Gotowe bibliografie tematyczne / Neutrino mass and mixing

Spis treści

  1. Artykuły w czasopismach
  2. Rozprawy doktorskie
  3. Książki
  4. Części książek
  5. Streszczenia konferencji
  6. Raporty organizacyjne

Gotowa bibliografia na temat „Neutrino mass and mixing”

Autor: Grafiati
Data publikacji: 2 czerwca 2025
Data aktualizacji: 31 lipca 2025

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Artykuły w czasopismach na temat "Neutrino mass and mixing"

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BILENKY, S. M., C. GIUNTI, and C. W. KIM. "FINALLY NEUTRINO HAS MASS." International Journal of Modern Physics A 15, no. 05 (2000): 625–50. http://dx.doi.org/10.1142/s0217751x00000318.

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The present status of the problem of neutrino mass, mixing and neutrino oscillations is briefly summarized. The evidence for oscillations of atmospheric neutrinos found recently in the Super-Kamiokande experiment is discussed. Indications in favor of neutrino oscillations obtained in solar neutrino experiments and in the accelerator LSND experiment are also considered. Implications of existing neutrino oscillation data for neutrino masses and mixing are discussed.
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KANG, KYUNGSIK, SIN KYU KANG, C. S. KIM, and SUN MYONG KIM. "NEUTRINO OSCILLATIONS AND LEPTON FLAVOR MIXING." Modern Physics Letters A 16, no. 33 (2001): 2169–75. http://dx.doi.org/10.1142/s0217732301005473.

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In view of the recent announcement on nonzero neutrino mass from Super-Kamiokande experiment, it would be very timely to investigate all the possible scenarios on masses and mixings of light neutrinos. Recently suggested mass matrix texture for the quark CKM mixing, which can be originated from the family permutation symmetry and its suitable breakings, is assumed for the neutrino mass matrix and determined by the four combinations of solar, atmospheric and LSND neutrino data and cosmological hot dark matter bound as input constraints. The charged-lepton mass matrix is assumed to be diagonal s
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Saez, M. M., O. Civitarese, and M. E. Mosquera. "Neutrino mixing in nuclear rapid neutron-capture processes." International Journal of Modern Physics E 29, no. 04 (2020): 2050022. http://dx.doi.org/10.1142/s0218301320500226.

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A possible mechanism for the formation of heavy-mass elements in supernovae is the rapid neutron-capture-mechanism ([Formula: see text]-process). It depends upon the electron-fraction [Formula: see text], a quantity which is determined by beta-decay-rates. In this paper, we focus on the calculation of electroweak decay-rates in presence of massive neutrinos. The resulting expressions are then used to calculate nuclear reactions entering the rapid-neutron capture. We fix the astrophysical parameters to the case of a core-collapse supernova. The neutrino sector includes a mass scheme and mixing
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Bhatti, A. Aziz, and Harald Fritzsch. "Zero texture lepton mass matrices and near tribimaximal mixing in the SO(10) theory." Modern Physics Letters A 29, no. 12 (2014): 1450059. http://dx.doi.org/10.1142/s021773231450059x.

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We have described the quark and lepton masses and mixings in context of non-SUSY SO(10) and "four-zero-texture" (FZT). In the FZT case, the fermion masses and the mixing angles can be related. We predict the neutrino masses using the near tribimaximal (TBM) mixing and the triminimal mixing. Our results show that under TBM, the neutrinos have a normal, but weak hierarchy. Variations of the neutrino masses under the "Near TBM-scenario" are also discussed.
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FRITZSCH, HARALD. "FLAVOR SYMMETRIES, NEUTRINO MASSES AND NEUTRINO MIXING." International Journal of Modern Physics A 23, no. 21 (2008): 3179–82. http://dx.doi.org/10.1142/s0217751x08041773.

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We discuss the neutrino mixing, using the texture 0 mass matrices, which work very well for the quarks. The solar mixing angle is directly linked to the mass ratio of the first two neutrinos. The neutrino masses are hierarchical, but the mass ratios turn out to be much smaller than for quarks. The atmospheric mixing angle is 38°. The CP violation for leptons should be much smaller than for quarks.
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Nicolaidis, Argyris. "Neutrinos and the structure of space-time." Facta universitatis - series: Physics, Chemistry and Technology 12, no. 2 (2014): 179–88. http://dx.doi.org/10.2298/fupct1402179n.

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The phenomenon of neutrino oscillations is studied usually as a mixing between the flavor neutrinos and the neutrinos having a definite mass. The mixing angles and the mass eigenvalues are treated independently in order to accommodate the experimental data. We suggest that neutrino oscillations are connected to the structure of spacetime. We expand on a recently proposed model, where two ?mirror? branes coexist. One brane hosts left-handed particles (our brane), while the other brane hosts right-handed particles. Majorana-type couplings mixes neutrinos in an individual brane, while Dirac-type
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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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Vien, V. V. "Lepton mass and mixing in a neutrino mass model based onS4flavor symmetry." International Journal of Modern Physics A 31, no. 09 (2016): 1650039. http://dx.doi.org/10.1142/s0217751x16500391.

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We study a neutrino mass model based on [Formula: see text] flavor symmetry which accommodates lepton mass, mixing with nonzero [Formula: see text] and CP violation phase. The spontaneous symmetry breaking in the model is imposed to obtain the realistic neutrino mass and mixing pattern at the tree-level with renormalizable interactions. Indeed, the neutrinos get small masses from one [Formula: see text] doublet and two [Formula: see text] singlets in which one being in [Formula: see text] and the two others in [Formula: see text] under [Formula: see text] with both the breakings [Formula: see
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Verma, Surender. "Theoretical and Phenomenological Status of Neutrino Physics: A Brief Review." Advances in High Energy Physics 2015 (2015): 1–15. http://dx.doi.org/10.1155/2015/385968.

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We present an overview of recent progress in the theoretical and phenomenological studies of neutrino masses, lepton avor mixing, and CP violation. Firstly, We discuss the status of neutrino mass with in the Standard Model (SM) of particle physics. Then the possible ways in which neutrino mass terms can be included in the SM are discussed. The inclusion of new physics beyond the SM inevitably brings new parameters which are not constrained by the present experimental data on neutrino masses and mixing angles and, thus, are free parameters of the theory. We, also, discuss various theoretically
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FRITZSCH, H. "FLAVOR MIXING, QUARK MASSES, NEUTRINO MASSES AND NEUTRINO OSCILLATIONS." International Journal of Modern Physics A 24, no. 18n19 (2009): 3354–58. http://dx.doi.org/10.1142/s0217751x09046941.

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We study a model for the mass matrices of the quarks and leptons. Two of the three flavor mixing angles of the quarks can be calculated in terms of the quark mass ratios. They agree very well with the experiments. We are able to relate the mass eigen values of the charged leptons and of the neutrinos to the mixing angles and can predict the masses of the neutrinos. We find a normal hierarchy -the masses are 0.004 eV, 0.01 eV and 0.05 eV. The atmospheric mixing angle is given by the mass ratios of the charged leptons and the neutrinos. We find 38 degrees, consistent with the experiments. The mi
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Rozprawy doktorskie na temat "Neutrino mass and mixing"

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Cooper, Iain K. "On discrete flavour symmetries, neutrino mass and mixing." Thesis, University of Southampton, 2012. https://eprints.soton.ac.uk/345719/.

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Neutrino mixing is a thriving area of particle physics research, with the recent discovery of non-zero θ13 inspiring a large amount of research into the field. This thesis presents two models which aim to explain the observed neutrino mixing patterns in the context of Grand Unified Theories, which also output quark masses and mixings. A model predicting Tri-Bimaximal mixing is presented which combines a previously published SU(5) model with an A4 family symmetry. Extra adjoint fermionic matter is present as prescribed by the original Unified model, and this provides 2 seesaw particles; however
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Mannaa, Sammy, and Antek Szadaj. "Distribution of Neutrino Mixing Parameters FromReal and Complex Random Neutrino Mass Matrices." Thesis, KTH, Teoretisk fysik, 2013. http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-127458.

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The theory of neutrino oscillations is covered. Also, the theory of Dirac, Majorana, and Dirac-Majorana neutrinos is presented. From this theory, and the model presented in [7], a program is constructed which creates a suitable number of neutrino mass matrices M using pseudo-random numbers generated in MATLAB. These matrices are diagonalised, and from the general notion of the Pontecorvo-Maki-Nakagawa-Sakata matrix UPMNS, statistical distributions of six mixing parameters are presented, namely; 12; 13; 23, the CP-violating Dirac phase delta ( ), and two Majorana CP-violating phases alpha one a
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Schirato, Richard C. "Neutrino mass and mixing schemes : effects on supernova signal and an experiment for direct verification /." Diss., Connect to a 24 p. preview or request complete full text in PDF format. Access restricted to UC campuses, 2002. http://wwwlib.umi.com/cr/ucsd/fullcit?p3071051.

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Hällgren, Tomas. "Aspects of Dimensional Deconstruction and Neutrino Physics." Doctoral thesis, KTH, Teoretisk partikelfysik, 2007. http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-4480.

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The existence of at or curved extra spatial dimensions provides new insights into several of the problems which face the Standard Model of particle physics, including the gauge hierarchy problem, the smallness of neutrino masses, and the dark matter problem. However, higher-dimensional gauge theories are not renormalizable and can only be considered as low-energy effective theories, with limited applicability. Dimensional deconstruction provides a class of manifestly gauge invariant possible ultraviolet completions of higher-dimensional gauge theories, formulated within conventional quantum el
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Medina, Alberto Martin Gago. "Soluções de grande comprimento de oscilação para o problema de neutrinos solares." Universidade de São Paulo, 2001. http://www.teses.usp.br/teses/disponiveis/43/43134/tde-04122013-105222/.

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Esta tese apresenta uma análise estatística detalhada dos dados de experimentos com neutrinos solares mais recentes, com duas diferentes soluções para oscilações de neutrinos, ambas caracterizadas por um grande comprimento de oscilação. A primeira baseada no mecanismo de oscilação padrão, ou seja, induzida por massa, sendo esta estudada nos casos de duas e três gerações e dentro do regime de quase-vácuo. E a segunda, uma exótica, que usa como mecanismo de oscilação uma possível violação do princípio de equivalência, que foi analisada somente para o caso de duas gerações, sendo este discutido p
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Blennow, Mattias. "Theoretical and Phenomenological Studies of Neutrino Physics." Doctoral thesis, Stockholm : Department of Theoretical Physics, Royal Institute of Technology, 2007. http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-4415.

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Bergström, Johannes. "Predictions of Effective Models in Neutrino Physics." Licentiate thesis, KTH, Teoretisk partikelfysik, 2011. http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-35267.

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Experiments on neutrino oscillations have confirmed that neutrinos have small, but non-zero masses, and that the interacting neutrino states do not have definite masses, but are mixtures of such states.The seesaw models make up a group of popular models describing the small neutrino masses and the corresponding mixing.In these models, new, heavy fields are introduced and the neutrino masses are suppressed by the ratio between the electroweak scale and the large masses of the new fields. Usually, the new fields introduced have masses far above the electroweak scale, outside the reach of any for
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Bergström, Johannes. "Models in Neutrino Physics : Numerical and Statistical Studies." Doctoral thesis, KTH, Teoretisk partikelfysik, 2013. http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-127409.

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The standard model of particle physics can excellently describe the vast majorityof data of particle physics experiments. However, in its simplest form, it cannot account for the fact that the neutrinos are massive particles and lepton flavorsmixed, as required by the observation of neutrino oscillations. Hence, the standardmodel must be extended in order to account for these observations, opening up thepossibility to explore new and interesting physical phenomena. There are numerous models proposed to accommodate massive neutrinos. Thesimplest of these are able to describe the observations us
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Ohlsson, Tommy. "Dynamics of quarks and leptons : theoretical Studies of Baryons and Neutrinos." Doctoral thesis, KTH, Fysik, 2000. http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-2991.

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The Standard Model of Elementary Particle Physics (SM) is the present theoryfor the elementary particles and their interactions and is a well-established theorywithin the physics community. The SM is a combination of Quantum Chromodynamics(QCD) and the Glashow{Weinberg{Salam (GWS) electroweak model. QCDis a theory for the strong force, whereas the GWS electroweak model is a theoryfor the weak and electromagnetic forces. This means that the SM describes allfundamental forces in Nature, except for the gravitational force. However, the SMis not a nal theory and some of its problems will be discus
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Flohr, Jamin. "Massless neutrino mixing /." [St. Lucia, Qld.], 2006. http://www.library.uq.edu.au/pdfserve.php?image=thesisabs/absthe19503.pdf.

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Książki na temat "Neutrino mass and mixing"

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Winter, Klaus, and Guido Altarelli, eds. Neutrino Mass. Springer Berlin Heidelberg, 2003. http://dx.doi.org/10.1007/b13585.

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Scott, W. G. Tri-maximal vs. bi-maximal neutrino mixing. Rutherford Appleton Laboratory, 1999.

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

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Mohapatra, R. N. Massive neutrinos in physics and astrophysics. 3rd ed. World Scientific, 2005.

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Wesselingh, J. A. Mass transfer in multicomponent mixtures. Delft University Press, 2000.

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Wesselingh, J. A. Mass transfer in multicomponent mixtures. Delft Univ. Press, 2000.

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1938-, Barger V., and Cline D. 1933-, eds. Neutrino mass and low energy weak interactions, Telemark, 1984. World Scientific, 1985.

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Fujihara Seminar on Neutrino Mass and Seesaw Mechanism (2004 Kō-enerugī Kasokuki Kenkyū Kikō). Neutrino mass and seesaw mechanism: Proceedings of Fujihara Seminar on Neutrino Mass and Seesaw Mechanism : KEK, Japan, 23-25 February 2004. Elsevier, 2004.

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B, Pal P., ed. Massive neutrinos in physics and astrophysics. World Scientific, 1991.

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B, Pal P., ed. Massive neutrinos in physics and astrophysics. 3rd ed. World Scientific, 2004.

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Części książek na temat "Neutrino mass and mixing"

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Kayser, Boris. "Neutrino Mass, Mixing, and Flavor Change." In Springer Tracts in Modern Physics. Springer Berlin Heidelberg, 2003. http://dx.doi.org/10.1007/978-3-540-44901-0_1.

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Mazumder, Iffat Ara, and Rupak Dutta. "Two Minor Zeros in Neutrino Mass Matrix Using Trimaximal Neutrino Mixing." In Springer Proceedings in Physics. Springer Nature Singapore, 2025. https://doi.org/10.1007/978-981-97-7441-8_8.

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Dev, S., Radha Raman Gautam, Lal Singh, and M. M. Gupta. "Neutrino Mass Matrices with Two Texture Zeros and Near Maximal Atmospheric Neutrino Mixing." In Springer Proceedings in Physics. Springer International Publishing, 2015. http://dx.doi.org/10.1007/978-3-319-25619-1_49.

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Mahajan, Neelu. "Implications of Neutrino Mixing Data on Hierarchical Texture 2 Zero Mass Matrices." In Springer Proceedings in Physics. Springer Singapore, 2020. http://dx.doi.org/10.1007/978-981-15-6292-1_41.

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Branco, G. C., and J. I. Silva-Marcos. "Patterns for the Neutrino Mass Matrices and Mixings." In Recent Developments in Particle Physics and Cosmology. Springer Netherlands, 2001. http://dx.doi.org/10.1007/978-94-010-0676-7_3.

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Bilenky, Samoil. "Neutrino Mixing Matrix." In Introduction to the Physics of Massive and Mixed Neutrinos. Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-319-74802-3_6.

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Bilenky, Samoil. "Neutrino Mixing Matrix." In Introduction to the Physics of Massive and Mixed Neutrinos. Springer Berlin Heidelberg, 2010. http://dx.doi.org/10.1007/978-3-642-14043-3_5.

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Barger, V., and K. Whisnant. "Neutrino Mixing Schemes." In Current Aspects of Neutrino Physics. Springer Berlin Heidelberg, 2001. http://dx.doi.org/10.1007/978-3-662-04597-8_9.

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Mössbauer, Rudolf L. "Neutrino Mass." In NATO ASI Series. Springer US, 1997. http://dx.doi.org/10.1007/978-1-4899-0242-9_9.

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Deutsch, J., and R. Prieels. "Generation Mixing and Heavy Neutrinos." In Neutrino Physics. Springer Berlin Heidelberg, 1988. http://dx.doi.org/10.1007/978-3-642-73679-7_9.

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Streszczenia konferencji na temat "Neutrino mass and mixing"

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KAYSER, B. "NEUTRINO MASS, MIXING, AND OSCILLATION." In Proceedings of the Theoretical Advanced Study Institute in Elementary Particle Physics. WORLD SCIENTIFIC, 2001. http://dx.doi.org/10.1142/9789812811509_0017.

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Feruglio, Ferruccio. "What are the neutrino mass-mixing parameters telling us?" In Neutrino Oscillation Workshop. Sissa Medialab, 2017. http://dx.doi.org/10.22323/1.283.0005.

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Ma, Ernest. "Models of neutrino mass and mixing." In The fifth international conference on physics potential and development of muon colliders and neutrino factories. AIP, 2000. http://dx.doi.org/10.1063/1.1336243.

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Smirnov, Alexei Yu. "Neutrino Mass and Mixing: Leptons versus Quarks." In CAIRO INTERNATIONAL CONFERENCE ON HIGH ENERGY PHYSICS (CICHEP II). AIP, 2007. http://dx.doi.org/10.1063/1.2435284.

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Capozzi, Francesco, Eleonora Di Valentino, Eligio Lisi, Antonio Marrone, Antonio Palazzo, and Alessandro Melchiorri. "STATUS OF THREE NEUTRINO MASS AND MIXING PARAMETERS." In Nineteenth Lomonosov Conference on Elementary Particle Physics. WORLD SCIENTIFIC, 2021. http://dx.doi.org/10.1142/9789811233913_0001.

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Robertson, R. G. H. "Neutrino mass and mixing, and non-accelerator experiments." In Proceedings of the XXVI international conference on high energy physics. AIP, 1992. http://dx.doi.org/10.1063/1.43491.

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Lisi, Eligio, Francesco Capozzi, Eleonora Di Valentino, et al. "Recent topics in the analysis of neutrino mass-mixing parameters." In Corfu Summer Institute 2023 "School and Workshops on Elementary Particle Physics and Gravity". Sissa Medialab, 2024. http://dx.doi.org/10.22323/1.463.0118.

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STUCCHI, L., A. M. GAGO, and V. GUPTA. "CONSEQUENCES ON THE NEUTRINO MIXING MATRIX FROM TWO ZERO TEXTURES IN THE NEUTRINO MASS MATRIX." In Proceedings of the Fifth Latin American Symposium. WORLD SCIENTIFIC, 2006. http://dx.doi.org/10.1142/9789812773951_0040.

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FULLER, G. M. "CONSEQUENCES OF NEUTRINO MASS AND FLAVOR MIXING FOR CORE COLLAPSE SUPERNOVAE." In Open Issues in Core Collapse Supernova Theory. WORLD SCIENTIFIC, 2005. http://dx.doi.org/10.1142/9789812703446_0011.

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BALANTEKIN, A. B. "UNITARITY CONSTRAINTS ON NEUTRINO MASS AND MIXINGS." In Proceedings of the 7th International Symposium. WORLD SCIENTIFIC, 2000. http://dx.doi.org/10.1142/9789812792433_0067.

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Raporty organizacyjne na temat "Neutrino mass and mixing"

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Fuyuto, Kaori. Unraveling the origin of neutrino mass. Office of Scientific and Technical Information (OSTI), 2022. http://dx.doi.org/10.2172/1881767.

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Romosan, Alexandru. High statistics search for muon-neutrino (anti-muon-neutrino) ---> electron-neutrino (anti-electron-neutrino) oscillations in the small mixing angle regime. Office of Scientific and Technical Information (OSTI), 1996. http://dx.doi.org/10.2172/1421755.

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Bell, Nicole F., and /Fermilab. Constraints on the relic neutrino abundance and implications for cosmological neutrino mass limits. Fermi National Accelerator Laboratory (FNAL), Batavia, IL, 2004. http://dx.doi.org/10.2172/879071.

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Grossman, yuval. Neutrino masses and sneutrino mixing in R-parity violating supersymmetry. Office of Scientific and Technical Information (OSTI), 1999. http://dx.doi.org/10.2172/10100.

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Kunze, Eric. Lateral Mixing DRI Analysis: Submesoscale Water-Mass Spectra. Defense Technical Information Center, 2013. http://dx.doi.org/10.21236/ada601168.

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Elliott, Steven R. Double Beta Decay: Is the Neutrino Mass within Reach? Office of Scientific and Technical Information (OSTI), 2013. http://dx.doi.org/10.2172/1063921.

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Elliott, Steven R. Double Beta Decay, Neutrino Mass and the MAJORANA Project. Office of Scientific and Technical Information (OSTI), 2013. http://dx.doi.org/10.2172/1063922.

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Faraggi, A. E., and J. C. Pati. Meeting the constraint of neutrino-Higgsino mixing in gravity unified theories. Office of Scientific and Technical Information (OSTI), 1997. http://dx.doi.org/10.2172/466855.

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Zeller, Geralyn P. A Precise measurement of the weak mixing angle in neutrino - nucleon scattering. Office of Scientific and Technical Information (OSTI), 2002. http://dx.doi.org/10.2172/1420938.

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Farzan, Y. Effects of the Neutrino B-term on SLepton Mixing and Electric Dipole Moments. Office of Scientific and Technical Information (OSTI), 2003. http://dx.doi.org/10.2172/826458.

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