Relevant bibliographies by topics / Neutrinole

Contents

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

Academic literature on the topic 'Neutrinole'

Author: Grafiati
Published: 9 March 2023
Last updated: 19 July 2025

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Journal articles on the topic "Neutrinole"

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Khatun, Amina, та Fedor Šimkovic. "Effective Majorana Neutrino Mass for ΔL = 2 Neutrino Oscillations". Symmetry 14, № 7 (2022): 1383. http://dx.doi.org/10.3390/sym14071383.

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It is well known that the observations of neutrinoless double-beta decay prove the Majorana nature of the neutrino. However, with specific values of Majorana phases, the effective Majorana neutrino mass to be estimated from the observation of neutrinoless double-beta decay experiments is strongly suppressed if the neutrino mass pattern adheres to a normal ordering. In this case, double-beta decay might not be observed even though the neutrino is Majorana in nature. We show if neutrinos oscillate to antineutrinos in their propagation; then, the observation of this oscillation proves that neutri
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Lu, Jianlong, Aik Hui Chan, and Choo Hiap Oh. "A Phenomenological Model of Effectively Oscillating Massless Neutrinos and Its Implications." EPJ Web of Conferences 240 (2020): 02002. http://dx.doi.org/10.1051/epjconf/202024002002.

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We discuss an alternative picture of neutrino oscillation. In this phenomenological model, the flavor-changing phenomena of massless neutrinos arise from scattering processes between neutrinos and four types of undetected spin-0 massive particles pervading throughout the Universe, instead of neutrinos’ own nature. These scattering processes are kinematically similar to Compton scattering. One type of left-handed massless sterile neutrino is needed in order to reproduce the neutrino oscillation modes predicted in the theory of neutrino mixing. Implications of our model include the existence of
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Faessler, A. "Super-Kamiokande neutrino oscillations and the supersymmetric model." HNPS Proceedings 9 (February 11, 2020): 14. http://dx.doi.org/10.12681/hnps.2773.

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The standard model predicts a ratio of 2 for the number of atmospheric muon to electron neutrinos, while super-Kamiokande and others measure a much smaller value (1.30±0.02 for super-Kamiokande). Super-Kamiokande is also able to measure roughly the direction and the energy of the neutrinos. The zenith-angle dependence for the muon neutrinos suggests that the muon neutrinos oscillate into a third neutrino species, either into the r neutrino or a sterile neutrino. This finding is inves- tigated within the supersymmetric model. The neutrinos mix with the neutralinos, this meaning the wino, the bi
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BILENKY, S. M. "NEUTRINOS: A BRIEF REVIEW." Modern Physics Letters A 19, no. 33 (2004): 2451–77. http://dx.doi.org/10.1142/s0217732304015944.

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The major steps in the development of our knowledge about neutrinos are reviewed. The basics of neutrino oscillation formalism is presented. Neutrino oscillations in the framework of three-neutrino mixing are considered. The evidence for neutrino oscillations is discussed. Neutrinoless double β-decay is briefly considered.
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Giunti, Carlo, and Thierry Lasserre. "eV-Scale Sterile Neutrinos." Annual Review of Nuclear and Particle Science 69, no. 1 (2019): 163–90. http://dx.doi.org/10.1146/annurev-nucl-101918-023755.

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We address the phenomenology of light sterile neutrinos, with an emphasis on short-baseline neutrino oscillations. After reviewing the observed short-baseline neutrino oscillation anomalies, we discuss the global fit of the data and the current appearance–disappearance tension. We also review briefly the effects of light sterile neutrinos in β decay, neutrinoless double-β decay, and cosmology. Finally, we discuss future perspectives of the search for the effects of eV-scale sterile neutrinos.
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Verma, Rishu, Monal Kashav, Ankush B, Gazal Sharma, Surender Verma, and B. C. Chauhan. "Texture One Zero Model Based on A4 Flavor Symmetry and its Implications to Neutrinoless Double Beta Decay." Journal of Nuclear Physics, Material Sciences, Radiation and Applications 9, no. 1 (2021): 67–71. http://dx.doi.org/10.15415/jnp.2021.91012.

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Neutrinos are perhaps the most elusive particles in our Universe. Neutrino physics could be counted as a benchmark for various new theories in elementary particle physics and also for the better understanding of the evolution of the Universe. To complete the neutrino picture, the missing information whether it is about their mass or their nature that the neutrinos are Majorana particles could be provided by the observation of a process called neutrinoless double beta (0νββ) decay. Neutrinoless double beta decay is a hypothesised nuclear process in which two neutrons simultaneously decay into p
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Francis, Ng K., and Ankur Nath. "The Effects of Majorana Phases in Estimating the Masses of Neutrinos." International Journal of Modern Physics: Conference Series 47 (January 2018): 1860100. http://dx.doi.org/10.1142/s201019451860100x.

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Majorana CP violating phases coming from heavy right-handed Majorana mass matrices([Formula: see text]) are considered to estimate the masses of neutrinos. The effects of phases on quasi-degenerate neutrinos mass matrix obeying [Formula: see text] symmetry predicts the results consistent with observations for (i) solar mixing angle([Formula: see text]) below TBM, (ii) absolute neutrino mass parameters[[Formula: see text]] in neutrinoless double beta([Formula: see text]) decay, and (iii) cosmological upper bound [Formula: see text]. Analysis is carried out through parameterization of light left
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Kudenko, Yury. "New results and perspectives in neutrino physics." EPJ Web of Conferences 212 (2019): 01005. http://dx.doi.org/10.1051/epjconf/201921201005.

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A brief review of new results and perspectives in neutrino physics is presented. An emphasis on a search for CP violation in neutrino oscillations and a search for sterile neutrinos is given. Status of measurement of the direct neutrino mass measurement and searches for neutrinoless double beta decay are also discussed.
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Petcov, S. T. "The Nature of Massive Neutrinos." Advances in High Energy Physics 2013 (2013): 1–20. http://dx.doi.org/10.1155/2013/852987.

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The compelling experimental evidences for oscillations of solar, reactor, atmospheric, and accelerator neutrinos imply the existence of 3-neutrino mixing in the weak charged lepton current. The current data on the 3-neutrino mixing parameters are summarised and the phenomenology of 3-νmixing is reviewed. The properties of massive Majorana neutrinos and of their various possible couplings are discussed in detail. Two models of neutrino mass generation with massive Majorana neutrinos—the type I see-saw and the Higgs triplet model—are briefly reviewed. The problem of determining the nature, Dirac
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Okada, Nobuchika, and Osamu Yasuda. "A Sterile Neutrino Scenario Constrained By Experiments and Cosmology." International Journal of Modern Physics A 12, no. 21 (1997): 3669–94. http://dx.doi.org/10.1142/s0217751x97001894.

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We analyze a scheme in which three active neutrinos and one sterile neutrino account for the solar, the atmospheric and the LSND neutrino anomalies in a model-independent way. It is shown that if the equivalent number, Nν, of the light neutrino species is less than 4, then the constraints from these anomalies, accelerator and reactor experiments and big bang nucleosynthesis force a general 4 × 4 mixing matrix to be effectively split into two 2 × 2 matrices. If these neutrinos are of the Majorana type, then negative results of neutrinoless double beta decay experiments imply that the total mass
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Dissertations / Theses on the topic "Neutrinole"

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POZZI, STEFANO. "Search for double-beta decay of 130Te to the excited states of 130Xe in CUORE-0." Doctoral thesis, Università degli Studi di Milano-Bicocca, 2017. http://hdl.handle.net/10281/158137.

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CUORE-0 è stato un esperimento bolometrico, mantenuto in funzione dal 2013 al 2015, il cui scopo scientifico principale è stata la ricerca del decadimento doppio beta senza emissione di neutrini (0vbb) nel 130Te. Il rivelatore era costituito da 52 cristalli di TeO2, usati sia come rivelatore che come sorgente dell'isotopo di interesse. I cristalli erano organizzati in una singola torre e contenuti in un criostato capace di raggiungere la temperatura di 10 mK. Grazie al basso fondo radioattivo raggiunto dall'esperimento, la ricerca di altri processi rari, oltre al decadimento doppio beta senza
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Wong, Chan Fai. "Phenomenology of sterile neutrinos at different mass scales : neutrinoless double beta decay and neutrino oscillations." Thesis, Durham University, 2012. http://etheses.dur.ac.uk/4931/.

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The existence of neutrino oscillation is the first evidence of physics beyond the Standard Model. It proves that neutrinos are massive and motivates the study of the neutrino nature, mixings and mass generation models. To have a better understanding of neutrino masses and mixings, the existence and character of sterile neutrinos would be an important factor. In this thesis, we will describe the phenomena of neutrinoless double beta decay and sterile neutrino oscillations. The studies of these two topics will contribute to understanding the properties of sterile neutrinos in the heavy and light
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Gratieri, Diego Rossi 1982. "Fenomenologia de neutrinos atmosféricos com neutrinos de massa variável." [s.n.], 2012. http://repositorio.unicamp.br/jspui/handle/REPOSIP/278535.

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Orientador: Orlando Luis Goulart Peres<br>Tese (doutorado) - Universidade Estadual de Campinas, Instituto de Física Gleb Wataghin<br>Made available in DSpace on 2018-08-20T17:03:07Z (GMT). No. of bitstreams: 1 Gratieri_DiegoRossi_D.pdf: 1179296 bytes, checksum: 9a313c3efcf6512bd55d97d0b99d491b (MD5) Previous issue date: 2012<br>Resumo: Neste trabalho obtemos de forma independente a descrição da distribuição angular dos eventos de neutrinos atmosféricos vistos pelo detector Super-Kamiokande tanto para as regiões de sub-GeV como multi-GeV. Para tal, estudamos de forma detalhada a seção de choq
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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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Girardi, Ivan. "Discrete Symmetry Approach to Lepton Flavour, Neutrino Mixing and Leptonic CP Violation, and Neutrino Related Physics Beyond the Standard Theory." Doctoral thesis, SISSA, 2016. http://hdl.handle.net/20.500.11767/4923.

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The experimental evidences of neutrino oscillation, caused by non-zero neutrino masses and neutrino mixing, which were obtained in the experiments with solar, atmospheric, accelerator and reactor neutrinos, opened new field of research in elementary particle physics. The principal goal is to understand at fundamental level the mechanism giving rise to non-zero neutrino masses and neutrino mixing. The open fundamental questions include those of the nature — Dirac or Majorana — of massive neutrinos, of the type of spectrum neutrino masses obey, of the status of CP symmetry in the lepton sector,
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George, Jeffrey S. "Experimental study of the atmospheric [Nu][mu]/[Nu]e ratio in the multi-GeV energy range /." Thesis, Connect to this title online; UW restricted, 1998. http://hdl.handle.net/1773/9752.

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Manzanillas, Luis. "Development of the source calibration system of the STEREO experiment and search for sterile neutrinos at the ILL." Thesis, Université Grenoble Alpes (ComUE), 2016. http://www.theses.fr/2016GREAY079/document.

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L'expérience STEREO a été proposé afin de donner une réponse sans ambiguïté àl'idée d'un état de neutrino stérile léger ($Delta m^{2}sim 1eV^{2}$) comme l'origine del'anomalie réacteur des antineutrinos. Le but de l'expérience est de confirmer ou de rejetercette hypothèse en recherchant un patron d'oscillation à courte distance (9-11 m) dans lespectre en énergie des $overline{nu_{e}}$'s émis par le réacteur nucléaire de recherchede l'Institut Laue-Langevin à Grenoble (France). A cet effet, le détecteur estcomposé de 2 tonnes du liquide scintillant dopé au Gd et lu par un réseau detubes photomu
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Pascoal, Kellen Alves. "Neutrino-magnetohidrodinâmica, oscilações de neutrinos e instabilidades em plasmas." reponame:Biblioteca Digital de Teses e Dissertações da UFRGS, 2018. http://hdl.handle.net/10183/180517.

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Foi feita uma modificação da teoria magnetohidrodinâmica, incorporando a dinâmica dos neutrinos, chamada magnetohidrodinâmica de neutrinos. Elétrons e íons foram toma- dos como não-relativísticos, juntamente com os neutrinos eletrônicos (ultra) relativísticos acoplados via força eletro-fraca. Devido à ressonância com um feixe de neutrinos, foi prevista a desestabilização das ondas magnetosônicas rápidas. Admitindo modos oblí- quos, é possível detectar uma instabilidade que se torna mais forte quando o vetor de onda é paralelo ao campo magnético de equilíbrio, associando-se à onda magnetosônica
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Tapia, Herrera Luis Carlos 1982. "Fenomenologia dos decaimentos de neutrinos de supernova." [s.n.], 2011. http://repositorio.unicamp.br/jspui/handle/REPOSIP/278537.

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Orientador: Orlando Luis Goulart Peres<br>Dissertação (mestrado) - Universidade Estadual de Campinas, Instituto de Física Gleb Wataghin<br>Made available in DSpace on 2018-08-19T13:26:00Z (GMT). No. of bitstreams: 1 TapiaHerrera_LuisCarlos1982-_M.pdf: 3198399 bytes, checksum: bd22a4c22f21d4db7bc8f29cda4bd521 (MD5) Previous issue date: 2011<br>Resumo: Apresentamos neste trabalho um estudo da fenomenologias dos neutrinos, que inicia com um modelo além do Modelo Padrão, que gera massa e decaimento para os neutrinos. O modelo foi proposto por Gelmini e Roncadelli [3], no modelo é introducido um
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Boriero, Daniel Francisco 1981. "Fenomenologia de neutrinos massivos em cosmologia." [s.n.], 2013. http://repositorio.unicamp.br/jspui/handle/REPOSIP/278586.

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Orientador: Pedro Cunha de Holanda<br>Tese (doutorado) - Universidade Estadual de Campinas, Instituto de Física Gleb Wataghin<br>Made available in DSpace on 2018-08-22T08:38:27Z (GMT). No. of bitstreams: 1 Boriero_DanielFrancisco_D.pdf: 1994859 bytes, checksum: a59e512b9fdcb71d04bb5f9702f0fb60 (MD5) Previous issue date: 2013<br>Resumo: Cosmologia de neutrinos é a atividade de pesquisa dedicada ao teste de propriedades de neutrinos através de observáveis cosmológicos. Particularmente, as propriedades estudadas e testadas ao longo desta tese de doutorado foram à massa dos neutrinos e o número
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Books on the topic "Neutrinole"

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1949-, Cherry M. L., Lande K, and Fowler William A, eds. Solar neutrinos and neutrino astronomy: (Homestake, 1984). American Institute of Physics, 1985.

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1938-, Barger V., ed. Neutrino masses and neutrino astrophysics: Including Supernova 1987a : Ashland, Wisconsin, 1987. World Scientific Pub. Co., 1987.

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1930-, Winter Klaus, ed. Neutrino physics. Cambridge University Press, 1991.

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International, Conference on Neutrino Physics and Astrophysics (1992 Granada Spain). Neutrino 92: Proceedings of the 15th International Conference on Neutrino Physics and Astrophysics, Granada, Spain, 7-12 June 1992. North-Holland, 1993.

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International, Conference on Neutrino Physics and Astrophysics (19th 2000 Sudbury Canada). Neutrino 2000: Proceedings of the XIXth International Conference on Neutrino Physics and Astrophysics, Sudbury, Canada, 16-21 June 2000. North Holland, 2001.

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International, Conference on Neutrino Physics and Astrophysics (13th 1988 Medford Mass ). Proceedings of the 13th International Conference on Neutrino Physics and Astrophysics, Boston (Medford), June 5-11, 1988. World Scientific Pub. Co., 1989.

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International Conference on Neutrino Physics and Astrophysics (16th 1994 Eilat, Israel). Neutrino 94: Proceedings of the 16th International Conference on Neutrino Physics and Astrophysics : Eilat, Israel, 29 May-3 June, 1994. North-Holland, 1995.

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International Conference on Neutrino Physics and Astrophysics (21st 2004 Paris, France). Neutrino 2004: Proceedings of the XXIst International Conference on Neutrino Physics and Astrophysics, Paris, France, 14-19 June 2004. Elsevier, 2005.

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International Conference on Neutrino Physics and Astrophysics (18th 1998 Takayama, Japan). Neutrino '98: Proceedings of the XVIIIth International Conference on Neutrino Physics and Astrophysics : Takayama, Japan, 4-9 June 1998. North-Holland, 1999.

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International Workshop on Neutrino-Nucleus Interactions in the Few-GeV Region (3rd 2004 Assergi, Italy). NuInt04: Proceedings of the Third International Workshop on Neutrino-Nucleus Interactions in the Few-GeV Region : Assergi, Italy, 17-21 March 2004. Elsevier, 2005.

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Book chapters on the topic "Neutrinole"

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Binchi, Leen, and Amine Ahriche. "Neutrinos from Type-II Supernovae." In Springer Proceedings in Physics. Springer Nature Singapore, 2025. https://doi.org/10.1007/978-981-96-3276-3_4.

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Abstract In our work we investigate the stellar surface fluxes of different neutrino flavors, both with and without matter effects, while aiming to consider the varying density of the progenitor star to reveal intriguing variations in their behavior. By examining both normal and inverted neutrino mass hierarchies in studies of neutrino fluxes, a behavioral difference is detected which highlights the significance of the chosen mass hierarchy for studies in understanding the neutrino oscillation phenomena. This difference in flux behavior also serves as a clue to probe the mass hierarchy; within the energy range of 13–19 meV, the neutrino mass hierarchy can be determined as normal or inverted by detecting excess or missing events in the non-electronic neutrinos. We also examine the level crossing diagrams of neutrinos to illustrate how different neutrino masses and energies affect the transformation of neutrino flavors as they propagate through matter with constant density. We determine the resonance regions (both high and low) with the highest flipping probability using the level crossing diagrams. This allows us to estimate where within a star we are most likely to find neutrino flavor conversions.
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Medhi, Abinash, Prantik Sarmah, Moon Moon Devi, Sovan Chakraborty, and Debanjan Bose. "Probing Neutrino Mass Ordering with Supernova Neutrinos." In Springer Proceedings in Physics. Springer Nature Singapore, 2024. http://dx.doi.org/10.1007/978-981-97-0289-3_271.

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Ejiri, Hiroyasu. "Neutrino-less double beta decays and Majorana neutrinos." In PAVI09. Springer Netherlands, 2011. http://dx.doi.org/10.1007/978-94-007-4023-5_12.

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Ronga, F. "Atmosperic Neutrinos and Neutrino Oscillations in the Macro Experiment." In Cosmic Radiations: From Astronomy to Particle Physics. Springer Netherlands, 2001. http://dx.doi.org/10.1007/978-94-010-0634-7_10.

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Ando, Shin’ichiro, and Katsuhiko Sato. "Supernova Relic Neutrinos and Observational Implications for Neutrino Oscillation." In Beyond the Desert 2003. Springer Berlin Heidelberg, 2004. http://dx.doi.org/10.1007/978-3-642-18534-2_47.

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von Feilitzsch, F. "Neutrino Properties." In Neutrinos. Springer Berlin Heidelberg, 1988. http://dx.doi.org/10.1007/978-3-642-46648-9_1.

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Gelmini, G. "Neutrinos in Cosmology." In Neutrinos. Springer Berlin Heidelberg, 1988. http://dx.doi.org/10.1007/978-3-642-46648-9_10.

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Winter, K. "Neutrino Reactions and the Structure of the Neutral Weak Current." In Neutrinos. Springer Berlin Heidelberg, 1988. http://dx.doi.org/10.1007/978-3-642-46648-9_2.

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Langacker, P. "Massive Neutrinos in Gauge Theories." In Neutrinos. Springer Berlin Heidelberg, 1988. http://dx.doi.org/10.1007/978-3-642-46648-9_3.

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Mohapatra, R. N. "Neutrinos in Left-Right Symmetric, SO(10) and Superstring Inspired Models." In Neutrinos. Springer Berlin Heidelberg, 1988. http://dx.doi.org/10.1007/978-3-642-46648-9_4.

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Conference papers on the topic "Neutrinole"

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Petropavlova, Maria. "Constraints on Neutrino Self Interactions from Multi-messenger neutrinos scattering on C$\nu$B." In 42nd International Conference on High Energy Physics. Sissa Medialab, 2024. https://doi.org/10.22323/1.476.0185.

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Yurchenko, V., and A. Ivanchik. "Relic neutrinos distribution function at low coordinate momentums." In ASTRONOMY AT THE EPOCH OF MULTIMESSENGER STUDIES. Proceedings of the VAK-2021 conference, Aug 23–28, 2021. Crossref, 2022. http://dx.doi.org/10.51194/vak2021.2022.1.1.170.

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The effect of processes p + e − → n + ν e and µ + → e + + ν̃ µ + ν e on relic neutrino distribution function in the region ofsmall coordinate momentums is studied. The Boltzmann kinetic equation on the electron neutrino distribution function issolved in this region at temperatures above 10 MeV taking into account generation of electron neutrinos due to the aboveprocesses in the assumption that at these temperatures neutrinos of larger momentums are thermalized instantaneously.The effect of thermalization of neutrinos due to their scattering on electrons and positrons on the distribution function
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Kuzmitskiy, A. V., and A. A. Kochanov. "DEPTH INTENSITY RELATION AND ANGULAR DISTRIBUTION OF THE HIGH-ENERGY ATMOSPHERIC MUONS IN WATER MEDIUM: NEW CALCULATION." In Baikal Young Scientists’ International School on Fundamental Physics. Institute of Solar-Terrestrial Physics SB RAS, 2024. http://dx.doi.org/10.62955/0135-3748-2024-51.

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One of the important tasks of high-energy astrophysics is the search for cosmic neutrinos and the determination of their sources. To solve this problem, large-volume detectors are being created – neutrino telescopes that register Cherenkov light from charged particles generated by neutrino interactions in the medium. Cherenkov light can be produced not only by muons from neutrinos or hadron showers, but also by transit atmospheric muons. Therefore, the analysis of events, recorded in neutrino telescopes, requires a thorough study of the background of muons. It is necessary to know the characte
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Krestyanskikh, M. G., and I. A. Perevalova. "HIT SELECTION AND RECONSTRUCTION OF NEAR-VERTICAL MUON TRACKS BASED ON DATA FROM ONE STRING OF THE BAIKAL-GVD." In Baikal Young Scientists’ International School on Fundamental Physics. Institute of Solar-Terrestrial Physics SB RAS, 2024. http://dx.doi.org/10.62955/0135-3748-2024-48.

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Baikal neutrino telescope is a deep water installation used for detection of high-energy astrophysical neutrinos, with energies up to 1018 eV. Neutrinos interact with matter extremely weakly, so the process of its registration is quite complicated. Flying through the Earth, a neutrino can interact weakly with the matter, with secondary particle appearing, for example muon, which keeps direction the first neutrino direction, and its known energy part as well. Moving in water, a muon that appeared this way has the speed exceeding the phase speed of light and, therefore, outputs Cherenkov radiati
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Zhou, Fan, Yang Du, Zhiping Chen, Shaojing Hou, and Yuekun Heng. "Design and Application of an Equator Flexible Supported Acrylic Spherical Vessel for Neutrino Detector." In ASME 2018 Pressure Vessels and Piping Conference. American Society of Mechanical Engineers, 2018. http://dx.doi.org/10.1115/pvp2018-84128.

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The second stage of the Daya Bay neutrino experiment, the Jiangmen Underground Neutrino Observatory (JUNO), will be launched to investigate more neutrino physics. The vessel, which is used to contain the liquid target for detecting neutrinos, plays a significant role in JUNO. It must meet diverse design criteria according to the requirements for physics measurement and safe operation. This paper proposed an alternative structural scheme for the containment vessel. Acrylic is selected as the material for its high transparency and excellent mechanical properties. A sphere 35.5m in diameter is ch
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Lin, T. "EVENT INDEX BASED CORRELATION ANALYSIS FOR THE JUNO EXPERIMENT." In 9th International Conference "Distributed Computing and Grid Technologies in Science and Education". Crossref, 2021. http://dx.doi.org/10.54546/mlit.2021.49.10.001.

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The Jiangmen Underground Neutrino Observatory (JUNO) experiment is mainly designed todetermine the neutrino mass hierarchy and precisely measure oscillation parameters by detectingreactor anti-neutrinos. The total event rate from DAQ is about 1 kHz and the estimated volume of rawdata is about 2 PB/year. But the event rate of reactor anti-neutrino is only about 60/day. So one of thechallenges for data analysis is to select sparse physics signal events in a very large amount of data,whose volume can not be reduced by using the traditional data streaming method. In order to improvethe speed of da
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Stanev, Todor. "ATMOSPHERIC NEUTRINOS AND NEUTRINO OSCILLATIONS." In Proceedings of the International School of Cosmic Ray Astrophysics 20th Anniversary, 11th Course. WORLD SCIENTIFIC, 2000. http://dx.doi.org/10.1142/9789812793997_0004.

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Kang, Sin Kyu. "Neutrinoless double beta decay, Majonara neutrino masses and Neutrino Oscillations." In Proceedings of the Sixth Workshop. WORLD SCIENTIFIC, 2002. http://dx.doi.org/10.1142/9789812778352_0004.

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ANDO, SHIN’ICHIRO, and KATSUHIKO SATO. "SUPERNOVA RELIC NEUTRINOS AND NEUTRINO OSCILLATION." In Proceedings of the Fourth International Workshop. WORLD SCIENTIFIC, 2004. http://dx.doi.org/10.1142/9789812703101_0007.

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NARDI, E. "MEASURING NEUTRINO MASSES WITH SUPERNOVA NEUTRINOS." In Proceedings of the MG10 Meeting held at Brazilian Center for Research in Physics (CBPF). World Scientific Publishing Company, 2006. http://dx.doi.org/10.1142/9789812704030_0079.

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Reports on the topic "Neutrinole"

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Fallot, M., B. Littlejohn, and Paraskevi Dimitriou. Antineutrino spectra and their applications. IAEA Nuclear Data Section, 2019. http://dx.doi.org/10.61092/iaea.e4zk-7ryk.

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Abstract:
A summary is given of a Technical Meeting assembled to review the status-of-affairs in experiments, models and nuclear data associated with the determination of the anti-neutrino flux and spectrum as produced by reactor neutrinos. Participants discussed the latest experimental results in measurements and models and recommended future improvements in the data analysis, nuclear model corrections and nuclear decay data. There was overall consensus that the field of reactor neutrinos would benefit from international coordination in the form of an international working group. Details of the discuss
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Wolfenstein, L. Neutrino masses and solar neutrinos. Office of Scientific and Technical Information (OSTI), 1992. http://dx.doi.org/10.2172/6967046.

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Wolfenstein, L. Neutrino masses and solar neutrinos. Office of Scientific and Technical Information (OSTI), 1992. http://dx.doi.org/10.2172/10187797.

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Elliott, Steven. Neutrinoless double beta decay and the neutrino. Office of Scientific and Technical Information (OSTI), 2021. http://dx.doi.org/10.2172/1787275.

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Fuyuto, Kaori. Neutrinoless double beta decay with light sterile neutrinos. Office of Scientific and Technical Information (OSTI), 2023. http://dx.doi.org/10.2172/1908468.

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Gollapinni, Sowjanya. Unlocking the Mysteries of Neutrinos with the Deep Underground Neutrino Experiment. Office of Scientific and Technical Information (OSTI), 2021. http://dx.doi.org/10.2172/1771069.

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Dishaw, j. The Production of Neutrinos and Neutrino-like Particles in Proton-Nucleus Interactions. Office of Scientific and Technical Information (OSTI), 2018. http://dx.doi.org/10.2172/1453961.

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Coleman, Stephen James. A measurement of neutrino oscillations with muon neutrinos in the MINOS experiment. Office of Scientific and Technical Information (OSTI), 2011. http://dx.doi.org/10.2172/1023978.

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Groh, Micah. Constraints on Neutrino Oscillation Parameters from Neutrinos and Antineutrinos with Machine Learning. Office of Scientific and Technical Information (OSTI), 2021. http://dx.doi.org/10.2172/1774291.

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Mendez Mendez, Diana Patricia. Search for Muon Neutrino Disappearance in the Booster Neutrino Beam of Fermilab; Busqueda de Desaparicion de Neutrinos del Muon en el Haz de Neutrinos del Booster de Fermilab. Office of Scientific and Technical Information (OSTI), 2015. http://dx.doi.org/10.2172/1209242.

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You might also be interested in the extended bibliographies on the topic 'Neutrinole' for particular source types:
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