Relevant bibliographies by topics / OPERA Experiment

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  1. Journal articles
  2. Dissertations / Theses
  3. Books
  4. Book chapters
  5. Conference papers
  6. Reports

Academic literature on the topic 'OPERA Experiment'

Author: Grafiati
Published: 4 June 2021
Last updated: 10 March 2023

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Journal articles on the topic "OPERA Experiment"

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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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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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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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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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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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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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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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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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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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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Dissertations / Theses on the topic "OPERA Experiment"

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Kamiscioglu, Mustafa. "Analysis Of Neutrino Interactions In The Opera Experiment." Master's thesis, METU, 2012. http://etd.lib.metu.edu.tr/upload/12614023/index.pdf.

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OPERA stands for Oscillation Project with Emulsion t-Racking Apparatus. The main goal of the OPERA experiment is to search for tau neutrino appearance in almost pure muon neutrino beam. The detector is located at Gran Sasso, 730 km away from the neutrino source, at CERN. In this thesis, the reconstruction efficiency and purity of neutrino interactions in the OPERA target have been studied by using Monte Carlo simulation. The efficiency of primary vertex reconstruction for muon neutrino Charge Current (CC) events is estimated as 83.2 percent. The main source of inefficiency is due to Quasi-elastic like topologies in which only one track is reconstructed. The purity of primary vertex tracks is found to be 99 percent. On the other hand, the reconstruction efficiency for muon neutrino CC charm events is estimated to be 90.2 percent, while the purity of the primary tracks is 67 percent. The low purity is due the fact that the secondary vertex tracks are wrongly assigned in the primary vertex. This spoils the purity.
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Tufanli, Serhan. "D0 Background To Neutrino Oscillations In The Opera Experiment." Master's thesis, METU, 2009. http://etd.lib.metu.edu.tr/upload/12610330/index.pdf.

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The OPERA experiment is designed to search for nu-tau appearance in almost pure CERN-SPS nu-mu beam. The OPERA detector is placed in the Gran Sasso underground laboratory which is 730 km away from CERN. It is a hybrid set-up which combines a lead/emulsion target with various electronic detectors. The detector is composed of two super modules(SM) which contains about 150,000 ECC bricks. Each of the brick is obtained by stacking 56 lead plates with 57 emulsion films. Behind the each brick, an emulsion film doublet, called Changeable Sheet (CS) is attached in order to confirm tracks produced in neutrino interactions. The CS requires very low background track density in order to ensure the expected performance in the experiment. The background tracks in CS can be erased by a special treatment called as refreshing. A refreshing facility was constructed in the LNGS laboratory. The METU group has participated in the construction of the facility and the production of the CS films from the beginning. The main steps of emulsion refreshing and the test results on emulsion quality after the refreshing will be discussed. A Monte Carlo simulation is performed in order to estimate background to nu-mu to nu-tau oscillation due to D0 production and decay in the ECC brick. It is found that this background is significant for the short decay path topology of the tau lepton.
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Meneer, Nathanael. "Horatio Parker's Mona: an experiment in American grand opera." Thesis, Boston University, 2012. https://hdl.handle.net/2144/32036.

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Thesis (M.A.)--Boston University
Horatio William Parker (1863-1919) was a prominent American composer who belonged to the Second New England School (the "Boston Six"), and served as the Dean of Music at Yale University from 1904 until his death. His opera Mona (Opus 71) was created in collaboration with his librettist, Brian Hooker (1880-1946), as an entry to a contest that was being held by the Metropolitan Opera Company for the best English-language opera written by an American-born composer. Parker and Hooker won the contest, and received $10,000 in prize money along with a production of Mona at the Met. The contest generated a considerable amount of interest in the American musical community, and sparked debate concerning the characteristics that should epitomize "American" opera. After difficult rehearsals and extensive revisions, Mona premiered on March 14'h, 1912. Despite its lavish production, the opera was met with a lukewarm reception by the American public, and failed to make its way into the permanent repertory of the Met. Willie American opera of this era was commonly criticized for being simple and frivolous, Mona is notable for being a serious opera of considerable complexity that was ultimately rejected by the American public. The opera is also significant in that it seems to mark a turning point in Parker's biography, after which he placed greater emphasis on the popular appeal of his compositions.
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Roda, Marco. "Study of multiple vertices neutrino interactions in the OPERA experiment." Doctoral thesis, Università degli studi di Padova, 2016. http://hdl.handle.net/11577/3426767.

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OPERA is a long baseline neutrino experiment designed for tau neutrino searches in an almost pure muon neutrino beam. The detection is performed on an event-by-event basis which is possible thanks to the high spatial resolution of the detector. In fact, the set-up is able to observe very short decaying particles produced in neutrino interactions, such as tau or charmed particles. In particular, the experiment searches for events with one secondary vertex within 1 mm from the primary one. An event was recorded with an unexpected topology: instead of one secondary vertex it has two. Such an event was completely unexpected and a totally new analysis was required in order to understand its nature. The possibilities taken into account include most of the combinations of tau, charmed particle and hadron re-interaction within the lead. The new software, based on GEANT4, was set-up and successfully tested using a dedicated OPERA test beam. Thus, an ad hoc Monte Carlo generation was prepared in order to describe the properties of such a rare observation. Finally, a sample having the interesting topology was obtained and a blind procedure for the event identification could be developed. The event turned out to be very likely an tau neutrino interaction with charm production with a significance close to 3.5 sigma.
OPERA è un esperimento per lo studio di neutrini da fascio progettato per ricerca di neutrini del tau in un fascio quasi puro di neutrini muonici. La ricerca è basata su un’analisi evento per evento che è resa possibile dall’elevata risoluzione spaziale del rivelatore. Infatti, l’apparato è in grado di osservare particelle emesse durante un’interazione di neutrino che decadono entro brevi distanze. In particolare, l’esperimento ricerca eventi che presentano vertici secondari entro circa un millimetro dal vertice primario di interazione. Un evento interessante è stato osservato con una topologia inaspettata: invece un solo vertice secondario ne sono stati osservati due. Questo tipo di eventi era completamente inaspettato e una nuova analisi era necessaria per capire la natura dell’evento. Le possibilità considerate includono quasi tutte le combinazioni di tau, particelle charmate e reinterazioni adroniche nel piombo. Un nuovo algoritmo di simulazione, basato su GEANT4, è stato sviluppato e testato con successo usando i dati di uno dei test beam di OPERA. Quindi, una nuova produzione Monte Carlo è stata preparata per poter descrivere le proprietà di questo raro fenomeno. Infine, è stata preparata un’analisi per l’identificazione dell’evento osservato. L’evento è risultato essere molto probabilmente un’interazione di neutrino del tau con produzione di charm, con una significanza di quasi 3.5 sigma.
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Brunetti, Giulia. "Neutrino velocity measurement with the OPERA experiment in the CNGS beam." Phd thesis, Université Claude Bernard - Lyon I, 2011. http://tel.archives-ouvertes.fr/tel-00843100.

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The thesis concerns the measurement of the neutrino velocity with the OPERA experiment in the CNGS beam. There are different theoretical models that allow for Lorentz violating effects which can be investigated with measurements on terrestrial neutrino beams. The MINOS experiment published in 2007 a measure on the muon neutrinos over a distance of 730 km finding a deviation with respect to the expected time of flight of 126 ns with a statistical error of 32 ns and a systematic error of 64 ns. The OPERA experiment observes as well muon neutrinos 730 km away from the source, with a sensitivity significantly better than MINOS thanks to the higher number of interactions in the detector due to the higher energy beam and the much more sophisticated timing system explicitly upgraded in view of the neutrino velocity measurement. This system is composed by atomic cesium clocks and GPS receivers operating in "common view mode". Thanks to this system a time-transfer between the two sites with a precision at the level of 1 ns is possible. Moreover, a Fast Waveform Digitizer was installed along the proton beam line at CERN in order to measure the internal time structure of the proton pulses that are sent to the CNGS target. The result on the neutrino velocity is the most precise measurement so far with terrestrial neutrino beams: the neutrino time of flight was determined with a statistical uncertainty of about 10 ns and a systematic uncertainty smaller than 20 ns.
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Brunetti, Giulia <1981&gt. "Neutrino velocity measurement with the OPERA experiment in the CNGS beam." Doctoral thesis, Alma Mater Studiorum - Università di Bologna, 2011. http://amsdottorato.unibo.it/3917/1/brunetti_giulia_tesi.pdf.

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In the thesis is presented the measurement of the neutrino velocity with the OPERA experiment in the CNGS beam, a muon neutrino beam produced at CERN. The OPERA detector observes muon neutrinos 730 km away from the source. Previous measurements of the neutrino velocity have been performed by other experiments. Since the OPERA experiment aims the direct observation of muon neutrinos oscillations into tau neutrinos, a higher energy beam is employed. This characteristic together with the higher number of interactions in the detector allows for a measurement with a much smaller statistical uncertainty. Moreover, a much more sophisticated timing system (composed by cesium clocks and GPS receivers operating in “common view mode”), and a Fast Waveform Digitizer (installed at CERN and able to measure the internal time structure of the proton pulses used for the CNGS beam), allows for a new measurement with a smaller systematic error. Theoretical models on Lorentz violating effects can be investigated by neutrino velocity measurements with terrestrial beams. The analysis has been carried out with blind method in order to guarantee the internal consistency and the goodness of each calibration measurement. The performed measurement is the most precise one done with a terrestrial neutrino beam, the statistical accuracy achieved by the OPERA measurement is about 10 ns and the systematic error is about 20 ns.
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Brunetti, Giulia <1981&gt. "Neutrino velocity measurement with the OPERA experiment in the CNGS beam." Doctoral thesis, Alma Mater Studiorum - Università di Bologna, 2011. http://amsdottorato.unibo.it/3917/.

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In the thesis is presented the measurement of the neutrino velocity with the OPERA experiment in the CNGS beam, a muon neutrino beam produced at CERN. The OPERA detector observes muon neutrinos 730 km away from the source. Previous measurements of the neutrino velocity have been performed by other experiments. Since the OPERA experiment aims the direct observation of muon neutrinos oscillations into tau neutrinos, a higher energy beam is employed. This characteristic together with the higher number of interactions in the detector allows for a measurement with a much smaller statistical uncertainty. Moreover, a much more sophisticated timing system (composed by cesium clocks and GPS receivers operating in “common view mode”), and a Fast Waveform Digitizer (installed at CERN and able to measure the internal time structure of the proton pulses used for the CNGS beam), allows for a new measurement with a smaller systematic error. Theoretical models on Lorentz violating effects can be investigated by neutrino velocity measurements with terrestrial beams. The analysis has been carried out with blind method in order to guarantee the internal consistency and the goodness of each calibration measurement. The performed measurement is the most precise one done with a terrestrial neutrino beam, the statistical accuracy achieved by the OPERA measurement is about 10 ns and the systematic error is about 20 ns.
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Altinok, Ozgur. "High-speed Automatic Scanning System For Emulsion Analysis In The Opera Experiment." Master's thesis, METU, 2011. http://etd.lib.metu.edu.tr/upload/12613364/index.pdf.

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The aim of the OPERA experiment is to verify the neutrino oscillation, directly measuring the appearance of from an initially pure beam produced at CERN. For this purpose OPERA detector is located underground Gran Sasso Laboratory(LNGS) 730 km away from CERN. The detector structure designed to be a hybrid system consisting of emulsion targets and electronic detectors. Total area of the emulsion targets in the OPERA detector is around 110000 m2 which needs fast and reliable automatic scanning systems. For this purpose, two dierent automatic scanning systems were developed in Japan and Europe. For now there are 12 scanning laboratories dedicated to the OPERA Experiment. The Emulsion Scanning Laboratory in the Physics department of METU is one of the scanning laboratories for the OPERA Experiment. The automatic scanning system in METU is European type which is using commercial hardware for easy construction and maintain. Also the laboratory has a unique feature in terms of experimental high energy physics laboratories. The emulsion scan- ning laboratory in METU is the
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Hosseini, Behzad. "Neutrino Interaction Analysis With An Automatic Scanning System In The Opera Experiment." Master's thesis, METU, 2012. http://etd.lib.metu.edu.tr/upload/12614370/index.pdf.

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The OPERA experiment was designed to search for nu-mu to nu-tau oscillations through the observation of nu-tau charged-current interactions in the OPERA target. This search requires a massive detector and very high spatial accuracy. Both requirements are ful
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Pozzato, Michele <1980&gt. "Reconstruction of CNGS neutrino events in the emulsions of the OPERA experiment." Doctoral thesis, Alma Mater Studiorum - Università di Bologna, 2009. http://amsdottorato.unibo.it/1755/1/PhD_Theses_Pozzato.pdf.

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The OPERA experiment aims at the direct observation of ν_mu -> ν_tau oscillations in the CNGS (CERN Neutrinos to Gran Sasso) neutrino beam produced at CERN; since the ν_e contamination in the CNGS beam is low, OPERA will also be able to study the sub-dominant oscillation channel ν_mu -> ν_e. OPERA is a large scale hybrid apparatus divided in two supermodules, each equipped with electronic detectors, an iron spectrometer and a highly segmented ~0.7 kton target section made of Emulsion Cloud Chamber (ECC) units. During my research work in the Bologna Lab. I have taken part to the set-up of the automatic scanning microscopes studying and tuning the scanning system performances and efficiencies with emulsions exposed to a test beam at CERN in 2007. Once the triggered bricks were distributed to the collaboration laboratories, my work was centered on the procedure used for the localization and the reconstruction of neutrino events.
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Books on the topic "OPERA Experiment"

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Musiktheater im Experiment: Fünfundzwanzig Aufsätze. Berlin: Lukas, 2004.

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translator, Levin Becker Daniel, Monk Ian translator, Noteboom Michelle translator, and Poucel Jean-Jacques translator, eds. Minute-operas. Providence: Burning Deck/Anyart, 2014.

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Fieled, Adam. Opera Bufa: Expanded Edition. Edited by Otoliths, Mark Young, and Adam Fieled. Conshohocken, Pa: IA (Funtime Press), 2013.

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Young, Mark, ed. Opera Bufa. Rockhampton, Queensland, Australia: Otoliths, 2007.

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1952-, Taymor Julie, ed. Julie Taymor, playing with fire: Theater, opera, film. New York: H.N. Abrams, 1995.

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Fieled, Adam. Opera Bufa (prefaced edition '13). Edited by Otoliths and Mark Young. Conshohocken, Pa: IA (Funtime Press), 2013.

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Smet, Julien de. The Orphans of Tar -: A speculative opera. Sint-Amandsberg: Art Paper Editions, 2019.

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Fieled, Adam. Opera Bufa (original Otoliths book pdf). Edited by Mark Young. Rockhampton, Queensland, Australia: Otoliths, 2007.

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Young, Mark, ed. Opera Bufa (excerpt: OB in Otoliths 6). Rockhampton, Australia: Otoliths, 2007.

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Room, Red, ed. Opera Bufa (excerpt: OB in RR '14). California, USA: Red Room, 2014.

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Book chapters on the topic "OPERA Experiment"

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Chukanov, A. "OPERA Experiment — Status Report." In NATO Science for Peace and Security Series B: Physics and Biophysics, 89–95. Dordrecht: Springer Netherlands, 2009. http://dx.doi.org/10.1007/978-90-481-2287-5_9.

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Łętowska, Ewa, and Krzysztof Pawłowski. "What Is Allowed in the Opera: Law as the Borderline of Artistic Experiment." In Law and Opera, 297–314. Cham: Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-319-68649-3_20.

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Döhring, Sieghart. "Zwischen Welttheater und Experiment: französisches Musiktheater im 20. Jahrhundert." In Oper im 20. Jahrhundert, 282–302. Stuttgart: J.B. Metzler, 2000. http://dx.doi.org/10.1007/978-3-476-03796-1_11.

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Holland, Dietmar. "Mozarts geniale musikalische Experimente La clemenza di Tito — die Rückkehr zur Opera seria?" In »Der moderne Komponist baut auf der Wahrheit«, 266–72. Stuttgart: J.B. Metzler, 2003. http://dx.doi.org/10.1007/978-3-476-02925-6_34.

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Ariga, Tomoko. "NEW RESULTS FROM THE OPERA EXPERIMENT." In Particle Physics at the Year of Light, 54–60. WORLD SCIENTIFIC, 2017. http://dx.doi.org/10.1142/9789813224568_0008.

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Autiero, D., M. Komatsu, P. Migliozzi, and F. Terranova. "The OPERA Experiment in the CNGS Beam." In Neutrino Oscillations, 173–96. WORLD SCIENTIFIC, 2008. http://dx.doi.org/10.1142/9789812771971_0009.

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Zemskova, Svetlana. "SEARCH FOR vμ → ve OSCILLATIONS IN THE OPERA EXPERIMENT." In Particle Physics at the Year of Light, 147–50. WORLD SCIENTIFIC, 2017. http://dx.doi.org/10.1142/9789813224568_0022.

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Rescigno, R. "THE ELECTRONIC DETECTORS OF THE HYBRID OPERA NEUTRINO EXPERIMENT." In Particle Physics at the Tercentenary of Mikhail Lomonosov, 120–23. WORLD SCIENTIFIC, 2013. http://dx.doi.org/10.1142/9789814436830_0026.

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Pupilli, Fabio. "SEARCH FOR ντINTERACTIONS WITH THE NUCLEAR EMULSION FILMS OF THE OPERA EXPERIMENT." In Particle Physics at the Tercentenary of Mikhail Lomonosov, 116–19. WORLD SCIENTIFIC, 2013. http://dx.doi.org/10.1142/9789814436830_0025.

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Marrone, Gaetana. "Operatic Microhistory." In The Cinema of Francesco Rosi, 121–52. Oxford University Press, 2020. http://dx.doi.org/10.1093/oso/9780190885632.003.0004.

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Il momento della verità (The Moment of Truth, 1965), a thematic departure from earlier films, is a bold experiment in shooting “freely” without a script. The film, informed by a keen sense of class consciousness and Rosi's penchant for location shooting, centers on the career of a matador, Miguel Mateo “Miguelín,” a peon who leaves the country for the city to escape poverty. Visually, Rosi’s searing exposure of the corruption and exploitation rampant in contemporary Spain is achieved through the use of a long 300mm lens. Sacrificial rituals also lie at the heart of Carmen (Bizet’s Carmen, 1984), Rosi's only experiment in opera adaptation. Also shot in Andalusia and featuring actual soldiers, gypsies, and locals, Carmen counterposes realistic settings to staged theatricality.
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Conference papers on the topic "OPERA Experiment"

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PESSARD, HENRI. "THE OPERA EXPERIMENT." In Proceedings of the 32nd International Conference. World Scientific Publishing Company, 2005. http://dx.doi.org/10.1142/9789812702227_0033.

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GORNUSHKIN, YU. "OPERA – STATUS OF THE EXPERIMENT." In Proceedings of the 33rd International Conference. World Scientific Publishing Company, 2007. http://dx.doi.org/10.1142/9789812790873_0051.

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Russo, A., S. K. Singh, J. G. Morfin, Makoto Sakuda, and K. D. Purohit. "Status of the OPERA experiment." In NuInt11. AIP, 2011. http://dx.doi.org/10.1063/1.3661598.

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Capua, Francesco Di. "Status of the OPERA experiment." In International Europhysics Conference on High Energy Physics. Trieste, Italy: Sissa Medialab, 2007. http://dx.doi.org/10.22323/1.021.0177.

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Russo, Andrea. "Status of the OPERA experiment." In The XIXth International Workshop on High Energy Physics and Quantum Field Theory. Trieste, Italy: Sissa Medialab, 2011. http://dx.doi.org/10.22323/1.104.0081.

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PESSARD, Henri. "Status of the OPERA neutrino experiment." In European Physical Society Europhysics Conference on High Energy Physics. Trieste, Italy: Sissa Medialab, 2010. http://dx.doi.org/10.22323/1.084.0280.

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Gornushkin, Yuri. "More results from the OPERA Experiment." In 38th International Conference on High Energy Physics. Trieste, Italy: Sissa Medialab, 2017. http://dx.doi.org/10.22323/1.282.0952.

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Galati, Giuliana. "Neutrino oscillations with the OPERA experiment." In Neutrino Oscillation Workshop. Trieste, Italy: Sissa Medialab, 2017. http://dx.doi.org/10.22323/1.283.0010.

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PUPILLI, F. "RECENT RESULTS OF THE OPERA EXPERIMENT." In International Conference on Advanced Technology and Particle Physics. WORLD SCIENTIFIC, 2014. http://dx.doi.org/10.1142/9789814603164_0044.

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Gornushkin, Yury. "REVIEW OF THE OPERA EXPERIMENT RESULTS." In Nineteenth Lomonosov Conference on Elementary Particle Physics. WORLD SCIENTIFIC, 2021. http://dx.doi.org/10.1142/9789811233913_0005.

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Reports on the topic "OPERA Experiment"

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McIntyre, Phillip, Susan Kerrigan, and Marion McCutcheon. Australian Cultural and Creative Activity: A Population and Hotspot Analysis: Coffs Harbour. Queensland University of Technology, 2021. http://dx.doi.org/10.5204/rep.eprints.208028.

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Coffs Harbour on the north coast of NSW is a highway city sandwiched between the Great Dividing Range and the Pacific Ocean. For thousands of years it was the traditional land of the numerous Gumbaynggirr peoples. Tourism now appears to be the major industry, supplanting agriculture and timber getting, while a large service sector has grown up around a sizable retirement community. It is major holiday destination. Located further away from the coast in the midst of a dairy farming community, Bellingen has become a centre of alternative culture which relies heavily on a variety of festivals activated by energetic tree changers and numerous professionals who have relocated from Sydney. Both communities rely on the visitor economy and there have been considerable changes to how local government in this region approach strategic planning for arts and culture. The newly built Coffs Harbour Education Campus (CHEC) is an experiment in encouraging cross pollination between innovative businesses and education and incorporates TAFE NSW, Coffs Harbour Senior College and Southern Cross University as well as the Coffs Harbour Technology Park and Coffs Harbour Innovation Centre all on one site. The 250 seat Jetty Memorial Theatre is the main theatre in Coffs Harbour for local and touring productions while local halls and converted theatres are the mainstay of smaller communities in the region. As peak body Arts Mid North Coast reports, there is a good record of successful arts related events which range across all genres of music, art, sculpture, Aboriginal culture, street art, literature and even busking and opera. These are mainly managed by passionate local volunteers.
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