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Dissertations / Theses on the topic 'Neutrino Solar'

Author: Grafiati

Published: 4 June 2021

Last updated: 1 February 2022

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1

Lyon, Matthew Jeremy. "Neutron transport in the Sudbury neutrino detector." Thesis, University of Oxford, 1996. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.337422.

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2

Miknaitis, Kathryn Kelly Schaffer. "A search for matter enhanced neutrino oscillations through measurements of day and night solar neutrino fluxes at the Sudbury Neutrino Observatory /." Thesis, Connect to this title online; UW restricted, 2005. http://hdl.handle.net/1773/9636.

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3

Laberge, Gaetan (Gaetan Joseph Henri) Carleton University Dissertation Physics. "212Pb assay for the determination of the neutral current background at the Sudbury Neutrino Observatory." Ottawa, 1995.

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4

Paterson, David John Carleton University Dissertation Physics. "Studies of a novel method for solar neutrino neutral current detection in the Sudbury neutrino observatory." Ottawa, 1989.

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5

Smith, Miles Walter Eldon. "An investigation of matter enhanced neutrino oscillation with the Sudbury Neutrino Observatory /." Thesis, Connect to this title online; UW restricted, 2002. http://hdl.handle.net/1773/9701.

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6

Wikström, Gustav. "A search for solar dark matter with the IceCube neutrino telescope." Doctoral thesis, Stockholms universitet, Fysikum, 2009. http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-27352.

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Dark matter particles in the form of supersymmetric Weakly Interacting Massive Particles (WIMPs) could accumulate in the centre of the Sun because of gravitational trapping. Pair-wise annihilations of WIMPs could create standard model particles out of which neutrinos could reach the Earth. Data from the IceCube 22-string neutrino telescope have been searched for signals from dark matter annihilations in the Sun. Highly sophisticated analysis methods have been developed to discern signal neutrinos from the severe background of atmospheric particle showers. No signal has been found in a dataset

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7

Loach, James Chilton. "Measurement of the Flux of 8B Solar Neutrinos at the Sudbury Neutrino Observatory." Thesis, University of Oxford, 2008. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.490107.

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The Sudbury Neutrino Observatory (SNO) was a heavy water Cerenkov detector that had the unique ability to measure both the total il active flux of solar neutrino, using a neutral current (NC) interaction, and the flux of electron neutrinos, using a charged current (CC) interaction. The experiment has demonstrated that neutrinos 3 change flavour and that the total neutrino flux is consistent with the prediction of solar models.

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8

Heron, Heidi. "Techniques to measure the NC background in the SNO experiment." Thesis, University of Oxford, 1998. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.244578.

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9

DeKok, Alan (Alan T. ). Carleton University Dissertation Physics. "A Process degasser for the SNO Ultra-pure light water facility." Ottawa, 1996.

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10

Cravens, J. P., K. Abe, T. Iida, et al. "Solar neutrino measurements in Super-Kamiokande-II." American Physical Society, 2008. http://hdl.handle.net/2237/11302.

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11

Bhattacharya, Atri, Rikard Enberg, Yu Seon Jeong, et al. "Prompt atmospheric neutrino fluxes: perturbative QCD models and nuclear effects." SPRINGER, 2016. http://hdl.handle.net/10150/622473.

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We evaluate the prompt atmospheric neutrino flux at high energies using three different frameworks for calculating the heavy quark production cross section in QCD: NLO perturbative QCD, k(T) factorization including low-x resummation, and the dipole model including parton saturation. We use QCD parameters, the value for the charm quark mass and the range for the factorization and renormalization scales that provide the best description of the total charm cross section measured at fixed target experiments, at RHIC and at LHC. Using these parameters we calculate differential cross sections for ch

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12

Burgess, Thomas. "A Search for Solar Neutralino Dark Matter with the AMANDA-II Neutrino Telescope." Doctoral thesis, Stockholm : Physics Department, Stockholm University, 2008. http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-7378.

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13

Thornewell, Peter Michael. "Â³He neutral current detectors for the Sudbury Neutrino Observatory." Thesis, University of Oxford, 1997. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.343004.

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14

Yeung, Alan B. (Alan Brian) Carleton University Dissertation Physics. "A Monte Carlo study of the Sudbury Neutrino Observatory small test detector experiment." Ottawa, 1990.

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15

Boardman, Robert James. "The detection of Cerenkov radiation from neutrino interactions." Thesis, University of Oxford, 1992. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.315715.

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16

Cox-Mobrand, Gary A. "Data integrity and electronic calibrations for the neutral current detector phase measurement of the 8B solar neutrino flux at the Sudbury Neutrino Observatory /." Thesis, Connect to this title online; UW restricted, 2008. http://hdl.handle.net/1773/9647.

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17

Wilson, Jeanne R. "A measurement of the â¸B solar neutrino energy spectrum at the Sudbury Neutrino Observatory." Thesis, University of Oxford, 2004. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.409729.

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18

Orebi, Gann Gabriel D. "An improved measurement of the B Solar Neutrino energy spectrum at the sudbury neutrino observatory." Thesis, University of Oxford, 2008. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.510201.

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19

Hardy, Steven. "Measuring the ⁷Be Neutrino Flux From the Sun: Calibration of the Borexino Solar Neutrino Detector." Diss., Virginia Tech, 2010. http://hdl.handle.net/10919/26728.

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The Borexino solar neutrino detector is a real-time liquid scintillator detector designed to measure sub-MeV neutrinos. With its unprecedented level of radio-purity, Borexino is poised to provide the most precise measurements to-date of solar neutrino and geo-antineutrino fluxes. However, in order to reduce the systematic errors to sub-5% levels, the detector must be care- fully calibrated to understand, among other things, the position and energy reconstructions. To that end, the Virginia Tech component of the Borexino collaboration has constructed a system for deploying and locating calib

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20

Stonehill, Laura C. "Deployment and background characterization of the Sudbury Neutrino Observatory neutral current detectors /." Thesis, Connect to this title online; UW restricted, 2005. http://hdl.handle.net/1773/9665.

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21

Heeger, Karsten Miklas. "Model-independent measurement of the neutral-current interaction rate of solar ⁸B neutrinos with deuterium in the Sudbury Neutrino Observatory /." Thesis, Connect to this title online; UW restricted, 2002. http://hdl.handle.net/1773/9774.

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22

Houdy, Thibaut. "Testing non-standard neutrino interactions from 8B solar neutrino rate measurement with Borexino to characterization of the 144Ce source of the SOX experiment." Thesis, Sorbonne Paris Cité, 2017. http://www.theses.fr/2017USPCC209/document.

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Le détecteur Borexino, situé au laboratoire souterrain du Gran Sasso (LNGS), mesure les neutrinos solaires depuis 10 ans. Parmi les neutrinos solaires, le spectre continu du 8B jusqu’à 17 MeV permet de tester la zone de transition de l’effet de résonance dans la matière dit effet MSW. Cette nouvelle analyse augmente d’un ordre de grandeur la statistique par rapport à la précédente mesure de Borexino publiée en 2011. Pour ce faire, l’ensemble du volume scintillant a été inclus dans l’analyse, aucune coupure géométrique n’ayant été effectué au dessus de 5 MeV. Cela a permis l’identification d’un

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23

Hayward, Scott Kelly. "Three neutrino oscillations applied to solar and long baseline experiments." Thesis, National Library of Canada = Bibliothèque nationale du Canada, 1998. http://www.collectionscanada.ca/obj/s4/f2/dsk2/tape15/PQDD_0031/NQ27158.pdf.

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24

Ferraris, Andrew Peter. "Radiogenic background supression in a heavy water solar neutrino detector." Thesis, University of Oxford, 1992. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.314875.

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25

Back, Henning Olling. "Internal Radioactive Source Calibration of the Borexino Solar Neutrino Experiment." Diss., Virginia Tech, 2004. http://hdl.handle.net/10919/11255.

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A measurement of solar neutrinos below 1 MeV of energy will further our knowledge of the neutrino's mass and mixing properties and will provide a probe to possible physics beyond the standard model of particle physics, as well as advance our understanding of energy production in the Sun. Borexino is a liquid scintillator detector that will measure the neutrino energy spectrum to the lowest energy threshold to date. It has been designed to measure the flux of the mono-energetic neutrinos produced by electron capture on 7Be in the Sun's core, which will produce a Compton-like edge in the energ

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26

Yokley, Zachary W. "Solar and Sterile Neutrino Physics with the Raghavan Optical Lattice." Diss., Virginia Tech, 2016. http://hdl.handle.net/10919/71330.

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The neutrino is, by its nature, an elusive particle that requires massive detectors with small backgrounds to capture a handful of events. Nevertheless, neutrino experiments stand at the heart of the current mysteries of particle physics and astrophysics. These include the origin and size of neutrino mass, the existence of additional types of neutrinos, CP violation and the matter--antimatter asymmetry, the amount of metals in the Sun's core, and the existence of non-nuclear energy sources in the Sun. This dissertation concerns the the use of a novel detector technology, the Raghavan Optical L

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27

Chen, Xin. "Monte Carlo simulations and analyses of backgrounds in the Sudbury Neutrino Observatory." Thesis, University of Oxford, 1997. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.244717.

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28

Orrell, John Laurence. "A search for an electron antineutrino signal in the Sudbury Neutrino Observatory /." Thesis, Connect to this title online; UW restricted, 2004. http://hdl.handle.net/1773/9794.

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29

Lay, Michael David. "Creation and detection of Cerenkov light in the Sudbury Neutrino Observatory." Thesis, University of Oxford, 1994. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.239323.

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30

Krofcheck, David. "Gamow-Teller strength distributions for solar neutrino detectors via the (p,n) reaction /." The Ohio State University, 1987. http://rave.ohiolink.edu/etdc/view?acc_num=osu1487327695622858.

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31

Niedermeier, Ludwig Stefan. "High efficiency purification of liquid scintillators for the solar neutrino experiment Borexino." [S.l.] : [s.n.], 2005. http://deposit.ddb.de/cgi-bin/dokserv?idn=974437638.

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32

Manecki, Szymon M. "Annual Modulation Measurement of the Low Energy Solar Neutrino Flux with the Borexino Detector." Diss., Virginia Tech, 2013. http://hdl.handle.net/10919/23250.

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This work reports a first attempt to measure the solar neutrino annual<br />flux modulation due to Earth\'s elliptical orbit with the Borexino detector. Borexino is a real-time calorimetric detector for low energy neutrino spectroscopy located in the underground laboratory of Gran Sasso, Italy. The experiment\'s main focus is the direct measurement of the 7Be solar neutrino flux of all flavors via neutrino-electron scattering in an ultra-pure scintillation liquid. The original goal of this work was to quantify sensitivity of the Borexino detector to a 7% peak-to-peak signal variation over the

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33

Bravo, Berguno David. "Precision Background Stability and Response Calibration in Borexino: Prospects for Wideband, Precision Solar Neutrino Spectroscopy and BSM Neutrino Oscillometry Through a Deeper Detector Understanding." Diss., Virginia Tech, 2016. http://hdl.handle.net/10919/73581.

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This work sets out to be a description of the initiatives utilizing the Borexino liquid scintillator neutrino observatory to perform the first direct, high-precision, wideband solar neutrino spectroscopy measurement of the the solar neutrino spectrum's main components, as well as its next-generation short-baseline source program (SOX). Its original scope revolved around the creation of a O(MCi) ⁵¹Cr source to be inserted under the detector, intended to explore the small region of the anomaly-favored sin²θ₁₄/Δm₁₄² phase space where sterile neutrinos may lie -or otherwise unambiguously measure o

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34

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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35

Holanda, Pedro Cunha de 1973. "Soluções ao problema do neutrino solar e suas predições às informações independentes do fluxo." [s.n.], 2001. http://repositorio.unicamp.br/jspui/handle/REPOSIP/278307.

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Orientador: Marcelo Moraes Guzzo<br>Tese (doutorado) - Universidade Estadual de Campinas, Instituto de Fisica Gleb Wataghin<br>Made available in DSpace on 2018-07-28T19:01:19Z (GMT). No. of bitstreams: 1 Holanda_PedroCunhade_D.pdf: 921009 bytes, checksum: 1679afe611048c21dbec6885a2706273 (MD5) Previous issue date: 2001<br>Resumo: O Problema do Neutrino Solar, caracterizado por um déficit do fluxo destes neutrinos detectado em experimentos terrestres em relação às predições teóricas, completa 30 anos sem uma explicação definitiva. Mas o atual panorama experimental propicia que diversos mecani

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36

O'Keeffe, Helen Mary. "Low energy background in the NCD phase of the Sudbury Neutrino Observatory." Thesis, University of Oxford, 2008. http://ora.ox.ac.uk/objects/uuid:b53c04b1-5dba-4cfb-98ec-c0d8b87fb58b.

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The Sudbury Neutrino Observatory (SNO) was a 1 kilotonne heavy water Č{C}erenkov detector. Evidence for flavour changing neutrino oscillations was found by comparing the rate of Charged Current interactions with that of Neutral Current (NC) interactions. This thesis is concerned with the accurate determination of the NC flux in the Neutral Current Detector (NCD) phase of SNO. The measurement and understanding of radioactive backgrounds arising from decays of naturally occurring $^{232}$Th and $^{238}$U chain nuclei is crucial. This is because their daughter nuclei can produce neutrons via phot

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37

Clémentine, Vulliet. "Study Of Non-Standard Interaction Effects On The Solar Neutrino Day-Night Asymmetry." Thesis, KTH, Teoretisk fysik, 2015. http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-161648.

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38

Blennow, Mattias. "Matter and damping effects in neutrino mixing and oscillations." Licentiate thesis, Stockholm, 2005. http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-301.

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39

Dalnoki-Veress, Ferenc J. R. Carleton University Dissertation Physics. "Investigation of the triggered source technique for the calibration of SNO." Ottawa, 1996.

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40

Silva, Flavio Maux Vianna da. "Estudo do fluxo de neutrino solar com o c?digo evolutivo de Toulouse - Geneva." Universidade Federal do Rio Grande do Norte, 2014. http://repositorio.ufrn.br:8080/jspui/handle/123456789/18607.

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Made available in DSpace on 2015-03-03T15:15:30Z (GMT). No. of bitstreams: 1 FlavioMVS_DISSERT.pdf: 786675 bytes, checksum: 15c59d932af3a41769e781bb08d4e3e9 (MD5) Previous issue date: 2014-04-24<br>Coordena??o de Aperfei?oamento de Pessoal de N?vel Superior<br>The study of solar neutrinos is very important to a better comprehension of the set of nuclear reactions that occurs inside the Sun and in solar type stars. The ux of neutrinos provides a better comprehension of the stellar structure as a whole. In this dissertation we study the ux of neutrinos in a solar model, addressing the

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41

Lanfranchi, Jean-Côme. "Development of a new composite cryogenic detection concept for a radiochemical solar neutrino experiment." [S.l.] : [s.n.], 2005. http://deposit.ddb.de/cgi-bin/dokserv?idn=979098238.

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42

Wagner, Louis. "Precise nuclear data of the 14N(p,gamma)15O reaction for solar neutrino predictions." Helmholtz-Zentrum Dresden-Rossendorf, 2018. https://tud.qucosa.de/id/qucosa%3A31122.

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The 14N(p,gamma)15O reaction is the slowest stage of the carbon-nitrogen-oxygen cycle of hydrogen burning and thus determines its reaction rate. Precise knowledge of its rate is required to improve the model of hydrogen burning in our sun. The reaction rate is a necessary ingredient for a possible solution of the solar abundance problem that led to discrepancies between predictions of the solar standard model and helioseismology. The solar 13N and 15O neutrino fluxes are used as independent observables that probe the carbon and nitrogen abundances in the solar core. This could settle the disag

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43

Watson, L. Scott. "Solar models including revised abundances and dark matter : constraints from helioseismology and neutrino observations." Thesis, University of Oxford, 2007. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.491613.

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This thesis presents several topics in both standard and non-standard solar models using the Iben Stellar Evolution Code. First, a set of standard solar models are developed using the abundance determination of Grevesse & Noels (1993) and the more recent determination of Asplund et al. (2005a,b). This recent solar photospheric abundance analysis reduces the abundances of heavy elements, most notably C, N, 0, Ne and Ar, by 0.15 to 0.20 dex, lowering the solar Z/X to 0.0165, compared to the previous Grevesse & Noels value of Z/X = 0.0245. A comparison study between these models show evolutions b

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44

Wiebe, Klaus [Verfasser]. "All-flavor based searches for solar dark matter with the IceCube Neutrino Observatory / Klaus Wiebe." Mainz : Universitätsbibliothek Mainz, 2017. http://d-nb.info/1124030700/34.

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45

Rabaey, Gregory Francis. "The observed properties of the intermediate-degree gravity modes and their relevance to the solar neutrino paradox." Diss., The University of Arizona, 1989. http://hdl.handle.net/10150/184730.

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Intermediate-degree g-modes (those with angular order ℓ ≈ 30) were first observed in the late 1970's by Hill and Caudell (1979). However, it wasn't until 1986 that a preliminary survey was made of the 1979 differential radius observations (see Bos 1982) and a set of 4 multiplets exhibiting mode-locking was classified by Hill (1986). These multiplets with angular order ℓ ≈ 30 and eigenfrequencies of ≈350 μHz were used as a starting point for the comprehensive analysis discussed in this work. This comprehensive study culminated in the classification of a set of 20 intermediate-degree g-mode mult

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46

Möllenberg, Randolph Verfasser], Lothar [Akademischer Betreuer] Oberauer, and Shawn [Akademischer Betreuer] [Bishop. "Monte Carlo Study of Solar 8B Neutrinos and the Diffuse Supernova Neutrino Background in LENA / Randolph Möllenberg. Gutachter: Shawn Bishop ; Lothar Oberauer. Betreuer: Lothar Oberauer." München : Universitätsbibliothek der TU München, 2013. http://d-nb.info/1045730149/34.

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47

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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48

Zoll, Marcel Christian Robert. "A search for solar dark matter with the IceCube neutrino detector : Advances in data treatment and analysis technique." Doctoral thesis, Stockholms universitet, Fysikum, 2016. http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-125341.

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There is compelling observational evidence for the existence of dark matter in the Universe, including our own Galaxy, which could possibly consist of weakly interacting massive particles (WIMPs) not contained in the standard model (SM) of particle physics. WIMPs may get gravitationally trapped inside heavy celestial bodies of ordinary matter. The Sun is a nearby candidate for such a capture process which is driven by the scattering of WIMPs on its nuclei. Forming an over-density at the Sun's core the WIMPs would self-annihilate yielding energetic neutrinos, which leave the Sun and can be dete

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49

Rountree, Steven Derek. "Science and Technology of a Low-Energy Solar Neutrino Spectrometer (LENS) and Development of the MiniLENS Underground Prototype." Diss., Virginia Tech, 2010. http://hdl.handle.net/10919/27803.

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A real time low energy spectral measurement of the neutrinos coming from the Sun will give us a greater understanding of energy production in the Sun, and the mechanisms of neutrino mixing. We will, for the first time, measure the solar neutrino spectrum for all solar neutrinos <2MeV in particular pp, Be and CNO neutrinos, be able to compare the solar photon derived energy luminosity (Lï §) to the solar neutrino derived energy luminosity (Lï ®) independent of any solar model, explore dark energy with respect to mass varying neutrinos, and explore CNO abundances in the Sun. These measurements

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50

Valdiviesso, Gustavo do Amaral. "Introdução à fenomenologia da oscilação de neutrinos, no vácuo e na matéria." [s.n.], 2004. http://repositorio.unicamp.br/jspui/handle/REPOSIP/278301.

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Orientador: Marcelo Moraes Guzzo<br>Dissertação (mestrado) - Universidade Estadual de Campinas, Instituto de Fisica Gleb Wataghin<br>Made available in DSpace on 2018-08-09T11:03:28Z (GMT). No. of bitstreams: 1 Valdiviesso_GustavodoAmaral_M.pdf: 1768172 bytes, checksum: d1861e9e1805a2a55abc030dde4bf22b (MD5) Previous issue date: 2004<br>Resumo: O objetivo deste trabalho é produzir um texto didático que sirva como base para alunos de física, ao ingressarem na área da fenomenologia de neutrinos. Introduz-se o modelo de mistura de neutrinos no vácuo, baseado no conceito de superposição de estado

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