Готові списки джерел за темами / Flavour oscillations

Добірка наукової літератури з теми "Flavour oscillations"

Автор: Grafiati
Опубліковано: 11 березня 2023

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Статті в журналах з теми "Flavour oscillations"

1

Schubert, Klaus R. "Flavour oscillations." Progress in Particle and Nuclear Physics 21 (January 1988): 3–31. http://dx.doi.org/10.1016/0146-6410(88)90030-0.

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2

Pal, B. K. "Flavour mixing neutrino oscillations." Il Nuovo Cimento A 103, no. 8 (August 1990): 1113–20. http://dx.doi.org/10.1007/bf02820538.

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3

Filip, Peter. "Flavour Oscillations in Dense Baryonic Matter." Journal of Physics: Conference Series 779 (January 2017): 012047. http://dx.doi.org/10.1088/1742-6596/779/1/012047.

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4

Mangano, Gianpiero, Gennaro Miele, Sergio Pastor, Teguayco Pinto, Ofelia Pisanti, and Pasquale D. Serpico. "Relic neutrino decoupling including flavour oscillations." Nuclear Physics B 729, no. 1-2 (November 2005): 221–34. http://dx.doi.org/10.1016/j.nuclphysb.2005.09.041.

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5

de Salas, Pablo F., and Sergio Pastor. "Relic neutrino decoupling with flavour oscillations revisited." Journal of Cosmology and Astroparticle Physics 2016, no. 07 (July 28, 2016): 051. http://dx.doi.org/10.1088/1475-7516/2016/07/051.

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6

Osland, P., and G. Vigdel. "Solar-neutrino oscillations and third-flavour admixture." Physics Letters B 438, no. 1-2 (October 1998): 129–35. http://dx.doi.org/10.1016/s0370-2693(98)00973-3.

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7

Neubert, Matthias. "Nonleptonic weak decays, flavour oscillations, and diquarks." Nuclear Physics B - Proceedings Supplements 21 (June 1991): 351–58. http://dx.doi.org/10.1016/0920-5632(91)90276-k.

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8

Gluza, J., and M. Zrałek. "Parameters' domain in three flavour neutrino oscillations." Physics Letters B 517, no. 1-2 (September 2001): 158–66. http://dx.doi.org/10.1016/s0370-2693(01)00962-5.

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9

Abdullaeva, Umsalimat, Vadim Shakhov, Alexander Studenikin, and Alexander Tsvirov. "Dirac and Majorana neutrino oscillations in magnetized moving and polarized matter." Journal of Physics: Conference Series 2156, no. 1 (December 1, 2021): 012229. http://dx.doi.org/10.1088/1742-6596/2156/1/012229.

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Анотація:
Abstract In the present paper we develop the quantum theory of neutrino spin and spin-flavour oscillations in moving magnetized matter with a special focus on the effects of matter polarization. We derive an effective neutrino evolution Hamiltonian and corresponding expressions for the neutrino oscillation probabilities. Both the case of Dirac and Majorana neutrinos are considered. From the comparison of the neutrino spin oscillation probabilities in the transversally moving matter for the Dirac and Majorana neutrinos it follows that the oscillation patterns is different for theses two cases. In particular, the conditions for the resonances in these two cases are realized at different densities of matter.
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10

Boriero, Daniel, Dominik J. Schwarz, and Hermano Velten. "Flavour Composition and Entropy Increase of Cosmological Neutrinos After Decoherence." Universe 5, no. 10 (September 25, 2019): 203. http://dx.doi.org/10.3390/universe5100203.

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Анотація:
We propose that gravitational interactions of cosmic neutrinos with the statistically homogeneous and isotropic fluctuations of space-time lead to decoherence. This working hypothesis, which we describe by means of a Lindblad operator, is applied to the system of two- and three-flavour neutrinos undergoing vacuum oscillations and the consequences are investigated. As a result of this decoherence we find that the neutrino entropy would increase as a function of initial spectral distortions, mixing angles and charge-parity (CP)-violation phase. Subsequently we discuss the chances to discover such an increase observationally (in principle). We also present the expected flavour composition of the cosmic neutrino background after decoherence is completed. The physics of two- or three-flavour oscillation of cosmological neutrinos resembles in many aspects two- or three-level systems in atomic clocks, which were recently proposed by Weinberg for the study of decoherence phenomena.
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Дисертації з теми "Flavour oscillations"

1

Donadi, Sandro. "Electromagnetic Radiation Emission and Flavour Oscillations in Collapse Models." Doctoral thesis, Università degli studi di Trieste, 2014. http://hdl.handle.net/10077/9961.

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2012/2013
In order to solve the measurement problem, collapse models modify the Schroedinger dynamics by adding non linear and stochastic terms. Collapse models provide different predictions compare to Quantum mechanics. In this thesis we focus on two phenomena where the predictions of quantum mechanics and collapse models are different: the electromagnetic radiation emission from charged systems and the flavour oscillations. We analysed both of them and obtained the quantitative deviations from standard quantum behaviour.
Al fine di risolvere il problema della misura, i modelli di collasso spontaneo della funzione d'onda modificano la dinamica data dall'equazione di Schroedinger aggiungendo termini non lineari e stocastici. I modelli di collasso forniscono previsioni differenti rispetto alla meccanica quantistica. In questa tesi studieremo due fenomeni dove le predizioni della meccanica quantistica e dei modelli di collasso sono diverse: l'emissione di radiazione elettromagnetica da sistemi elettricamente non neutri e le oscillazioni dei sapori. Analizzeremo entrambi i fenomeni al fine di ottenere deviazioni quantitative dal comportamento quantistico standard.
XXVI Ciclo
1985
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2

Elevant, Jessica. "CP-violation in Supernova Neutrino Oscillations." Thesis, Linköpings universitet, Teoretisk Fysik, 2014. http://urn.kb.se/resolve?urn=urn:nbn:se:liu:diva-109922.

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Анотація:
It is astonishing both how little and how much we know about neutrinos. On one hand, the neutrino is the second most abundant particle in our Universe. Neutrinos may be created in the Sun, core collapse supernovae, cosmic rays, geological background radiation, supernova remnants and in the Big Bang. On the other hand, they have unimaginably small masses and are unwilling to react with their surroundings. Because of their abundance and their inclination to show us physics beyond the standard model of particle physics, neutrinos are hoped to carry yet unknown information of the Universe. However, it will take some effort and time to persuade the neutrinos to tell us what they know. Among the things we do not yet know of the neutrinos, is the -phase in the neutrino mixing matrix. If is in fact non-zero, neutrino flavour oscillations violate CP-symmetry. Also, if neutrino masses are introduced in the standard model through the See-Saw mechanism and if leptogenesis is a valid theory, CP-violation in neutrino oscillations could help explain why our Universe has no antimatter even though equal amounts of matter and antimatter should have been created at the Big Bang. In this thesis, we investigate the flavour evolution of supernova neutrinos. We present the full Hamiltonian in the flavour basis for our system and identify how the different contributions affect the evolution and in which environment. We also present a theoretical motivation from [1, 2] as to how a non-zero -phase affects the flavour evolution and the final energy spectra. The analytical conclusion is that it has no impact under the assumptions made in our analysis. Thus, the -phase may not be measurable from supernova neutrinos.
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3

Bourret, Simon. "Neutrino oscillations and earth tomography with KM3NeT-ORCA." Thesis, Sorbonne Paris Cité, 2018. http://www.theses.fr/2018USPCC247.

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Анотація:
Les oscillations de saveur des neutrinos, découvertes au tournant du 21ème siècle, constituent à ce jour le signe le plus direct de physique au-delà du Modèle Standard. La collaboration KM3NeT a commencé la construction d'un détecteur à effet Tcherenkov de neutrinos au fond de la mer Méditerranée: ORCA (Oscillation Research with Cosmics in the Abyss). Le but principal d'ORCA sera la détermination de la hiérarchie de masse des neutrinos, un paramètre fondamental, encore inconnu, du modèle théorique des oscillations de neutrinos. Le principe de la mesure est la détection d'un large échantillon de neutrinos atmosphériques ayant traversé la Terre, et l'analyse de leurs oscillations de saveur. Ces oscillations sont modifiées et augmentées par les effets de matière, dus à la présence d'une densité d'électrons le long de la trajectoire des neutrinos. Au-delà de la hiérarchie de masse et de la mesure des paramètres d'oscillation atmosphériques, ORCA sera alors capable de mesurer la densité en électrons et donc, en principe, de fournir des informations nouvelles sur la composition chimique des couches profondes de la Terre. Cette thèse présente une nouvelle étude, menée au sein de la collaboration KM3NeT, de la sensibilité d'ORCA à la détermination de la hiérarchie de masse des neutrinos, aux paramètres d'oscillations atmosphériques, et à la densité en électrons dans le noyau externe et le manteau inférieur de la Terre. La thèse se concentre sur le développement d'une nouvelle méthode d'analyse dont le but est de rendre compte de la réponse du détecteur de la manière la plus précise possible. Pour cela, la méthode est basée sur l'utilisation de matrices de réponses corrélées et construites à partir de simulations Monte Carlo. Les méthodes statistiques et sources d'incertitude systématique sont aussi étudiées en détail. La méthode développée permet une première exploration de nouvelles stratégies d'analyse optimisées. Les études de sensibilité montrent qu'ORCA atteindra une sensibilité médiane à la hiérarchie de masse d'au moins 3 sigma après quelques années d'opération, le résultat dépendant en grande partie de la valeur réelle de la hiérarchie de masse et des autres paramètres d'oscillation encore inconnus. Une performance compétitive pour la mesure des paramètres d'oscillation atmosphériques est aussi attendue. Dans le cas où la hiérarchie de masse est normale et après 10 ans de prise de données, la densité en électrons pourra être mesurée avec une précision d'environ 5% dans le manteau inférieur, et 7% dans le noyau externe
Neutrino flavour oscillations, discovered at the turn of the 21st century, currently provide the most direct window on physics beyond the Standard Model. The KM3NeT collaboration has started the construction of a megaton-scale Cherenkov neutrino detector deep underwater in the Mediterranean: ORCA (Oscillation Research with Cosmics in the Abyss). ORCA's main goal will be the determination of the neutrino mass hierarchy, a major unknown in the current understanding of neutrino oscillations, via the detection of large samples of atmospheric neutrinos crossing the Earth and the analysis of their flavour oscillations. These oscillations are enhanced by matter effects, sensitive to the electron density along the neutrino paths. Beyond the neutrino mass hierarchy and the measurement of atmospheric oscillation parameters, this will allow ORCA to measure the electron density of the deep Earth, and possibly provide constraints on the chemical composition of its innermost layers. This thesis presents a new study, undertaken within the KM3NeT collaboration, of the sensitivity of ORCA to the determination of the neutrino mass hierarchy, oscillation parameters, and the electron density in the outer core and lower mantle of the Earth. The focus is given to the development of a new analysis methodology intended to account for detector effects as precisely as possible by the use of a Monte Carlo based correlated model of detector response. Statistical methods and systematic uncertainties are also addressed in some detail. The methodology allows for a preliminary exploration of the potential of improved analysis strategies. Sensitivity studies show that ORCA is expected to achieve a median sensitivity to the NMH determination at the level of 3 sigma or better after a few years of operation, depending on the true hierarchy and true value of the oscillation parameters. Competitive performance for the measurement of atmospheric oscillation parameters is also expected. Assuming a normal mass hierarchy, the electron density can be measured with a precision of about 5% in the lower mantle, and 7% in the outer core
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4

Huber, Patrick. "Three flavour effects in future neutrino oscillation experiments." [S.l. : s.n.], 2003. http://deposit.ddb.de/cgi-bin/dokserv?idn=969864272.

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5

Keil, Mathias Thorsten. "Supernova neutrino spectra and applications to flavor oscillations." [S.l. : s.n.], 2003. http://deposit.ddb.de/cgi-bin/dokserv?idn=969382340.

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6

Leonardo, Nuno Teotónio Viegas Guerreiro. "Analysis of B [sigma] flavor oscillations at CDF." Thesis, Massachusetts Institute of Technology, 2006. http://hdl.handle.net/1721.1/39293.

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Анотація:
Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, February 2007.
In title on t.p., "[sigma]" appears as the lower-case Greek letter.
Includes bibliographical references (p. 367-376).
The search for and the study of flavor oscillations in the neutral B,B, meson system is an experimentally challenging endeavor. This constitutes a flagship analysis of the Tevatron proton-antiproton collider physics program. In this dissertation we develop such an analysis of the time-dependent B, flavor oscillations using data collected with the CDF detector. The data samples are formed of both fully and partially reconstructed B meson decays, B, -+ D7r(irir) and B8 -- Dalv. A likelihood fitting framework is implemented and appropriate models and techniques developed for describing the mass, proper decay time, and flavor tagging characteristics of the data samples. The analysis is extended to samples of B+ and Bo mesons, which are further used for algorithm calibration and method validation. The B mesons lifetimes are extracted. The measurement of the Bo oscillation frequency yields Amd = 0.522 ± 0.017 ps-1. The search for B, oscillations is performed using an amplitude method based on a frequency scanning procedure. Applying a combination of lepton and jet charge flavor tagging algorithms, with a total tagging power ED2 of 1.6%, to a data sample of 355 pb-1, a sensitivity of 13.0 ps-1 is achieved.
(cont.) In a preliminary study, we develop a same side kaon tagging algorithm, which is found to provide a superior tagging power, of about 4.0% for the B, meson species. An evaluation of the dilution systematic uncertainties is not reported but after including the algorithm as is in the analysis the sensistivity is significantly increased to about 18 ps-'. An indication of a B, oscillation signal is seen at a frequency of about 17.5 ps-1. We show that the extension of the analysis to the increasing data samples with the inclusion of the same side tagging algorithm is capable of providing an observation of B, mixing beyond the standard model expectation. We show also that the improved knowledge of Am, has a considerable impact on constraining the CKM matrix elements.
by Nuno Teotónio Viegas Guerreiro Leonardo.
Ph.D.
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7

Ballett, Peter Alexander. "Probing leptonic flavour with future long-baseline neutrino oscillation experiments." Thesis, Durham University, 2013. http://etheses.dur.ac.uk/7745/.

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Over the last 50 years, the study of the properties of neutrinos has unveiled a number of surprising facts that necessitate physics beyond the standard model. We now know that neutrinos are not only massive, but that there is a non-trivial alignment between the mass and flavour bases, inducing flavour changing transitions known as neutrino oscillations. Understanding the neutrino sector is a crucial first step in our attempts to extend our current theories of fundamental physics, and studies of neutrino oscillation provide us with a unique tool to probe these elusive particles. In this thesis, we assess the potential of the next generation of neutrino oscillation experiments to probe physical effects both within and beyond the current neutrino flavour paradigm: resolving existing unknowns, and constraining the correlations induced by theories of leptonic flavour.
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8

Mack, Philipp. "Kalibration neuer 'Flavor Tagging' Algorithmen mittels Bs-Oszillationen Calibration of new flavor tagging algorithms using Bs oscillations /." [S.l. : s.n.], 2007. http://digbib.ubka.uni-karlsruhe.de/volltexte/1000007124.

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9

Wendell, Roger Alexandre Scholberg Kate. "Three flavor oscillation analysis of atmospheric neutrinos in super-kamiokande." Chapel Hill, N.C. : University of North Carolina at Chapel Hill, 2008. http://dc.lib.unc.edu/u?/etd,1965.

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Анотація:
Thesis (Ph. D.)--University of North Carolina at Chapel Hill, 2008.
Title from electronic title page (viewed Dec. 11, 2008). "... in partial fulfillment of the requirements for the degree of Doctor of Philosophy in the Department of Physics and Astronomy." Discipline: Physics and Astronomy; Department/School: Physics and Astronomy.
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10

Calland, Richard. "A 3 flavour joint near and far detector neutrino oscillation analysis at T2K." Thesis, University of Liverpool, 2014. http://livrepository.liverpool.ac.uk/2009123/.

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The Tokai-to-Kamioka (T2K) experiment is a second generation long-baseline neutrino experiment and the first to use an off-axis neutrino beam to produce narrow neutrino energy spectrum. T2K was designed to measure with precision the atmospheric mixing parameters, and also look for evidence of non-zero θ13. T2K's near detector (ND280) provides constraints on the beam flux and neutrino cross-section uncertainties, as well as making valuable cross-section measurements. This thesis describes an oscillation analysis that uses samples from both near and far detectors. Importantly, vμ and Ve samples at the far detector are combined to produce a joint oscillation analysis. A Markov chain Monte Carlo is used to construct the Bayesian posterior distribution by sampling a likelihood function. From the Bayesian posterior distribution, the oscillation parameters of interest and their errors are estimated.
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Книги з теми "Flavour oscillations"

1

Fritzsch, Harald. Massive neutrinos: Flavor mixing of leptons and neutrino oscillations. Singapore: World Scientific, 2015.

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2

Franke, Arthur. Searching for Reactor Antineutrino Flavor Oscillations with the Double Chooz Far Detector. [New York, N.Y.?]: [publisher not identified], 2012.

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3

Kikawa, Tatsuya. Measurement of Neutrino Interactions and Three Flavor Neutrino Oscillations in the T2K Experiment. Singapore: Springer Singapore, 2016. http://dx.doi.org/10.1007/978-981-287-715-4.

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4

Kikawa, Tatsuya. Measurement of Neutrino Interactions and Three Flavor Neutrino Oscillations in the T2K Experiment. Springer, 2015.

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5

Kikawa, Tatsuya. Measurement of Neutrino Interactions and Three Flavor Neutrino Oscillations in the T2K Experiment. Springer, 2015.

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6

Kikawa, Tatsuya. Measurement of Neutrino Interactions and Three Flavor Neutrino Oscillations in the T2K Experiment. Springer, 2016.

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7

Kikawa, Tatsuya. Measurement of Neutrino Interactions and Three Flavor Neutrino Oscillations in the T2K Experiment. Springer, 2015.

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8

Vigdor, Steven E. Where’s the Antimatter Gone, Long Time Passing? Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198814825.003.0002.

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Chapter 2 describes experiments searching for CP symmetry violations that might account for the matter–antimatter imbalance in our universe. It describes the historical discovery of mesons and quantum-mechanical oscillations between particle and antiparticle (i.e., particle–antiparticle oscillations) in the neutral K meson and heavier meson systems. It introduces quarks and quark flavor. The chapter relates CP violation to violations of time reversal invariance that might be revealed by a spatial separation of positive and negative electric charge within or around the fundamental constituent particles of matter. It describes a halfcentury of experimental searches, including ongoing projects, for the particle electric dipole moments that would characterize such a charge separation. Technological advances (such as ultra-cold neutron beams) and theoretical concepts (such as vacuum polarization) relevant to these searches are introduced. While some CP violation has been clearly observed, its extent remains insufficient to account for the universe’s matter–antimatter imbalance.
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9

Vigdor, Steven E. Trinity. Oxford University Press, 2018. http://dx.doi.org/10.1093/oso/9780198814825.003.0003.

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Chapter 3 explains evidence for three generations of quarks and leptons, as needed to provide natural means for standard model CP violation. It describes the cross-generational mixing of quarks and of neutrinos of different flavor, and the matrices that characterize the mixing. CP violation from quark mixing is well measured but insufficient to explain the universe’s matter–antimatter imbalance, while CP violation in neutrino mixing is the subject of ongoing searches. Discoveries revealing and quantifying flavor oscillations among neutrinos from the sun and the atmosphere are reviewed. In describing attempts to understand the lightness and nature of neutrinos—whether they are Majorana neutrinos that are their own antiparticles—the chapter introduces the concept of chirality and searches for neutrinoless double beta decay. It also notes the strong CP problem, wherein nature maintains CP symmetry in interactions among the three quark colors even though quantum chromodynamics allows for sizable violations.
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10

(Editor), Yoshitaka Kuno, William R. Molzon (Editor), and Sandip Pakvasa (Editor), eds. New Initiatives on Lepton Flavor Violation and Neutrino Oscillation With High Intensity Muon and Neutrino Sources. World Scientific Publishing Company, 2003.

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Частини книг з теми "Flavour oscillations"

1

Kuhr, Thomas. "Flavor Oscillations." In Springer Tracts in Modern Physics, 77–99. Berlin, Heidelberg: Springer Berlin Heidelberg, 2012. http://dx.doi.org/10.1007/978-3-642-10300-1_6.

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2

Shafaq, Sheeba, and Poonam Mehta. "Impact of Non-standard Interactions on Violation of Leggett-Garg Inequality in Three-Flavour Neutrino Oscillations." In Springer Proceedings in Physics, 617–20. Singapore: Springer Nature Singapore, 2022. http://dx.doi.org/10.1007/978-981-19-2354-8_112.

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3

Suekane, Fumihiko. "Neutrino Oscillation: Relativistic Oscillation of Three-Flavor System." In Quantum Oscillations, 145–60. Cham: Springer International Publishing, 2021. http://dx.doi.org/10.1007/978-3-030-70527-5_12.

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4

Horwitz, Lawrence P. "Gauge Fields and Flavor Oscillations." In Fundamental Theories of Physics, 51–69. Dordrecht: Springer Netherlands, 2015. http://dx.doi.org/10.1007/978-94-017-7261-7_4.

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5

Waldi, Roland. "Flavour Oscillation and CP Violation of B Mesons." In CP Violation in Particle, Nuclear and Astrophysics, 43–195. Berlin, Heidelberg: Springer Berlin Heidelberg, 2002. http://dx.doi.org/10.1007/3-540-47895-7_4.

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6

Kikawa, Tatsuya. "Measurement of Neutrino Oscillations." In Measurement of Neutrino Interactions and Three Flavor Neutrino Oscillations in the T2K Experiment, 155–91. Singapore: Springer Singapore, 2015. http://dx.doi.org/10.1007/978-981-287-715-4_10.

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7

Waldi, Roland. "Flavour Oscillation and CP Violation: Experimental Results on B Mesons." In Particle Physics in the New Millennium, 244–64. Berlin, Heidelberg: Springer Berlin Heidelberg, 2003. http://dx.doi.org/10.1007/3-540-36539-7_18.

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8

Kikawa, Tatsuya. "Introduction to Neutrino Physics." In Measurement of Neutrino Interactions and Three Flavor Neutrino Oscillations in the T2K Experiment, 1–22. Singapore: Springer Singapore, 2015. http://dx.doi.org/10.1007/978-981-287-715-4_1.

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9

Kikawa, Tatsuya. "Conclusions." In Measurement of Neutrino Interactions and Three Flavor Neutrino Oscillations in the T2K Experiment, 193–95. Singapore: Springer Singapore, 2015. http://dx.doi.org/10.1007/978-981-287-715-4_11.

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10

Kikawa, Tatsuya. "T2K Experiment." In Measurement of Neutrino Interactions and Three Flavor Neutrino Oscillations in the T2K Experiment, 23–35. Singapore: Springer Singapore, 2015. http://dx.doi.org/10.1007/978-981-287-715-4_2.

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Тези доповідей конференцій з теми "Flavour oscillations"

1

ENNADIFI, SALAH EDDINE. "On Neutrino Oscillations and Flavour Persistence." In Unified Field Mechanics II: Preliminary Formulations and Empirical Tests, 10th International Symposium Honouring Mathematical Physicist Jean-Pierre Vigier. WORLD SCIENTIFIC, 2017. http://dx.doi.org/10.1142/9789813232044_0042.

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2

Lichkunov, Alexey, Konstantin Stankevich, Alexander Studenikin, and Maxim Vyalkov. "Neutrino decay processes and flavour oscillations." In The European Physical Society Conference on High Energy Physics. Trieste, Italy: Sissa Medialab, 2022. http://dx.doi.org/10.22323/1.398.0202.

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3

Grigoriev, A., A. Lobanov, and A. Studenikin. "EFFECT OF MATTER MOTION AND POLARIZATION IN NEUTRINO FLAVOUR OSCILLATIONS." In Proceedings of the Tenth Lomonosov Conference on Elementary Particle Physics. WORLD SCIENTIFIC, 2003. http://dx.doi.org/10.1142/9789812704948_0004.

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4

Vecchi, Stefania. "Flavour tagging at LHCb and measurements of B meson oscillations." In 36th International Conference on High Energy Physics. Trieste, Italy: Sissa Medialab, 2013. http://dx.doi.org/10.22323/1.174.0365.

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5

Akhmedov, E. Kh. "Three-Flavour Effects and CP- and T-Violation in Neutrino Oscillations." In Proceedings of Nobel Symposium 129. WORLD SCIENTIFIC, 2006. http://dx.doi.org/10.1142/9789812773906_0009.

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6

Popov, Artem, Alexey Lichkunov, and Alexander Studenikin. "Interplay of neutrino spin and three-flavour oscillations in a magnetic field." In The European Physical Society Conference on High Energy Physics. Trieste, Italy: Sissa Medialab, 2022. http://dx.doi.org/10.22323/1.398.0197.

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7

De Cecco, Sandro. "Search for B[sub s][sup 0] Flavour Oscillations with the CDF Experiment." In IFAE 2005: XVII Incontri de Fisica delle Alte Energie; 17th Italian Meeting on High Energy Physics. AIP, 2005. http://dx.doi.org/10.1063/1.2125651.

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8

Titov, Arsenii, Ivan Girardi, and Serguey Petcov. "CPV Predictions from Flavour Symmetries." In Neutrino Oscillation Workshop. Trieste, Italy: Sissa Medialab, 2017. http://dx.doi.org/10.22323/1.283.0027.

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9

Carceller, Juan Miguel. "3-flavour results with NOvA." In Neutrino Oscillation Workshop. Trieste, Italy: Sissa Medialab, 2023. http://dx.doi.org/10.22323/1.421.0015.

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10

Romanino, Andrea, and Yakefu Reyimuaji. "Unbroken flavour symmetries vs lepton masses and mixings." In Neutrino Oscillation Workshop. Trieste, Italy: Sissa Medialab, 2019. http://dx.doi.org/10.22323/1.337.0074.

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Звіти організацій з теми "Flavour oscillations"

1

Morlock, Jan. Flavour Tagging Calibration and Measurement of Bs Oscillations and CP Asymmetry. Office of Scientific and Technical Information (OSTI), June 2010. http://dx.doi.org/10.2172/1342791.

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2

Beale, Steven Thomas. Flavour oscillations and CP asymmetry in semileptonic Bs0 decays. Office of Scientific and Technical Information (OSTI), January 2010. http://dx.doi.org/10.2172/975165.

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3

Carroll III, Thomas Joseph. Three-Flavor Neutrino Oscillations with MINOS+. Office of Scientific and Technical Information (OSTI), January 2019. http://dx.doi.org/10.2172/1576527.

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4

Guerreiro Leonardo, Nuno Teotonio Viegas. Analysis of Bs flavor oscillations at CDF. Office of Scientific and Technical Information (OSTI), September 2006. http://dx.doi.org/10.2172/892478.

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5

Davoudiasl, H., H.-S. Lee, and W. Marciano. Long-Range Lepton Flavor Interactions and Neutrino Oscillations. Office of Scientific and Technical Information (OSTI), March 2011. http://dx.doi.org/10.2172/1017401.

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6

Martin, Joshua. Nonlinear, Multidimensional, and Beyond Mean-Field Coherent Neutrino Flavor Oscillations. Office of Scientific and Technical Information (OSTI), August 2022. http://dx.doi.org/10.2172/1880466.

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7

MacFarlane, David B. Measurement of B0-anti-B0 Flavor Oscillations in Hadronic B0 Decays. Office of Scientific and Technical Information (OSTI), January 2002. http://dx.doi.org/10.2172/798947.

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8

Mack, Philipp. Calibration of new flavor tagging algorithms using Bs oscillations. Office of Scientific and Technical Information (OSTI), July 2007. http://dx.doi.org/10.2172/920111.

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9

Belloni, Alberto. Observation of Bs0 - anti-Bs0 Oscillations and the Development and Application of Same-Side-Kaon Flavor Tagging. Office of Scientific and Technical Information (OSTI), July 2007. http://dx.doi.org/10.2172/1415817.

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10

MacFarlane, David B. A Study of Time-Dependent CP-Violating Asymmetries and Flavor Oscillations in Neutral B Decays at the Upsilon(4S). Office of Scientific and Technical Information (OSTI), January 2002. http://dx.doi.org/10.2172/798946.

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