Relevant bibliographies by topics / Neutrino Solar

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

Academic literature on the topic 'Neutrino Solar'

Author: Grafiati
Published: 4 June 2021
Last updated: 1 February 2022

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Journal articles on the topic "Neutrino Solar"

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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 (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
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Ankush, Rishu Verma, Gazal Sharma, and B. C. Chauhan. "Investigating Sterile Neutrino Flux in the Solar Neutrino Data." Advances in High Energy Physics 2019 (June 2, 2019): 1–12. http://dx.doi.org/10.1155/2019/2598953.

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There are compelling evidences for the existence of a fourth degree of freedom of neutrinos, i.e., sterile neutrino. In the recent studies the role of sterile component of neutrinos has been found to be crucial, not only in particle physics, but also in astrophysics and cosmology. This has been proposed to be one of the potential candidates of dark matter. In this work we investigate the updated solar neutrino data available from all the relevant experiments including Borexino and KamLAND solar phase in a model independent way and obtain bounds on the sterile neutrino component present in the
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KWONG, WAIKWOK, and S. P. ROSEN. "THE SOLAR NEUTRINO PROBLEM AND BOUNDS ON SOLAR NEUTRINO FLUXES." Modern Physics Letters A 10, no. 19 (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 b
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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 t
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BELLERIVE, A. "REVIEW OF SOLAR NEUTRINO EXPERIMENTS." International Journal of Modern Physics A 19, no. 08 (2004): 1167–79. http://dx.doi.org/10.1142/s0217751x04019093.

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This paper reviews the constraints on the solar neutrino mixing parameters with data collected by the Homestake, SAGE, GALLEX, Kamiokande, SuperKamiokande, and SNO experiments. An emphasis will be given to the global solar neutrino analyses in terms of matter-enhanced oscillation of two active flavors. The results to-date, including both solar model dependent and independent measurements, indicate that electron neutrinos are changing to other active types on route to the Earth from the Sun. The total flux of solar neutrinos is found to be in very good agreement with solar model calculations. F
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Miramonti, Lino, Matteo Agostini, Konrad Altenmueller, et al. "Solar Neutrinos Spectroscopy with Borexino Phase-II." Universe 4, no. 11 (2018): 118. http://dx.doi.org/10.3390/universe4110118.

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Solar neutrinos have played a central role in the discovery of the neutrino oscillation mechanism. They still are proving to be a unique tool to help investigate the fusion reactions that power stars and further probe basic neutrino properties. The Borexino neutrino observatory has been operationally acquiring data at Laboratori Nazionali del Gran Sasso in Italy since 2007. Its main goal is the real-time study of low energy neutrinos (solar or originated elsewhere, such as geo-neutrinos). The latest analysis of experimental data, taken during the so-called Borexino Phase-II (2011-present), wil
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Minakata, H., and C. Peña-Garay. "Solar Neutrino Observables Sensitive to Matter Effects." Advances in High Energy Physics 2012 (2012): 1–15. http://dx.doi.org/10.1155/2012/349686.

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We discuss constraints on the coefficientAMSWwhich is introduced to simulate the effect of weaker or stronger matter potential for electron neutrinos with the current and future solar neutrino data. The currently available solar neutrino data leads to a boundAMSW=1.47+0.54−0.42(+1.88−0.82)at 1σ(3σ) CL, which is consistent with the Standard Model predictionAMSW=1. For weaker matter potential (AMSW<1), the constraint which comes from the flat8B neutrino spectrum is already very tight, indicating the evidence for matter effects. However for stronger matter potential (AMSW>1), the bound is m
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PAL, PALASH B. "PARTICLE PHYSICS CONFRONTS THE SOLAR NEUTRINO PROBLEM." International Journal of Modern Physics A 07, no. 22 (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 magn
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KLEIN, JOSHUA R. "SOLAR NEUTRINO RESULTS FROM THE SUDBURY NEUTRINO OBSERVATORY." International Journal of Modern Physics A 17, no. 24 (2002): 3378–92. http://dx.doi.org/10.1142/s0217751x0201279x.

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We describe here the measurement of the flux of neutrinos created by the decay of solar 8B by the Sudbury Neutrino Observatory (SNO). The neutrinos were detected via the charged current (CC) reaction on deuterium and by the elastic scattering (ES) of electrons. The CC reaction is sensitive exclusively to νe's, while the ES reaction also has a small sensitivity to νμ's and ντ's. The flux of νe's from 8B decay measured by the CC reaction rate is [Formula: see text]. Assuming no flavor transformation, the flux inferred from the ES reaction rate is [Formula: see text]. Comparison of ϕ CC (νe) to t
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Schramm, D. N., and X. Shi. "Solar neutrinos: Solar physics and neutrino physics." Nuclear Physics B - Proceedings Supplements 35 (May 1994): 321–33. http://dx.doi.org/10.1016/0920-5632(94)90271-2.

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Dissertations / Theses on the topic "Neutrino Solar"

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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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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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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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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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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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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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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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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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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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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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Books on the topic "Neutrino Solar"

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L, Bergström, ed. Neutrino physics: Proceedings of Nobel Symposium 129 : Haga Slott, Enköping, Sweden, August 19-24, 2004. World Scientific, 2005.

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Germany) International Solar Neutrino Conference (4th 1997 Heidelberg. Proceedings of the Fourth International Solar Neutrino Conference, Heidelberg, Germany, April 8-11, 1997. Max-Planck-Institut für Kernphysik, 1997.

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Neutrino Oscillation Workshop (2004 Otranto, Italy). NOW 2004: Proceedings of the Neutrino Oscillation Workshop, Conca Specchiulla, Otranto, Italy, 11-17 September 2004. Elsevier, 2005.

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Neutrino Oscillation Workshop (2004 Otranto, Italy). NOW 2004: Proceedings of the Neutrino Oscillation Workshop : Conca Specchiulla, Otranto, Italy, 11-17 September 2004. Elsevier, 2005.

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

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Workshop on Neutrino Oscillations and their Origin (1st 2000 Fujiyoshida, Japan). Neutrino oscillations and their origin: Proceedings of the 1st Workshop on Neutrino Oscillations and their Origin, held on February 11-13, 2000, in Japan. Universal Academy Press, 2000.

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Confronting nature: The sociology of solar-neutrino detection. D. Reidel Pub. Co, 1986.

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Davini, Stefano. Measurement of the pep and CNO Solar Neutrino Interaction Rates in Borexino. Springer International Publishing, 2014. http://dx.doi.org/10.1007/978-3-319-01213-1.

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Boulay, Mark Guy. A new test of extraction efficiency for the homestake solar neutrino experiment. Laurentian University Press, 1996.

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1933-, Cline D., ed. Observational neutrino astronomy: Proceedings of the Workshop on Extra Solar Neutrino Astronomy : University of California, Los Angeles 30 Sept. - 2 Oct. 1987. World Scientific, 1988.

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Book chapters on the topic "Neutrino Solar"

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Zuber, Kai. "Solar neutrinos." In Neutrino Physics. CRC Press, 2020. http://dx.doi.org/10.1201/9781315195612-10.

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Davini, Stefano. "Solar Neutrino Observations." In Measurement of the pep and CNO Solar Neutrino Interaction Rates in Borexino. Springer International Publishing, 2013. http://dx.doi.org/10.1007/978-3-319-01213-1_2.

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Spiro, M., and D. Vignaud. "Solar Neutrino Projects." In Inside the Sun. Springer Netherlands, 1990. http://dx.doi.org/10.1007/978-94-009-0541-2_15.

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Gough, Douglas. "Solar Neutrino Production." In International Conference on Theoretical Physics. Birkhäuser Basel, 2003. http://dx.doi.org/10.1007/978-3-0348-7907-1_24.

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Mössbauer, Rudolf L. "The Solar Neutrino Puzzle." In The Superworld III. Springer US, 1990. http://dx.doi.org/10.1007/978-1-4684-8869-2_12.

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

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Suzuki, Yoichiro, and Kunio Inoue. "Indium Solar Neutrino Experiments." In Physics and Astrophysics of Neutrinos. Springer Japan, 1994. http://dx.doi.org/10.1007/978-4-431-67029-2_10.

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

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Valle, J. W. F. "Weak Interactions and Solar Neutrinos: Testing the Oscillation Hypothesis." In Neutrino Physics. Springer Berlin Heidelberg, 1988. http://dx.doi.org/10.1007/978-3-642-73679-7_26.

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Hampel, W. "The Present Status of the Gallium Solar Neutrino Detector GALLEX." In Neutrino Physics. Springer Berlin Heidelberg, 1988. http://dx.doi.org/10.1007/978-3-642-73679-7_23.

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Conference papers on the topic "Neutrino Solar"

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Ranucci, G. "Low-Energy Neutrino Experiments (Solar Neutrinos)." In The 28th International Symposium on Lepton Photon Interactions at High Energies. WORLD SCIENTIFIC, 2020. http://dx.doi.org/10.1142/9789811207402_0007.

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Wang, Zhe. "Prospects of solar neutrino study in Jinping Neutrino Experiment." In 5th International Solar Neutrino Conference. WORLD SCIENTIFIC, 2019. http://dx.doi.org/10.1142/9789811204296_0022.

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Lande, Kenneth. "The Beginning of Neutrino Astronomy — The Homestake Solar Neutrino Detector." In 5th International Solar Neutrino Conference. WORLD SCIENTIFIC, 2019. http://dx.doi.org/10.1142/9789811204296_0001.

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Fargion, Daniele, Pietro Oliva, P. G. De Sanctis Lucentini, et al. "Solar neutrino flare, megaton neutrino detectors and human space journey." In 5th International Solar Neutrino Conference. WORLD SCIENTIFIC, 2019. http://dx.doi.org/10.1142/9789811204296_0025.

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PETCOV, S. T. "SOLAR NEUTRINO OSCILLATIONS." In Proceedings of the Sixth School. WORLD SCIENTIFIC, 2002. http://dx.doi.org/10.1142/9789812777492_0002.

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Miramonti, Lino. "Solar Neutrino Detection." In 4th School on Cosmic Rays and Astrophysics. Sissa Medialab, 2011. http://dx.doi.org/10.22323/1.118.0030.

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Miramonti, Lino, Carlos Javier Solano Salinas, Jose Bellido, David Wahl, and Oscar Saavedra. "Solar neutrino detection." In COSMIC RAYS AND ASTROPHYSICS: Proceedings of the 3rd School on Cosmic Rays and Astrophysics. AIP, 2009. http://dx.doi.org/10.1063/1.3141352.

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Gonzalez-Garcia, M. C. "Solar Neutrino Oscillations." In Proceedings of the Third International Workshop. WORLD SCIENTIFIC, 2002. http://dx.doi.org/10.1142/9789812776488_0007.

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Fujita, Y. "Nuclei as neutrino detectors." In 5th International Solar Neutrino Conference. WORLD SCIENTIFIC, 2019. http://dx.doi.org/10.1142/9789811204296_0009.

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Wurm, M., M. Agostini, K. Altenmüller, et al. "Solar neutrino spectroscopy in Borexino." In 5th International Solar Neutrino Conference. WORLD SCIENTIFIC, 2019. http://dx.doi.org/10.1142/9789811204296_0016.

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Reports on the topic "Neutrino Solar"

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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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Bowles, T. J., S. J. Brice, E. I. Esch, et al. Solar Neutrino Physics. Office of Scientific and Technical Information (OSTI), 1999. http://dx.doi.org/10.2172/759169.

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

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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), 1994. http://dx.doi.org/10.2172/10191828.

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

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Bruggen, M., W. C. Haxton, and Y. Z. Qian. Landau-Zener treatments of solar neutrino oscillations. Office of Scientific and Technical Information (OSTI), 1995. http://dx.doi.org/10.2172/10108392.

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Elliott, S. R., J. F. Wilkerson, and J. N. Abdurashitov. The Russian-American gallium solar neutrino experiment. Office of Scientific and Technical Information (OSTI), 1995. http://dx.doi.org/10.2172/88574.

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Pal, P. B. Particle physics confronts the solar neutrino problem. Office of Scientific and Technical Information (OSTI), 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), 1994. http://dx.doi.org/10.2172/10155794.

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