Relevant bibliographies by topics / Taux de neutrinos

Contents

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

Academic literature on the topic 'Taux de neutrinos'

Author: Grafiati
Published: 25 January 2025
Last updated: 31 July 2025

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Journal articles on the topic "Taux de neutrinos"

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JONES, J., I. MOCIOIU, I. SARCEVIC, and M. H. RENO. "ULTRAHIGH ENERGY TAU NEUTRINOS." International Journal of Modern Physics A 20, no. 19 (2005): 4656–63. http://dx.doi.org/10.1142/s0217751x0502834x.

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We study ultrahigh energy astrophysical neutrinos and the contribution of tau neutrinos from neutrino oscillations, relative to the contribution of the other flavors. We show the effect of tau neutrino regeneration and tau energy loss as they propagate through the Earth. We consider a variety of neutrino fluxes, such as cosmogenic neutrinos and neutrinos that originate in Active Galactic Nuclei. We discuss signals of tau neutrinos in detectors such as IceCube, RICE and ANITA.
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JONES, J., I. MOCIOIU, I. SARCEVIC, and M. H. RENO. "TRACING VERY HIGH ENERGY TAU NEUTRINOS FROM COSMOLOGICAL SOURCES IN ICE." International Journal of Modern Physics A 20, no. 06 (2005): 1204–11. http://dx.doi.org/10.1142/s0217751x05024092.

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Astrophysical sources of ultrahigh energy neutrinos yield tau neutrino fluxes due to neutrino oscillations. We study in detail the contribution of tau neutrinos with energies above 106 GeV relative to the contribution of the other flavors. We consider several different initial neutrino fluxes and include tau neutrino regeneration in transit through the Earth and energy loss of charged leptons. We discuss signals of tau neutrinos in detectors such as IceCube, RICE and ANITA.
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Wissel, Stephanie, Jaime Alvarez-Muñiz, Washington R. Carvalho, Andrés Romero-Wolf, Harm Schoorlemmer, and Enrique Zas. "A New Concept for High-Elevation Radio Detection of Tau Neutrinos." EPJ Web of Conferences 216 (2019): 04007. http://dx.doi.org/10.1051/epjconf/201921604007.

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Cosmic neutrinos are expected to include a significant flux of tau neutrinos due to flavor mixing over astronomical length scales. However, the tau-neutrino content of astrophysical neutrinos is poorly constrained and a significant flux of cosmogenic tau neutrinos awaits discovery. Earth-skimming tau neutrinos undergo charged-current interactions that result in a tau lepton exiting the Earth. The tau lepton decay generates anextensive air shower and geomagnetic radio emission. To target the tau neutrinos, we present a new tau neutrino detector concept that uses phased antenna arrays placed on
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ATHAR, H. "ATMOSPHERIC AND GALACTIC TAU NEUTRINOS." Modern Physics Letters A 19, no. 13n16 (2004): 1171–78. http://dx.doi.org/10.1142/s0217732304014525.

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Neutrinos with energy greater than GeV are copiously produced in the p(A,p) interactions occurring in the earth atmosphere and in our galactic plane. A comparison of the tau and mu neutrino flux in the presence of neutrino oscillations from these two astrophysical sites is presented. It is pointed out that the galactic plane tau neutrino flux dominates over the downward going atmospheric tau neutrino flux at much lower energy value than that for the dominance of the mu neutrino flux from these two sites. Future prospects for possible observations of galactic tau neutrino flux are also briefly
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Miloi, Mădălina Mihaela. "The DsTau Experiment: A Study for Tau-Neutrino Production." Particles 3, no. 1 (2020): 164–68. http://dx.doi.org/10.3390/particles3010013.

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For clarifying the validity of the Lepton Universality hypothesis, one of the fundamental statements of the Standard Model, the interaction cross section for all three flavors of leptons have to be known with high precision. In neutrino sector, for electron and muon neutrinos, the interaction cross section is known fairly well, but for tau neutrino only poor estimations exist. In particular, the most direct measurement by the DONuT experiment was performed with rather poor accuracy due to low statistics and an uncertainty of the tau neutrino flux. The DsTau experiment proposes to study tau-neu
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Kato, Tokufumi. "Tau Neutrino Appearance in Atmospheric Neutrinos." Nuclear Physics B - Proceedings Supplements 221 (December 2011): 356. http://dx.doi.org/10.1016/j.nuclphysbps.2011.10.006.

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De Lellis, Giovanni, Sergey Dmitrievsky, Giuliana Galati, et al. "Dataset of tau neutrino interactions recorded by the OPERA experiment." EPJ Web of Conferences 245 (2020): 08013. http://dx.doi.org/10.1051/epjconf/202024508013.

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We describe the dataset of very rare events recorded by the OPERA experiment. The events represent tracks of particles associated with tau neutrino interactions coming from the transformation of muon neutrinos due to a process known as neutrino oscillations. The events have been published on the CERN Open Data Portal. We describe the dataset semantics and the interactive event display visualisation tool accompanying the data release.
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GNINENKO, S. N. "ON MIXING ANGLES AND MAGNETIC MOMENT OF HEAVY TAU NEUTRINO." Modern Physics Letters A 13, no. 22 (1998): 1791–94. http://dx.doi.org/10.1142/s0217732398001868.

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If the magnetic moment of unstable tau neutrinos with the mass of 0(MeV) is in the region of 10-8μB≲ μντ≲ 10-6μB, it is compatible with the present experimental and cosmological bounds. We point out that if the tau neutrino has such a large magnetic moment and can oscillate into a neutrino of another flavor, the results from νe scattering experiment at LAMPF constrain the tau neutrino mixing angles to sin 2 2θeτ≲ 2 × 10-6-2 × 10-2 and sin 2 2θμτ ≲ 10-6-10-2 depending on the magnetic moment value in the allowed region.
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LIU, CHUN. "CONFRONTING HEAVY TAU NEUTRINOS WITH NEUTRINO OSCILLATIONS." Modern Physics Letters A 16, no. 26 (2001): 1699–702. http://dx.doi.org/10.1142/s0217732301005023.

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If the tau neutrino is as heavy as 10 MeV which may have certain astrophysical implications, the neutrino mass pattern is studied so as to accommodate the new oscillation observations. It predicts that the electron neutrino has Marjorana mass around 0.05 eV. A supersymmetric model is described to realize the above scenario.
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Fukuda, S., Y. Fukuda, M. Ishitsuka, et al. "Tau Neutrinos Favored over Sterile Neutrinos in Atmospheric Muon Neutrino Oscillations." Physical Review Letters 85, no. 19 (2000): 3999–4003. http://dx.doi.org/10.1103/physrevlett.85.3999.

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Dissertations / Theses on the topic "Taux de neutrinos"

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Beau, Tristan. "Mesure des neutrinos solaires de la raie du béryllium dans l'expérience Borexino." Phd thesis, Université Paris-Diderot - Paris VII, 2002. http://tel.archives-ouvertes.fr/tel-00002065.

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L'expérience Borexino (BX), collaboration impliquant neuf pays, est implantée dans le laboratoire souterrain du Gran Sasso en Italie. Elle vise la mesure du flux de neutrinos solaires de la raie du béryllium à 862 keV, première mesure en temps réel à si basse énergie. Cette expérience impose des contraintes très fortes en radiopureté. Sa faisabilité technique est testée dans le prototype Counting Test Facility (CTF).<br> Le groupe du Collège de France est chargé du système de numérisation rapide (FADC) sur BX. Ces FADC ont été conçus au laboratoire et nous les avons finalisés début 2002. Les c
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Monzani, Maria Elena. "Characterization and calibration of the Borexino detector for solar and supernova neutrinos." Paris 7, 2005. http://www.theses.fr/2005PA077112.

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Onillon, Anthony. "Prédiction des taux de fission des coeurs de Chooz et estimation des incertitudes associées dans le cadre de l'expérience Double Chooz." Thesis, Nantes, Ecole des Mines, 2014. http://www.theses.fr/2014EMNA0116/document.

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Double Chooz est une expérience dédiée à la mesure de l'angle de mélange θ₁₃ caractérisant le phénomène d’oscillation des neutrinos. Elle consiste en l’installation de deux détecteurs identiques respectivement installés à 400 m et 1050 m des deux réacteurs à eau pressurisée de la centrale nucléaire de Chooz dans les Ardennes. Les réacteurs nucléaires sont en effet à l’origine d’un flux intense d’antineutrinos électroniques (de l’ordre de 10²¹ ⊽ₑ/s pour un réacteur de 1GWe)qui peut être détecté par réaction bêta inverse dans le liquide scintillant des détecteurs : ⊽ₑ + p −&gt; e⁺ + n. Le paramè
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Stachurska, Juliana. "Astrophysical Tau Neutrinos in IceCube." Doctoral thesis, Humboldt-Universität zu Berlin, 2020. http://dx.doi.org/10.18452/21611.

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Das IceCube Neutrino Observatorium am Südpol hat die Existenz eines diffusen astrophysikalischen Neutrinoflusses nachgewiesen. Die Flavor-Zusammensetzung astrophysikalischer Neutrinos trägt Informationen über Orte kosmischer Teilchenbeschleunigung und Auswirkungen potenzieller neuer Physik auf die Neutrinoausbreitung. Zur seiner Bestimmung ist die Beobachtung von Tau-Neutrinos nötig. Ab einer Energie von ~O(100 TeV) kann deren Wechselwirkung über geladene Ströme eine Doppelkaskaden-Topologie ergeben, bei der die zwei Energiedepositionen am Tau-Entstehungs- und Tau-Zerfallsvertex aufgelöst werd
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Duan, Mingya. "Study of neutron-star and supernova matter with Skyrme functionals : response functions and new parametrizations." Electronic Thesis or Diss., université Paris-Saclay, 2024. http://www.theses.fr/2024UPASP171.

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Les étoiles à neutrons sont des objets denses qui sont produits dans des explosions de supernova à effondrement de coeur. Pour la modélisation de la supernova et du refroidissement de l'étoile à neutrons, les taux d'absorption, d'émission et de diffusion des neutrinos jouent un rôle crucial. Dans une grande partie de ces systèmes astrophysiques, les noyaux sont complètement dissous. Dans ce cas, les taux de neutrinos peuvent être directement liés aux fonctions de réponse de la matière nucléaire, calculées aux densités, asymétries et températures correspondantes. Cette thèse développe d'abord l
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Iyer, Sharada Ramalingham. "A novel approach in the detection of muon neutrino to tau neutrino oscillation from extragalactic neutrinos." Diss., The University of Arizona, 2001. http://hdl.handle.net/10150/290068.

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A novel approach is proposed for studying the ν(μ) → ν(τ) oscillation and detection of extragalactic neutrinos. Active Galactic Nuclei (AGN), Gamma Ray Bursters (GRB) and Topological Defects are believed to be sources of ultrahigh energy ν(μ) and νₑ. These astrophysical sources provide a long baseline of 100Mpc, or more, for possible detection of ν(μ) → ν(τ) oscillation with mixing parameter Δm² down to 10⁻¹⁷ eV², many orders of magnitude below the current accelerator experiments. The propagation characteristics of upward going muon and tau neutrinos is studied to show that high energy tau neu
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Usner, Marcel. "Search for Astrophysical Tau-Neutrinos in Six Years of High-Energy Starting Events in the IceCube Detector." Doctoral thesis, Humboldt-Universität zu Berlin, 2018. http://dx.doi.org/10.18452/19458.

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Astrophysikalische Neutrinos können in der Wechselwirkung kosmischer Strahlungsteilchen mit Materie oder Photonen nahe derer Quellen entstehen. Die auf der Erde erwartete Flavor-Zusammensetzung kann mögliche Neutrino Produktionsmechanismen einschränken. Tau-Neutrinos sind aufgrund von Flavor-Oszillationen über kosmische Distanzen zu erwarten. Das IceCube Neutrino Observatorium hat astrophysikalische Neutrinos bei Energien zwischen ~60 TeV und ~10 PeV entdeckt. Die gemessene Flavor-Zusammensetzung ist kompatibel mit ~1:1:1, wie vom Pion Produktionsszenario erwartet wird. Die Elektron- und Tau-N
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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
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Bechet, Sabrina. "Recherche d'un flux diffus de neutrinos tauiques d'origine cosmique dans le détecteur IceCube." Doctoral thesis, Universite Libre de Bruxelles, 2012. http://hdl.handle.net/2013/ULB-DIPOT:oai:dipot.ulb.ac.be:2013/209628.

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Le détecteur IceCube est constitué d'un réseau de modules optiques digitaux (DOMs) déployés sur un volume d'1 km³ dans la glace antarctique. Les DOMs enregistrent la lumière Cerenkov émise par les particules secondaires issues des interactions des neutrinos avec la glace. Selon la répartition géographique des signaux lumineux dans la glace, on peut différencier les différentes saveurs de leptons et ainsi identifier la saveur du neutrino primaire. Les modèles astrophysiques prédisent une production dominante de neutrinos électroniques et muoniques au sein d'accélérateurs cosmiques. Cependant, l
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Niederhausen, Hans. "Measurement of the High Energy Astrophysical Neutrino Flux Using Electron and Tau Neutrinos Observed in Four Years of IceCube Data." Thesis, State University of New York at Stony Brook, 2018. http://pqdtopen.proquest.com/#viewpdf?dispub=10823307.

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<p> The high-energy universe is known to be violent. Ultra High Energy Cosmic Rays (UHECRs) have been observed with kinetic energies exceeding 10<sup> 20</sup> eV. Their origin, despite decades of observations, remains elusive. A unique probe of the sources and production mechanisms of these high energy cosmic rays can be neutrinos, since they are inevitably produced when high-energy protons interact. The IceCube Neutrino Observatory, located at the geographical South Pole in Antarctica, continuously monitors a total volume of 1 km<sup> 3</sup> of clear Antarctic ice for neutrino interactions.
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Books on the topic "Taux de neutrinos"

1

Dodelson, Scott. Is a massive tau neutrino just what cold dark matter needs? Fermi National Accelerator Laboratory, 1994.

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Dodelson, Scott. Is a massive tau neutrino just what cold dark matter needs? Fermi National Accelerator Laboratory, 1994.

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International, Workshop on Theoretical and Phenomenological Aspects of Underground Physics (2nd 1991 Toledo Spain). TAUP 91: Proceedings of the Second International Workshop on Theoretical and Phenomenological Aspects of Underground Physics, Toledo, Spain, 9-13 September 1991. North-Holland, 1992.

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International Workshop on Theoretical and Phenomenological Aspects of Underground Physics (4th 1995 Toledo, Spain). TAUP 95: Proceedings of the Fourth International Workshop on Theoretical and Phenomenological Aspects of Underground Physics, Toledo, Spain, 17-21 September 1995. North-Holland, 1996.

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International, Workshop on Theoretical and Phenomenological Aspects of Underground Physics (3rd 1993 Laboratori Nazionali del Gran Sasso INFN Italy). TAUP 93: Proceedings of the Third International Workshop on Theoretical and Phenomenological Aspects of Underground Physics, Laboratori Nazionali del Gran Sasso, INFN, Italy, 19-23 September, 1993. North-Holland, 1994.

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Grzelak, Katarzyna. Standard and Non-standard Neutrino Oscillations Involving Tau Neutrinos. Warsaw University Press, 2018. http://dx.doi.org/10.31338/uw.9788323534327.

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Tau Lepton & Its Neutrino. World Scientific Publishing Company, 2004.

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International Workshop on Theoretical and Phenomenological Aspects of Underground Physics (2nd 1991 Toledo, Spain). TAUP 91: Proceedings of the second International Workshop on Theoretical and Phenomenological Aspects of Underground Physics. North-Holland, 1992.

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Villar, J. A., A. Morales, and J. Morales. Taup 91: Proceedings of the Second International Workshop on Theoretical and Phenomenological Aspects of Underground Physics. Elsevier Science & Technology Books, 2016.

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TAUP 89: Workshop on Theoretical and Phenomenological Aspects of Underground Physics, Laboratori Nazionali Gran Sasso (INFN) and Universita dell'Aquila, September 25-28, 1989. Editions Frontieres, 1989.

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Book chapters on the topic "Taux de neutrinos"

1

Schubert, K. R. "Measurements of the Tau-Neutrino Mass." In Neutrino Physics. Springer Berlin Heidelberg, 1988. http://dx.doi.org/10.1007/978-3-642-73679-7_12.

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Fargion, Daniele. "Tau Neutrino Astronomy." In Beyond the Desert 2003. Springer Berlin Heidelberg, 2004. http://dx.doi.org/10.1007/978-3-642-18534-2_55.

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Fargion, Daniele. "Ultra High Energy Neutrinos by Tau Airshowers." In Dark Matter in Astro- and Particle Physics. Springer Berlin Heidelberg, 2001. http://dx.doi.org/10.1007/978-3-642-56643-1_65.

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Fargion, Daniele. "Detecting Ultra High Energy Neutrinos by Upward Tau Airshowers and Gamma Flashes." In Sources and Detection of Dark Matter and Dark Energy in the Universe. Springer Berlin Heidelberg, 2001. http://dx.doi.org/10.1007/978-3-662-04587-9_52.

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Singirala, Shivaramakrishna, Suchismita Sahoo, and Rukmani Mohanta. "Majorana Dark Matter, Neutrino Mass, and Flavor Anomalies in $$L_{\mu }-L_{\tau }$$ Model." In Springer Proceedings in Physics. Springer Singapore, 2021. http://dx.doi.org/10.1007/978-981-33-4408-2_48.

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Sinha, Roopam, Sukannya Bhattacharya, and Rome Samanta. "Consequences of a CP-Transformed $$\mu \tau $$-Flavored Friedberg-Lee Symmetry in a Neutrino Mass Model." In Springer Proceedings in Physics. Springer Singapore, 2021. http://dx.doi.org/10.1007/978-981-33-4408-2_71.

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Biswas, Anirban, Sandhya Choubey, and Sarif Khan. "Dark Matter, Neutrino Mass and Muon ($$g-2$$) in a $$U(1)_{L_{\mu }}-L_{\tau }$$ Model." In XXII DAE High Energy Physics Symposium. Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-319-73171-1_225.

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Arora, Simran, Monal Kashav, Surender Verma, and B. C. Chauhan. "Muon Anomalous Magnetic Moment and Neutrino Mass in $$U(1)_{L_\mu -L_\tau }$$ Extended Scotogenic Model." In Springer Proceedings in Physics. Springer Nature Singapore, 2024. http://dx.doi.org/10.1007/978-981-97-0289-3_171.

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"THE PHYSICS OF THE TAU LEPTON AND TAU NEUTRINO IN 1995." In Reflections on Experimental Science. WORLD SCIENTIFIC, 1995. http://dx.doi.org/10.1142/9789812795816_0008.

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Conference papers on the topic "Taux de neutrinos"

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Mandal, Maitrayee. "The appearance of tau neutrinos in the flux of atmospheric neutrinos at Super-Kamiokande." In 42nd International Conference on High Energy Physics. Sissa Medialab, 2024. https://doi.org/10.22323/1.476.0154.

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Lastoria, Chiara Filomena. "Exploring tau neutrino appearance measurements in KM3NeT/ORCA." In 42nd International Conference on High Energy Physics. Sissa Medialab, 2024. https://doi.org/10.22323/1.476.0119.

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Yuksel, Emin. "NA65(DsTau): Study of tau neutrino production in p-A interactions." In 31st International Workshop on Deep Inelastic Scattering. Sissa Medialab, 2024. https://doi.org/10.22323/1.469.0186.

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Wissel, Stephanie, Andrew Zeolla, Cosmin Deaconu, et al. "Targeting 100-PeV tau neutrino detection with an array of phased and high-gain reconstruction antennas." In 10th International Workshop on Acoustic and Radio EeV Neutrino Detection Activities. Sissa Medialab, 2024. http://dx.doi.org/10.22323/1.470.0058.

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Mandal, Maitrayee. "Tau Neutrino Appearance in the Flux of Atmospheric Neutrinos at the Super-Kamiokande Experiment." In 41st International Conference on High Energy physics. Sissa Medialab, 2022. http://dx.doi.org/10.22323/1.414.1074.

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Dutta, S. Iyer. "High Energy Tau Neutrinos." In COSMOLOGY AND ELEMENTARY PARTICLE PHYSICS: Coral Gables Conference on Cosmology and Elementary Particle Physics. AIP, 2002. http://dx.doi.org/10.1063/1.1492176.

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Tseng, Jie-Jun, Tsung-Wen Yeh, H. Athar, M. A. Huang, Fei-Fain Lee, and Guey-Lin Lin. "Tau leptons from Earth skimming tau neutrinos." In International Workshop on Astroparticle and High Energy Physics. Sissa Medialab, 2003. http://dx.doi.org/10.22323/1.010.0040.

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Yaeggy Alvarez, Barbara. "3D-Reconstruction of Tau Neutrinos in LArTPC Detectors." In 3D-Reconstruction of Tau Neutrinos in LArTPC Detectors. US DOE, 2024. http://dx.doi.org/10.2172/2397233.

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Jeong, Yu Seon, Weidong Bai, Milind Diwan, Maria Vittoria Garzelli, and Mary Hall Reno. "Prompt tau neutrinos at the LHC." In The 21st international workshop on neutrinos from accelerators. Sissa Medialab, 2020. http://dx.doi.org/10.22323/1.369.0096.

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CONFORTO, GIANNI. "ELECTRON TO TAU-NEUTRINO OSCILLATIONS." In 4th San Miniato Topical Seminar on The Standard Model and Just Beyond. WORLD SCIENTIFIC, 1993. http://dx.doi.org/10.1142/9789814536011_0043.

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Reports on the topic "Taux de neutrinos"

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Okada, Kensuke. Detecting Tau Neutrino Reactions. Office of Scientific and Technical Information (OSTI), 2001. http://dx.doi.org/10.2172/1420969.

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Jessop, Colin P. First Observation of tau -> 3 pi eta tau-neutrino and tau -> f1 pi tau-neutrino Decays. Office of Scientific and Technical Information (OSTI), 2003. http://dx.doi.org/10.2172/813066.

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Deshpande, N., and K. Sharma. Limit on tau neutrino magnetic moment from neutrino counting. Office of Scientific and Technical Information (OSTI), 1990. http://dx.doi.org/10.2172/5988723.

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Jessop, Colin P. Tau Decays into Three Charged Leptons and Two Neutrinos. Office of Scientific and Technical Information (OSTI), 2003. http://dx.doi.org/10.2172/813225.

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Snyderman, N. J. Tau neutrino component to tritium beta decay. Office of Scientific and Technical Information (OSTI), 1995. http://dx.doi.org/10.2172/97152.

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Jessop, Colin P. tau-neutrino Helicity from h+- Energy Correlations. Office of Scientific and Technical Information (OSTI), 2003. http://dx.doi.org/10.2172/813096.

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Jessop, Colin P. First Observation of the Decay tau- -> k- eta tau-neutrino. Office of Scientific and Technical Information (OSTI), 2003. http://dx.doi.org/10.2172/813220.

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Jessop, Colin P. Determination of the Michel Parameters and the tau Neutrino Helicity in tau Decay. Office of Scientific and Technical Information (OSTI), 2003. http://dx.doi.org/10.2172/813081.

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Sielaff, Jason Murray. Observation of the charged current interactions of the tau neutrino. Office of Scientific and Technical Information (OSTI), 2002. http://dx.doi.org/10.2172/1420943.

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Schwienhorst, Reinhard Heinrich. A New Upper Limit for the Tau Neutrino Magnetic Moment. Office of Scientific and Technical Information (OSTI), 2000. http://dx.doi.org/10.2172/1421473.

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