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Relevant bibliographies by topics / Solar neutrino problem

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Academic literature on the topic 'Solar neutrino problem'

Author: Grafiati

Published: 4 June 2021

Last updated: 27 April 2022

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Journal articles on the topic "Solar neutrino problem"

1

KWONG, WAIKWOK, and S. P. ROSEN. "THE SOLAR NEUTRINO PROBLEM AND BOUNDS ON SOLAR NEUTRINO FLUXES." Modern Physics Letters A 10, no. 19 (June 21, 1995): 1331–49. http://dx.doi.org/10.1142/s0217732395001460.

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We review the current status of the solar neutrino problem. A survey of the experiments and their results are given, and solar physics crucial to the understanding of these results are discussed. Semi-empirical methods are used to derive bounds on the fluxes of the three most important components (pp, 7Be and 8B) of the solar neutrino spectrum. The 8B neutrinos are directly measured to be about half of the theoretical prediction. Relative to their theoretical predictions, we find the 7Be neutrinos to be highly suppressed and the pp neutrinos not suppressed. We are also able to derive a lower bound on the pp flux.

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PAL, PALASH B. "PARTICLE PHYSICS CONFRONTS THE SOLAR NEUTRINO PROBLEM." International Journal of Modern Physics A 07, no. 22 (September 10, 1992): 5387–459. http://dx.doi.org/10.1142/s0217751x92002465.

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This review has four parts. In Part I, we describe the reactions that produce neutrinos in the sun and the expected flux of those neutrinos on the earth. We then discuss the detection of these neutrinos, and how the results obtained differ from the theoretical expectations, leading to what is known as the solar neutrino problem. In Part II, we show how neutrino oscillations can provide a solution to the solar neutrino problem. This includes vacuum oscillations, as well as matter enhanced oscillations. In Part III, we discuss the possibility of time variation of the neutrino flux and how a magnetic moment of the neutrino can explain the phenomenon. We also discuss particle physics models which can give rise to the required values of magnetic moments. In Part IV, we present some concluding remarks and outlook for the near future.

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Hargrove, C. K., and D. J. Paterson. "Solar-neutrino neutral-current detection methods in the Sudbury neutrino observatory." Canadian Journal of Physics 69, no. 11 (November 1, 1991): 1309–16. http://dx.doi.org/10.1139/p91-196.

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The Sudbury Neutrino Observatory will study the solar-neutrino problem through the detection of charged-current (CC), neutral-current (NC), and elastic-scattering (ES) interactions of solar neutrinos with heavy water. The measurement of the NC rate relative to the CC rate provides a nearly model-independent method of observing neutrino oscillations. The NC interaction breaks up the deuteron producing a neutron and a proton. The interaction rate in the original design is measured by observing Čerenkov light from showers produced by neutron-capture γ rays from the capture of the NC neutrons by a selected additive to the heavy water. These signals overlap the CC and ES signals, so that the measurement of the NC rate requires the subtraction of two signals obtained at different times. This paper describes our investigation of an alternate detection method in which the thermalized neutrons are captured by (n, α) or (n, p) reactions on light nuclei. The resulting charged-particle products are uniquely detected by scintillators or proportional counters, completely separating this NC signal from the CC and ES Čerenkov signals, thus simplifying its measurement, improving its significance, and allowing observation of otherwise unobservable short-term NC fluctuations. Although background rates for the new techniques have not yet been determined, the experimental advantages justify further development work.

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Spiro, M., and D. Vignaud. "Solar Neutrino Projects." International Astronomical Union Colloquium 121 (1990): 157–69. http://dx.doi.org/10.1017/s0252921100067919.

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AbstractAn overview of the solar neutrino projects is given, with an emphasis on the complementarity of the different experiments (gallium, indium, heavy water,...) to solve the solar neutrino problem that was raised by the chlorine and the Kamiokande results. The separation of the different sources of neutrinos in the Sun would contribute significantly to the astrophysical understanding of the Sun. Some of the planned experiments could be able to pinpoint neutrino oscillations (within a wide range of parameters) almost independently of solar models. Projects which are particularly sensitive to a variation of the neutrino flux with time are also discussed.

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Haxton, W. C. "The Solar Neutrino Problem." Annual Review of Astronomy and Astrophysics 33, no. 1 (September 1995): 459–503. http://dx.doi.org/10.1146/annurev.aa.33.090195.002331.

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Bahcall, John N. "The Solar-Neutrino Problem." Scientific American 262, no. 5 (May 1990): 54–61. http://dx.doi.org/10.1038/scientificamerican0590-54.

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Hampel, Wolfgang. "A solar neutrino problem?" Physics World 3, no. 9 (September 1990): 20–21. http://dx.doi.org/10.1088/2058-7058/3/9/18.

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Konijn, J. "The solar neutrino problem." European Journal of Physics 20, no. 6 (November 1, 1999): 399–407. http://dx.doi.org/10.1088/0143-0807/20/6/305.

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Prosper, Harrison B. "The solar neutrino problem." Pramana 54, no. 4 (April 2000): 611–22. http://dx.doi.org/10.1007/s12043-000-0154-6.

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de Sabbata, V., and C. Sivaram. "The solar-neutrino problem." Il Nuovo Cimento A 104, no. 10 (October 1991): 1577–79. http://dx.doi.org/10.1007/bf02817440.

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Dissertations / Theses on the topic "Solar neutrino problem"

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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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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 para transições entre neutrinos ativos, e entre neutrinos ativos e estéreis. Nossos resultados mostraram que ambas soluções são consistentes com os dados de neutrinos solares e, também, no caso específico do quase-vácuo, observamos que a hipótese de três gerações ficou desfavorecida.
This thesis presents a well detailed statistical analysis using the recent data from solar neutrino experiments. This analysis was done in the framework of two different solutions of neutrino oscillations, both characterized by a long oscillation wavelength. The first was based on the standard mass induced oscillation mechanism, here we worked in the scheme of two and three neutrino generations within the quasivacuum regime. The second was an exotic mechanism, where the neutrino oscillation is due to a possible breakdown of the equivalence principle, this alternative was analyzed only for two neutrino generations, in the cases for the conversion among active neutrino and active to sterile neutrino. Our results show a good agreement between the solar neutrino data and both solutions, also in the specific case of quasivacuum, we found that the hypothesis for the three neutrino generation is disfavored.

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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
Tese (doutorado) - Universidade Estadual de Campinas, Instituto de Fisica Gleb Wataghin
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
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 mecanismos envolvendo física nova para o neutrino forneçam uma solução aceitável ao Problema do Neutrino Solar. A proliferação destas possíveis soluções é devida em parte aos resultados negativos obtidos por um detector em particular, o Super-Kamiokande, ao tentar confirmar esta física nova através de análises independentes do fluxo total de neutrinos. Estas análises de informações independentes do uxo foram propostas com o objetivo de distinguir entre as possíveis soluções para o Problema do Neutrino Solar. Um resultado positivo destas análises indicaria qual dessas várias soluções é a correta. Um resultado negativo, contudo, não é suficiente para descartar nenhuma delas. Apesar disso, estes resultados contribuiram para enriquecer o campo de estudos do problema do neutrino solar, que se apresenta como uma janela para diversos mecanismos envolvendo uma física além do modelo padrão
Abstract: The Solar Neutrino Problem, which is a neutrino flux supression from the theoretical predictions detected in terrestrial experiments, has completed 30 years old without a final explanation. But the actual experimental data leaves us with a number of mechanisms involving new physics in the neutrino sector that can produce acceptable solutions to the Solar Neutrino Problem. The large amount of possible solutions is to some extent due to the negative results of the Super-Kamiokande experiment in its ux-independent analysis. This analysis was first proposed in order to discriminate between the possible solar neutrino problem solutions. A positive result would point to a specific solution, but negative results would not be able to eliminate any one. In spite of that, the SK results contributed to the solar neutrino physics field, which presents itself as a window to physics beyond the standard model
Doutorado
Física
Doutor em Ciências

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Kernan, Peter John. "Two astroparticle physics problems : solar neutrinos, and primordial 4[superscript]Helium /." The Ohio State University, 1993. http://rave.ohiolink.edu/etdc/view?acc_num=osu1487846354482934.

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Books on the topic "Solar neutrino problem"

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Sakurai, Kunitomo. Solar neutrino problems: How they were solved. Tokyo: Terrapub, 2014.

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United States. National Aeronautics and Space Administration., ed. E leptoquarks and the solar neutrino problem. [Batavia, Ill.?]: Fermi National Accelerator Laboratory, 1991.

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Ellam, Rob. Isotopes. Oxford University Press, 2016. http://dx.doi.org/10.1093/actrade/9780198723622.001.0001.

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An isotope is a variant form of a chemical element, containing a different number of neutrons in its nucleus. Most elements exist as several isotopes. Many are stable, others are radioactive, and some may only exist fleetingly before decaying into other elements. The study of isotope ratios has become central to many areas of science, and used to probe the age and history of the Earth and the origins of the Solar System. Radioactive isotopes find wide applications, from nuclear power to medicine and carbon dating. Isotopes: A Very Short Introduction provides an overview of the nature of stable and radioactive isotopes, considering their wide range of modern applications.

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Book chapters on the topic "Solar neutrino problem"

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Bahcall, John N. "The Solar Neutrino Problem." In Progress in Solar Physics, 53–63. Dordrecht: Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-4588-3_3.

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Haxton, W. C. "Neutrino Oscillations and the Solar Neutrino Problem." In Current Aspects of Neutrino Physics, 65–88. Berlin, Heidelberg: Springer Berlin Heidelberg, 2001. http://dx.doi.org/10.1007/978-3-662-04597-8_4.

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Antia, H. M., and S. M. Chitre. "Helioseismology and the Solar Neutrino Problem." In New Eyes to See Inside the Sun and Stars, 41–42. Dordrecht: Springer Netherlands, 1998. http://dx.doi.org/10.1007/978-94-011-4982-2_6.

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Newman, Michael J. "The Solar Neutrino Problem: Gadfly for Solar Evolution Theory." In Physics of the Sun, 33–45. Dordrecht: Springer Netherlands, 1986. http://dx.doi.org/10.1007/978-94-009-5255-3_2.

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Takata, M., and H. Shibahashi. "Seismic Solar Models and the Neutrino Problem." In New Eyes to See Inside the Sun and Stars, 21–24. Dordrecht: Springer Netherlands, 1998. http://dx.doi.org/10.1007/978-94-011-4982-2_3.

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Roxburgh, Ian W. "Helioseismic Constraints on Solar Structure and the Solar Neutrino Problem." In The Non-Sleeping Universe, 57–58. Dordrecht: Springer Netherlands, 1999. http://dx.doi.org/10.1007/978-94-011-4497-1_15.

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Spergel, David. "The Missing Mass and the Solar Neutrino Problem." In Dark Matter in the Universe, 496. Dordrecht: Springer Netherlands, 1987. http://dx.doi.org/10.1007/978-94-009-4772-6_98.

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Nozawa, S., Y. Kohyama, and K. Kubodera. "Exchange Currents in the Neutrino-Deuteron Reaction and the Solar Neutrino Problem." In Weak and Electromagnetic Interactions in Nuclei, 747–49. Berlin, Heidelberg: Springer Berlin Heidelberg, 1986. http://dx.doi.org/10.1007/978-3-642-71689-8_146.

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Rothstein, I. Z. "A Solution to the Time Varying Solar Neutrino Problem." In Physics at the Highest Energy and Luminosity, 279–302. Boston, MA: Springer US, 1992. http://dx.doi.org/10.1007/978-1-4615-3402-0_9.

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Haubold, H. J., and A. M. Mathai. "The Solar Neutrino Problem as a Probe for Nuclear Astrophysics." In Weak and Electromagnetic Interactions in Nuclei, 745–46. Berlin, Heidelberg: Springer Berlin Heidelberg, 1986. http://dx.doi.org/10.1007/978-3-642-71689-8_145.

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Conference papers on the topic "Solar neutrino problem"

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Villante, F. L., and A. Serenelli. "An updated discussion of the solar abundance problem." In 5th International Solar Neutrino Conference. WORLD SCIENTIFIC, 2019. http://dx.doi.org/10.1142/9789811204296_0005.

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Kaniadakis, G., A. Lavagno, M. Lissia, and P. Quarati. "The solar neutrino problem and Tsallis statistics." In Fifth Rio de Janeiro International Workshop. WORLD SCIENTIFIC, 1998. http://dx.doi.org/10.1142/9789814528917_0010.

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LIU, WEIPING, XIXIANG BAI, SHUHUA ZHOU, ZHANWEN MA, ZHICHANG LI, YOUBAO WANG, ANLI LI, et al. "SOLAR NEUTRINO PROBLEM RELATED NUCLEAR PHYSICS EXPERIMENTS." In Proceedings of the International Symposium. WORLD SCIENTIFIC, 2003. http://dx.doi.org/10.1142/9789812791276_0012.

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D'Olivo, Juan Carlos. "VEP Oscillation Solutions to the Solar Neutrino Problem." In Third Latin American Symposium on High Energy Physics. Trieste, Italy: Sissa Medialab, 2000. http://dx.doi.org/10.22323/1.005.0006.

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Bolaños, A., Luis Manuel Montaño Zetina, Gabino Torres Vega, Miguel Garcia Rocha, Luis F. Rojas Ochoa, and Ricardo Lopez Fernandez. "The solar neutrino problem and Non Standard Interactions." In FRONTIERS IN CONTEMPORARY PHYSICS. AIP, 2008. http://dx.doi.org/10.1063/1.3040263.

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POON, A. W. P. "SOLVING THE SOLAR NEUTRINO PROBLEM 2 km UNDERGROUND — THE SUDBURY NEUTRINO OBSERVATORY." In Proceedings of the 8th Conference. WORLD SCIENTIFIC, 2004. http://dx.doi.org/10.1142/9789812702708_0019.

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NUNOKAWA, HIROSHI. "EXOTIC SOLUTIONS TO THE SOLAR NEUTRINO PROBLEM AND SOME IMPLICATIONS FOR LOW ENERGY SOLAR NEUTRINO EXPERIMENTS." In Proceedings of the 2nd International Workshop. WORLD SCIENTIFIC, 2002. http://dx.doi.org/10.1142/9789812778000_0002.

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Miranda, O. G. "Resonant-Spin Flavour solutions to the Solar neutrino Problem." In PARTICLES AND FIELDS: Eight Mexican Workshop. AIP, 2002. http://dx.doi.org/10.1063/1.1489740.

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SMY, M. B. "A UNIQUE OSCILLATION SOLUTION TO THE SOLAR NEUTRINO PROBLEM?" In Proceedings of the Third International Workshop. WORLD SCIENTIFIC, 2002. http://dx.doi.org/10.1142/9789812776488_0006.

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MARCUCCI, LAURA ELISA. "WEAK PROTON CAPTURE ON 3He AND THE SOLAR NEUTRINO PROBLEM." In A Festschrift in Honour of the 65th Birthdays of John W Clark, Alpo J Kallio, Manfred L Ristig and Sergio Rosati. WORLD SCIENTIFIC, 2001. http://dx.doi.org/10.1142/9789812799760_0014.

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Reports on the topic "Solar neutrino problem"

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Akhmedov, E. Kh. Neutrino magnetic moments and the solar neutrino problem. Office of Scientific and Technical Information (OSTI), August 1994. http://dx.doi.org/10.2172/10177402.

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Pal, P. B. Particle physics confronts the solar neutrino problem. Office of Scientific and Technical Information (OSTI), June 1991. http://dx.doi.org/10.2172/10144522.

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Pal, P. B. Particle physics confronts the solar neutrino problem. Office of Scientific and Technical Information (OSTI), June 1991. http://dx.doi.org/10.2172/5297278.

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Smirnov, A. Y. The solar neutrino problem: Neither astrophysics nor oscillations? Office of Scientific and Technical Information (OSTI), June 1994. http://dx.doi.org/10.2172/10155794.

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Friedland, Alexander. Towards the resolution of the solar neutrino problem. Office of Scientific and Technical Information (OSTI), August 2000. http://dx.doi.org/10.2172/767627.

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Krastev, P. I., and A. Y. Smirnov. Boron neutrino flux and the MSW solution of the solar neutrino problem. Office of Scientific and Technical Information (OSTI), October 1994. http://dx.doi.org/10.2172/10191828.

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Bahcall, J. N., C. A. Barnes, J. Christensen-Dalsgaard, B. T. Cleveland, S. Degl'Innocenti, B. W. Filippone, A. Glasner, et al. Has a standard model solution to the solar neutrino problem been found? Office of Scientific and Technical Information (OSTI), August 1994. http://dx.doi.org/10.2172/10176840.

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West, G. B. Dark matter and the solar neutrino problem: Can particle physics provide a single solution. Office of Scientific and Technical Information (OSTI), January 1989. http://dx.doi.org/10.2172/5556822.

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