Relevant bibliographies by topics / Interaction antineutrino electron

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  1. Journal articles
  2. Dissertations / Theses
  3. Book chapters

Academic literature on the topic 'Interaction antineutrino electron'

Author: Grafiati
Published: 4 June 2021
Last updated: 5 February 2022

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Journal articles on the topic "Interaction antineutrino electron"

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Dzhioev, Alan A., and Gabriel Martínez-Pinedo. "Skyrme-RPA study of charged-current neutrino opacity in hot and dense supernova matter." EPJ Web of Conferences 194 (2018): 02006. http://dx.doi.org/10.1051/epjconf/201819402006.

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Neutrino emission and their transport of energy to the supernova shock region are sensitive to the physics of hot and dense nuclear matter, which is a complex problem due to the strong correlations induced by nuclear forces. We derive charged-current opacities for electron neutrinos and antineutrinos in supernova matter using a self-consistent approach based on the Skyrme effective interaction. We include a mean field energy shift due to nuclear interaction and corrections due to RPA correlations. A complete treatment of the full Skyrme interaction, including a spin-orbit term, is given. To te
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Ferdiyan, Akmal, and Urip Nurwijayanto Prabowo. "CROSS SECTION OF ELECTRON ANTINEUTRINO INTERACTION WITH 40AR AND 84KR AND ITS RELEVANCE TO GEONEUTRINO DETECTION." Jurnal Neutrino 13, no. 1 (2021): 25–30. http://dx.doi.org/10.18860/neu.v13i1.10602.

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Neutrino can carry information from places that cannot be reached by the usual detection mechanism because it has a very weak interaction with matter. This can be utilized to study the heat flow process inside the earth by using information carried by geoneutrino (electron antineutrino). In this sense, it is important to know the characteristics of neutrino interaction with materials. In this study, the cross-section calculation of the electron antineutrino interaction with Ar-40 and Kr-84 was carried out using computational methods with the help of GENIE software. In the energy range of 0-10
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WIETFELDT, F. E. "THE ELECTRON–ANTINEUTRINO ANGULAR CORRELATION IN FREE NEUTRON DECAY." Modern Physics Letters A 20, no. 24 (2005): 1783–96. http://dx.doi.org/10.1142/s0217732305017895.

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Free neutron beta decay is the simplest nuclear beta decay and the prototype charged-current semileptonic decay. It has some theoretical advantage over other nuclear decay systems in that there are no nuclear structure corrections, and it is the only mixed Fermi/Gamow–Teller beta decay for which the relative matrix elements can be directly calculated. The status of the electron–antineutrino angular correlation (a-coefficient) in neutron beta decay and its role in elucidating fundamental properties of the weak interaction are reviewed, with an emphasis on experiments. A new generation of experi
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NABI, JAMEEL-UN. "NEUTRINO AND ANTINEUTRINO ENERGY LOSS RATES IN MASSIVE STARS DUE TO ISOTOPES OF TITANIUM." International Journal of Modern Physics E 19, no. 01 (2010): 63–77. http://dx.doi.org/10.1142/s0218301310014716.

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Weak interaction rates on titanium isotopes are important during the late phases of evolution of massive stars. A search was made for key titanium isotopes from available literature and a microscopic calculation of weak rates of these nuclei were performed using the proton-neutron quasiparticle random phase approximation (pn-QRPA) theory. Earlier the author presented the stellar electron capture rates on titanium isotopes. In this paper I present the neutrino and antineutrino energy loss rates due to capture and decay rates on isotopes of titanium in stellar environment. Accurate estimate of n
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Faessler, Amand, Rastislav Hodák, Sergey Kovalenko, and Fedor Šimkovic. "Can one measure the Cosmic Neutrino Background?" International Journal of Modern Physics E 26, no. 01n02 (2017): 1740008. http://dx.doi.org/10.1142/s0218301317400080.

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The Cosmic Microwave Background (CMB) yields information about our Universe at around 380,000 years after the Big Bang (BB). Due to the weak interaction of the neutrinos with matter, the Cosmic Neutrino Background (CNB) should give information about a much earlier time of our Universe, around one second after the BB. Probably, the most promising method to “see” the CNB is the capture of the electron neutrinos from the Background by Tritium, which then decays into 3He and an electron with the energy of the the [Formula: see text]-value [Formula: see text] 18.562[Formula: see text]keV plus the e
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Khatun, Amina, Adam Smetana, and Fedor Šimkovic. "Three Flavor Quasi-Dirac Neutrino Mixing, Oscillations and Neutrinoless Double Beta Decay." Symmetry 12, no. 8 (2020): 1310. http://dx.doi.org/10.3390/sym12081310.

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The extension of the Standard model by three right-handed neutrino fields exhibit appealing symmetry between left-handed and right-handed sectors, which is only violated by interactions. It can accommodate three flavor quasi-Dirac neutrino mixing scheme, which allows processes with violation of both lepton flavor and total lepton number symmetries. We propose a 6×6 unitary matrix for parameterizing the mixing among three flavors of quasi-Dirac neutrino. This mixing matrix is constructed by two 3×3 unitary matrices that diagonalizes the Dirac mass term in the Lagrangian. By only assuming the St
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BARRANCO, J., A. BOLAÑOS, E. A. GARCÉS, O. G. MIRANDA, and T. I. RASHBA. "TENSORIAL NSI AND UNPARTICLE PHYSICS IN NEUTRINO SCATTERING." International Journal of Modern Physics A 27, no. 25 (2012): 1250147. http://dx.doi.org/10.1142/s0217751x12501473.

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We have analyzed the electron antineutrino scattering off electrons and the electron antineutrino–nuclei coherent scattering in order to obtain constraints on tensorial couplings. We have studied the formalism of nonstandard interactions (NSI) as well as the case of unparticle physics. For our analysis we have focused on the recent TEXONO collaboration results and we have obtained current constraints to possible electron antineutrino–electron tensorial couplings in both new physics formalisms. The possibility of measuring electron antineutrino–nucleus coherent scattering for the first time and
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Parkhomov, Alexander G., and Roman V. Karabanov. "LENR as a manifestation of weak nuclear interactions. New approach to creating LENR reactors." Radioelectronics. Nanosystems. Information Technologies. 13, no. 1 (2021): 45–58. http://dx.doi.org/10.17725/rensit.2021.13.045.

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Hypothesis is suggested about the generation of neutrino-antineutrino pairs in collisions of particles of matter at temperatures of several thousand degrees. Particularly intense generation should occur in metals and dense plasma. Resulting neutrinos and antineutrinos can excite exothermic nuclear reactions in the surrounding matter. A number of experiments were carried out that confirmed the energy release predicted by the hypothesis in a substance near a metal heated to a high temperature. The source of the neutrino-antineutrino (hot metal or dense plasma) can be separated from the "fuel " -
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Martellini, Cristina, Stefano Maria Mari, Paolo Montini, and Giulio Settanta. "Towards a reconstruction of Supernova Neutrino Spectra in JUNO." EPJ Web of Conferences 209 (2019): 01012. http://dx.doi.org/10.1051/epjconf/201920901012.

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Observation of supernovae (SN) through their neutrino emission is a fundamental point to understand both SN dynamics and neutrino physical properties. JUNO is a 20kton liquid scintillator detector, under construction in Jiangmen, China. The main aim of the experiment is to determine neutrino mass hierarchy by precisely measuring the energy spectrum of reactor electron antineutrinos. However due to its properties, JUNO has the capability of detecting a high statistics of SN events too. Existing data from SN neutrino consists only of 24 events coming from the SN 1987A,the detection of a SN burst
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Alikhanov, Ibragim, and Emmanuel Paschos. "A Light Mediator Relating Neutrino Reactions." Universe 7, no. 7 (2021): 204. http://dx.doi.org/10.3390/universe7070204.

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The extension of the standard model with a multiplicative U(1)R factor is consistent with a light vector boson. In its simplest realization, only right-handed particles carry charges of the new group. In this model, there is a residual τ3R symmetry and one new coupling constant which correlates neutrino interactions. We compute new contributions to antineutrino–electron scattering and coherent scattering on nuclei, and compare them with the XENON1T result.
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Dissertations / Theses on the topic "Interaction antineutrino electron"

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BON, NGUYEN ROMUALD. "Etude de la diffusion Ve-e auprès de la tranche 5 du centre de production nucléaire du Bugey : simulation de l'expérience MUNU de mesure du moment magnétique du neutrino." Université Joseph Fourier (Grenoble), 1997. http://www.theses.fr/1997GRE10173.

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L'experience munu a pour but la mesure du moment magnetique du neutrino grace a l'etude de la diffusion antineutrino electronique-electron aupres d'un reacteur nucleaire. Cette these presente le travail de simulation par la methode monte-carlo de l'experience munu. Cette simulation a permis de mettre en evidence les parametres ayant une influence sur les grandeurs observables de l'experience (moment magnetique, angle de weinberg, parametres decrivant les oscillations de neutrinos) ainsi que de preciser la sensibilite a ces grandeurs. En particulier, il apparait que munu permet d'obtenir une li
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Southwell, Luke. "Selecting electron antineutrino charged-current interactions at the T2K ND280." Thesis, Lancaster University, 2016. http://eprints.lancs.ac.uk/81386/.

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The contamination from ν ̄e in the T2K antineutrino beam is predicted to be approximately 1% and needs to be evaluated in order to constrain the systematic uncertainties in a T2K antineutrino oscillation measurement. In this thesis we present a ν ̄e charged-current selection with which we test the Monte Carlo predic- tion using T2K data. To select ν ̄e charged-current events, the tracker region and electromagnetic calorimeters of the T2K off-axis near detector are used. The selected sample has a ν ̄e purity of (41.9±2.4)% and an efficiency of (27.1± 1.7)%. The data to Monte Carlo ratio for ν ̄
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Roncin, Romain. "From the measurement of the θ₁₃ mixing angle to the search for geo-neutrinos : studying electron antineutrinos with Double Chooz and Borexino". Paris 7, 2014. http://www.theses.fr/2014PA077141.

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Double Chooz est une expérience d'oscillation de neutrinos de réacteur qui a pour but de mesurer l'angle de mélange θ₁₃ grâce à deux détecteurs identiques situés à différentes distances des deux réacteurs de la centrale nucléaire de Chooz, dans les Ardennes françaises. Tandis que le détecteur proche commencera à prendre des données à l'automne 2014 afin de normaliser le flux des neutrinos émis par les réacteurs nucléaires, le détecteur lointain fonctionne depuis avril 2011 et permet d'observer la disparition des neutrinos à travers le phénomène d'oscillation de neutrinos. Cette thèse est égale
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Hourlier, Adrien. "Background studies for electron anti-neutrino oscillations measurement at the Double Chooz experiment." Thesis, Sorbonne Paris Cité, 2016. http://www.theses.fr/2016USPCC192/document.

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L’expérience Double Chooz étudie les anti-neutrinos électroniques provenant de réacteurs nucléaires pour mesurer le paramètre de mélange θ13 dans le phénomène d’oscillation des neutrinos. Deux détecteurs souterrains identiques sont placés à différentes distances des réacteurs de la centrale de Chooz dans les Ardennes. Le Détecteur Lointain est entré en service en avril 2011, et le Détecteur Proche en janvier 2015. Cette thèse présente une analyse des phases simple et double détecteurs de l’expérience. Les neutrinos sont détectés par désintégration β inverse dans Double Chooz, où un positron et
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Book chapters on the topic "Interaction antineutrino electron"

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Kündig, W., M. Fritschi, E. Holzschuh, J. W. Petersen, R. E. Pixley, and H. Stüssi. "An Upper Limit for the Electron Antineutrino Mass." In Weak and Electromagnetic Interactions in Nuclei. Springer Berlin Heidelberg, 1986. http://dx.doi.org/10.1007/978-3-642-71689-8_154.

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JENKINS, T. L., F. E. KINARD, and F. REINES. "Electron Antineutrino Interaction with Deuterons." In Neutrinos and Other Matters. WORLD SCIENTIFIC, 1991. http://dx.doi.org/10.1142/9789814343060_0026.

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