERA collaboration, Agafonova, N., Aleksandrov, A., Anokhina, A., Aoki, S., Ariga, A., Ariga, T., Asada, T., Autiero, D., Badertscher, A., Ben Dhahbi, A., Bender, D., Bertolin, A., Bozza, C., Brugnera, R., Brunetti, G., Büttner, B., Buontempo, S., Chaussard, L., Chernyavskiy, M., Chiarella, V., Chukanov, A., Consiglio, L., D’Ambrosio, N., Del Amo Sanchez, P., De Lellis, G., De Serio, M., Di Crescenzo, A., Di Ferdinando, D., Di Marco, N., Dmitrievski, S., Dracos, M., Duchesneau, D., Dusini, S., Ebert, J., Ereditato, A., Favier, J., Ferber, T., Fini, R. A., Fukuda, T., Garfagnini, A., Giacomelli, G., Goellnitz, C., Goldberg, J., Gornushkin, Y., Grella, G., Grianti, F., Guler, A. M., Gustavino, C., Hagner, C., Hakamata, K., Hara, T., Hayakawa, T., Hierholzer, M., Hollnagel, A., Hosseini, B., Ishida, H., Ishiguro, K., Ishikawa, M., Jakovcic, K., Jollet, C., Kamiscioglu, C., Kamiscioglu, M., Katsuragawa, T., Kawahara, H., Kawada, J., Kim, J. H., Kim, S. H., Kimura, M., Kitagawa, N., Klicek, B., Kodama, K., Komatsu, M., Kose, U., Kreslo, I., Lauria, A., Lenkeit, J., Ljubicic, A., Longhin, A., Loverre, P., Malgin, A., Mandrioli, G., Marteau, J., Matsuo, T., Matveev, V., Mauri, N., Medinaceli, E., Meregaglia, A., Migliozzi, P., Mikado, S., Minotti, A., Miyanishi, M., Miyashita, E., Monacelli, P., Montesi, M. C., Morishima, K., Muciaccia, M. T., Naganawa, N., Naka, T., Nakamura, M., Nakano, T., Nakatsuka, Y., Niwa, K., Ogawa, S., Okateva, N., Olshevsky, A., Omura, T., Ozaki, K., Paoloni, A., Park, B. D., Park, I. G., Pastore, A., Patrizii, L., Pennacchio, E., Pessard, H., Pistillo, C., Podgrudkov, D., Polukhina, N., Pozzato, M., Pretzl, K., Pupilli, F., Rescigno, R., Roda, M., Roganova, T., Rokujo, H., Rosa, G., Rostovtseva, I., Rubbia, A., Russo, A., Ryazhskaya, O., Sato, O., Sato, Y., Schembri, A., Schmidt-Parzefall, W., Shakiryanova, I., Schcedrina, T., Sheshukov, A., Shibuya, H., Shiraishi, T., Shoziyoev, G., Simone, S., Sioli, M., Sirignano, C., Sirri, G., Spinetti, M., Stanco, L., Starkov, N., Stellacci, S. M., Stipcevic, M., Strauss, T., Strolin, P., Suzuki, K., Takahashi, S., Tenti, M., Terranova, F., Tioukov, V., Tolun, P., Tufanli, S., Vilain, P., Vladimirov, M., Votano, L., Vuilleumier, J. L., Wilquet, G., Wonsak, B., Yoon, C. S., Yoshida, J., Yoshimoto, M., Zaitsev, Y., Zemskova, S., & Zghiche, A.
- Venue
- Journal of High Energy Physics
- Published
- 2013-11
- Volume
- 2013
- Issue
- 11
- ISSN
- 1029-8479 (ISSN-L)
- OpenAlex
- W1521496145
- Cited by
- 278
- References
- 30
- FWCI
- 15.78
- Type
- journal article
- Language
- en
- Open access
- hybrid
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
Are you an author, or do you see a problem with this page? Request a review
How to cite
Cite CoChat for the checks on this page, and the paper for its own findings.
- This page
- CoChat. (2026). Citation check: New results on ν μ → ν τ appearance with the OPERA experiment in the CNGS beam. https://app.cochat.ai/papers/10.1007/jhep11(2013)036
- The paper
- The OPERA collaboration, Agafonova, N., Aleksandrov, A., Anokhina, A., Aoki, S., Ariga, A., Ariga, T., Asada, T., Autiero, D., Badertscher, A., Ben Dhahbi, A., Bender, D., Bertolin, A., Bozza, C., Brugnera, R., Brunetti, G., Büttner, B., Buontempo, S., Chaussard, L., . . . Zghiche, A. (2013). New results on ν μ → ν τ appearance with the OPERA experiment in the CNGS beam. Journal of High Energy Physics. https://doi.org/10.1007/jhep11(2013)036
Data sources
Bibliographic data: Semantic Scholar, OpenAlex, Crossref.
Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.