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Journal articles on the topic 'OPERA Experiment'

Author: Grafiati

Published: 4 June 2021

Last updated: 10 March 2023

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1

Komatsu, M. "OPERA experiment." Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 503, no. 1-2 (May 2003): 124–26. http://dx.doi.org/10.1016/s0168-9002(03)00653-3.

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2

Gustavino, Carlo. "The OPERA experiment." Journal of Physics: Conference Series 39 (May 1, 2006): 326–28. http://dx.doi.org/10.1088/1742-6596/39/1/083.

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3

Jollet, C. "The OPERA experiment." Physics of Atomic Nuclei 69, no. 11 (November 2006): 1872–75. http://dx.doi.org/10.1134/s1063778806110093.

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4

Agafonova, N., A. Aleksandrov, A. Anokhina, S. Aoki, A. Ariga, T. Ariga, D. Bender, et al. "The OPERA experiment." Nuclear and Particle Physics Proceedings 267-269 (October 2015): 87–93. http://dx.doi.org/10.1016/j.nuclphysbps.2015.10.087.

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5

De Lellis, Giovanni. "The OPERA experiment." Nuclear Physics B - Proceedings Supplements 155, no. 1 (May 2006): 203–4. http://dx.doi.org/10.1016/j.nuclphysbps.2006.02.048.

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6

Sioli, Maximiliano. "The OPERA experiment." Nuclear Physics B - Proceedings Supplements 168 (June 2007): 173–75. http://dx.doi.org/10.1016/j.nuclphysbps.2007.02.074.

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7

Cozzi, M. "The OPERA experiment." Nuclear Physics B - Proceedings Supplements 172 (October 2007): 152–55. http://dx.doi.org/10.1016/j.nuclphysbps.2007.08.063.

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8

Dracos, M. "The OPERA experiment." Physics of Atomic Nuclei 67, no. 6 (June 2004): 1092–96. http://dx.doi.org/10.1134/1.1772442.

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9

Pessard, H. "The OPERA Experiment." Physica Scripta T93, no. 1 (2001): 59. http://dx.doi.org/10.1238/physica.topical.093a00059.

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10

Strauss, Thomas. "OPERA HIGHLIGHTS." Acta Polytechnica 53, A (December 18, 2013): 512–17. http://dx.doi.org/10.14311/ap.2013.53.0512.

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The OPERA experiment is a long baseline neutrino oscillation experiment aimed at observing the ν<sub>μ</sub> → ν<sub>τ</sub> neutrino oscillation in the CERN neutrino to Gran Sasso beamline in the appearance mode by detecting the τ-decay. Here I will summarize the results from the run years 2008–10 with an update on observed rare decay topologies and the results of the neutrino velocity measurements.

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11

Antonov, Alexander. "Comment on the OPERA Experiment." American Journal of Scientific and Industrial Research 2, no. 6 (December 2011): 890–91. http://dx.doi.org/10.5251/ajsir.2011.2.6.890.891.

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12

Mauri, N. "Highlights from the OPERA experiment." EPJ Web of Conferences 70 (2014): 00045. http://dx.doi.org/10.1051/epjconf/20147000045.

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13

Crescenzo, A. Di. "Results from the OPERA experiment." EPJ Web of Conferences 164 (2017): 01025. http://dx.doi.org/10.1051/epjconf/201716401025.

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14

Medinaceli, E. "Status of the OPERA experiment." Journal of Physics: Conference Series 442 (June 10, 2013): 012021. http://dx.doi.org/10.1088/1742-6596/442/1/012021.

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15

Nakamura, Mitsuhiro. "Status of the OPERA experiment." Nuclear Physics B - Proceedings Supplements 149 (December 2005): 147–49. http://dx.doi.org/10.1016/j.nuclphysbps.2005.05.030.

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16

Di Crescenzo, A. "Results from the OPERA experiment." Nuclear and Particle Physics Proceedings 265-266 (August 2015): 186–88. http://dx.doi.org/10.1016/j.nuclphysbps.2015.06.047.

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17

Adam, T., E. Baussan, K. Borer, J.-E. Campagne, N. Chon-Sen, C. de La Taille, N. Dick, et al. "The OPERA experiment Target Tracker." Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 577, no. 3 (July 2007): 523–39. http://dx.doi.org/10.1016/j.nima.2007.04.147.

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18

Tufanli, Serhan. "The OPERA Experiment and Recent Results." EPJ Web of Conferences 71 (2014): 00133. http://dx.doi.org/10.1051/epjconf/20147100133.

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19

Duchesneau, D. "Latest results from the OPERA experiment." Journal of Physics: Conference Series 888 (September 2017): 012004. http://dx.doi.org/10.1088/1742-6596/888/1/012004.

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20

Dmitrievsky, Sergey. "New results from the OPERA experiment." EPJ Web of Conferences 182 (2018): 02036. http://dx.doi.org/10.1051/epjconf/201818202036.

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The OPERA experiment reached its main goal by proving the appearance of νη in the CNGS νμ beam. A total sample of 5 candidates fulfilling the analysis defined in the proposal was detected with a S/B ratio of about ten allowing to reject the null hypothesis at 5.1σ. The search has been extended to γη-like interactions failing the kinematical analysis defined in the experiment proposal to obtain a statistically enhanced, lower purity, signal sample. Based on the enlarged data sample the estimation of Δm223 in appearance mode is presented. The search for νe interactions has been extended over the full data set with a more than twofold increase in statistics with respect to published data. The analysis of the νμ μ νe channel is updated and the implications of the electron neutrino sample in the framework of the 3+1 sterile model is discussed. An analysis of νμ μ νπ interactions in the framework of the sterile neutrino model has also been performed. Moreover the results of the analysis of the annual modulation of the cosmic muon rate will be presented.

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21

Mauri, N. "More results from the OPERA experiment." Journal of Physics: Conference Series 1342 (January 2020): 012036. http://dx.doi.org/10.1088/1742-6596/1342/1/012036.

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22

Duchesneau, D. "Recent Results from the OPERA Experiment." Physics Procedia 61 (2015): 467–74. http://dx.doi.org/10.1016/j.phpro.2014.12.109.

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23

Autiero, D. "Status of the OPERA experiment (CNGS1)." Nuclear Physics B - Proceedings Supplements 143 (June 2005): 257–61. http://dx.doi.org/10.1016/j.nuclphysbps.2005.01.114.

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24

Scotto Lavina, L. "Recent results from the OPERA experiment." Nuclear Physics B - Proceedings Supplements 188 (March 2009): 185–87. http://dx.doi.org/10.1016/j.nuclphysbps.2009.02.042.

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25

Mauri, N. "The OPERA experiment at Gran Sasso." Nuclear Physics B - Proceedings Supplements 196 (December 2009): 213–20. http://dx.doi.org/10.1016/j.nuclphysbps.2009.09.040.

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26

Di Marco, N. "Recent results of the OPERA experiment." Nuclear Physics B - Proceedings Supplements 237-238 (April 2013): 187–89. http://dx.doi.org/10.1016/j.nuclphysbps.2013.04.086.

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27

Di Ferdinando, Donato. "Nuclear emulsions in the OPERA experiment." Radiation Measurements 44, no. 9-10 (October 2009): 840–45. http://dx.doi.org/10.1016/j.radmeas.2009.10.060.

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28

Cocco, A. G. "The OPERA experiment at Gran Sasso." Nuclear Physics B - Proceedings Supplements 85, no. 1-3 (May 2000): 125–28. http://dx.doi.org/10.1016/s0920-5632(00)00494-1.

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29

Naganawa, N. "Emulsion analysis in the OPERA experiment." Journal of Physics: Conference Series 203 (January 1, 2010): 012106. http://dx.doi.org/10.1088/1742-6596/203/1/012106.

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30

Paoloni, Alessandro, and on Behalf of OPERA Collaboration. "Results from the OPERA Experiment in the CNGS Beam." Universe 4, no. 12 (December 7, 2018): 143. http://dx.doi.org/10.3390/universe4120143.

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The OPERA experiment was designed to observe ν μ → ν τ oscillations through τ appearance on the CERN Neutrino to Gran Sasso (CNGS) beam over a baseline of 730 km. OPERA was a hybrid experiment composed of lead plates and emulsion layers acting as a target for neutrino interactions. The experiment was complemented with electronic detectors: scintillator strips used as Target Trackers and muon spectrometers. A review of the OPERA final results is presented in this paper.

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31

De Lellis, Giovanni, and Giuliana Galati. "The major achievements of the OPERA experiment and its legacy." Modern Physics Letters A 36, no. 06 (January 29, 2021): 2130004. http://dx.doi.org/10.1142/s0217732321300044.

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The OPERA experiment was designed to discover the [Formula: see text] appearance in a pure [Formula: see text] beam, resulting from neutrino oscillations. The detector, located in the underground Gran Sasso Laboratory, consisted of an emulsion/lead target complemented by electronic detectors and was exposed, from 2008 to 2012, to the (CERN Neutrinos to Gran Sasso (CNGS)) beam, an almost pure [Formula: see text] beam with a baseline of 730 km, collecting a total of [Formula: see text] protons on target. OPERA was unique in its capability of detecting all three neutrino flavors. OPERA discovered [Formula: see text] oscillations in appearance mode with a significance of [Formula: see text]. In this review, we report the major achievements of the OPERA experiment and its legacy in the nuclear emulsion technology.

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32

YAN, MU-LIN, SEN HU, WEI HUANG, and NENG-CHAO XIAO. "ON DETERMINATION OF THE GEOMETRIC COSMOLOGICAL CONSTANT FROM THE OPERA EXPERIMENT OF SUPERLUMINAL NEUTRINOS." Modern Physics Letters A 27, no. 11 (April 10, 2012): 1250041. http://dx.doi.org/10.1142/s0217732312500411.

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The recent OPERA experiment of superluminal neutrinos has deep consequences in cosmology. In cosmology a fundamental constant is the cosmological constant. From observations one can estimate the effective cosmological constant Λ eff which is the sum of the quantum zero point energy Λ dark energy and the geometric cosmological constant Λ. The OPERA experiment can be applied to determine the geometric cosmological constant Λ. It is the first study to distinguish the contributions of Λ and Λ dark energy from each other by experiment. The determination is based on an explanation of the OPERA experiment in the framework of Special Relativity with de Sitter spacetime symmetry.

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33

Blennow, Mattias, Davide Meloni, Tommy Ohlsson, Francesco Terranova, and Mattias Westerberg. "Non-standard interactions using the OPERA experiment." European Physical Journal C 56, no. 4 (August 2008): 529–36. http://dx.doi.org/10.1140/epjc/s10052-008-0683-6.

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34

Di Giovanni, A., A. Candela, N. Di Marco, M. D'Incecco, C. Gustavino, M. Lindozzi, D. Orlandi, and E. Tatananni. "The Veto system of the OPERA experiment." Nuclear Physics B - Proceedings Supplements 158 (August 2006): 40–43. http://dx.doi.org/10.1016/j.nuclphysbps.2006.07.015.

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35

Baussan, E., K. Borer, J. E. Campagne, N. Chon-Sen, M. Dracos, Y. Gornushkin, J. L. Guyonnet, et al. "The neutrino oscillation OPERA experiment Target Tracker." Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 581, no. 1-2 (October 2007): 465–68. http://dx.doi.org/10.1016/j.nima.2007.08.028.

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36

Bertolin, A., R. Brugnera, A. Candela, E. Cararra, L. Castellani, A. Cazes, G. Corradi, et al. "The RPC system of the OPERA experiment." Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 602, no. 3 (May 2009): 631–34. http://dx.doi.org/10.1016/j.nima.2008.12.071.

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37

Amata, E., P. Baldetti, G. Bellucci, V. Formisano, A. Morbidini, S. Orsini, A. Pavoni, R. Terenzi, and M. Viterbini. "The experiment OPERA for the mission Interball." Il Nuovo Cimento C 13, no. 1 (January 1990): 155–61. http://dx.doi.org/10.1007/bf02515785.

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38

Wilquet, G. "The OPERA long baseline neutrino oscillation experiment." Journal of Physics: Conference Series 110, no. 8 (May 1, 2008): 082022. http://dx.doi.org/10.1088/1742-6596/110/8/082022.

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39

Galati, Giuliana. "Final results of the OPERA experiment on ντ appearance and the OPERA “legacy”." Journal of Physics: Conference Series 1226 (May 2019): 012022. http://dx.doi.org/10.1088/1742-6596/1226/1/012022.

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40

MA, BO-QIANG. "THE PHANTOM OF THE OPERA: SUPERLUMINAL NEUTRINOS." Modern Physics Letters A 27, no. 04 (February 10, 2012): 1230005. http://dx.doi.org/10.1142/s0217732312300054.

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This is a brief review on the experimental measurements of the muon neutrino velocities from the OPERA, Fermilab and MINOS experiments and that of the (anti)-electron neutrino velocities from the supernova SN1987A, and consequently on the theoretical attempts to attribute the data as signals for superluminality of neutrinos. Different scenarios on how to understand and treat the background fields in the effective field theory frameworks are pointed out. Challenges on interpreting the OPERA result as a signal of neutrino superluminality are briefly reviewed and discussed. It is also pointed out that a covariant picture of Lorentz violation can avoid the refutation on the OPERA experiment.

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41

Di Crescenzo, Antonia. "OPERA: Status and prospects." Modern Physics Letters A 29, no. 08 (March 14, 2014): 1430008. http://dx.doi.org/10.1142/s0217732314300080.

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The Oscillation Project with Emulsion-tRacking Apparatus (OPERA) neutrino experiment was designed to perform a unique appearance measurement in the CNGS beam to confirm the oscillation mechanism in the atmospheric sector. Runs were successfully carried out from 2008 to 2012. The status of the analysis is reported and the topology and the kinematics of the first three ντ candidate events are described. A first result of the νμ→νe oscillation search is also presented.

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42

Pastore, A. "Search for charmed hadrons in the OPERA experiment." EPJ Web of Conferences 95 (2015): 04050. http://dx.doi.org/10.1051/epjconf/20159504050.

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43

Sirignano, Chiara. "The CNGS project and OPERA experiment at LNGS." Nuclear Physics B - Proceedings Supplements 221 (December 2011): 268–72. http://dx.doi.org/10.1016/j.nuclphysbps.2011.09.015.

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44

Di Marco, N., K. Hamada, and Y. Nonoyama. "The Emulsion Scanning System of the OPERA experiment." Nuclear Physics B - Proceedings Supplements 229-232 (August 2012): 469. http://dx.doi.org/10.1016/j.nuclphysbps.2012.09.106.

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45

Dracos, M. "Measurement of the neutrino velocity in OPERA experiment." Nuclear Physics B - Proceedings Supplements 235-236 (February 2013): 283–88. http://dx.doi.org/10.1016/j.nuclphysbps.2013.04.023.

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46

Candela, A., E. Carrara, M. D’Incecco, A. Di Giovanni, S. Dusini, C. Gustavino, A. Lindozzi, et al. "Glass resistive plate chambers in the OPERA experiment." Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 581, no. 1-2 (October 2007): 206–8. http://dx.doi.org/10.1016/j.nima.2007.07.065.

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47

Li, Na. "Multimedia Drama Imaging Technology Based on Big Data Information System." Mobile Information Systems 2022 (July 31, 2022): 1–15. http://dx.doi.org/10.1155/2022/4765619.

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Opera is a unique comprehensive stage art form in China. As a traditional Chinese drama style, it is known as the three ancient drama cultures in the world together with the tragicomedy of ancient Greece and the Sanskrit drama of India. However, in the trend of the new era, Chinese opera is facing a severe existential crisis. How to innovate the opera and make people fall in love with the opera again is a problem worthy of research and analysis at present. This study takes the research of multimedia opera image technology as the object, aims to improve the perception and experience of opera, and studies how to use modern technology to improve opera image. First, this study briefly expounds on the presentation methods and current situation of traditional opera video technology. This study then describes in detail the imaging technology that combines opera and modern technology and then establishes the algorithm model of virtual reality imaging technology. And it then describes in detail the video technology that combines Chinese opera with multimedia technologies such as projection and virtual reality interaction. It then established a virtual reality technology algorithm model for opera images. This study then experiments, analyzes, and improves the multimedia opera video technology based on virtual reality. Finally, by means of a questionnaire survey, it investigates and analyzes the viewing attitude of opera images based on virtual reality technology. Through the research of virtual reality image technology and the investigation of citizens, this study obtains the methods and models to improve traditional opera images and effectively innovates opera. In a survey of citizens, it was found that nearly 70% of the respondents held a positive and optimistic attitude toward the virtual reality-based opera video technology, indicating that people are willing to accept the combination of traditional culture and modern technology. In the element loss detection experiment, it was found that nearly 70% of the interviewees were very interested in the method of combining traditional opera with modern technology. The model of virtual opera scene construction was improved so that the element loss rate was lower than 4%. The element representation delay is less than 3%, which improves the smoothness of the picture and maintains a good viewing experience.

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48

Huck, Steffen, Imran Rasul, and Andrew Shephard. "Comparing Charitable Fundraising Schemes: Evidence from a Natural Field Experiment and a Structural Model." American Economic Journal: Economic Policy 7, no. 2 (May 1, 2015): 326–69. http://dx.doi.org/10.1257/pol.20120312.

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We present evidence from a natural field experiment and structural model to shed light on the efficacy of alternative fundraising schemes. In conjunction with the Bavarian State Opera, we mailed 25,000 opera attendees a letter describing a charitable fundraising project organized by the opera house. Recipients were randomly assigned to treatments designed to explore responses to fundraising schemes varying in: the presence of a lead donor; and how individual donations would be matched using the lead donation. The structural model estimates extensive and intensive margin responses, and is then utilized to predict giving behavior in counterfactual fundraising schemes. (JEL C93, D64, L31, L82)

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49

Mauri, N. "Results from the OPERA experiment at the CNGS beam." EPJ Web of Conferences 164 (2017): 01026. http://dx.doi.org/10.1051/epjconf/201716401026.

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50

Kreslo, Igor E. "Opera neutrino oscillation experiment: On the way to ντobservation." Journal of Physics: Conference Series 171 (June 1, 2009): 012066. http://dx.doi.org/10.1088/1742-6596/171/1/012066.

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