Relevant bibliographies by topics / Solar Neutrino Observatory

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

Academic literature on the topic 'Solar Neutrino Observatory'

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

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Journal articles on the topic "Solar Neutrino Observatory"

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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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KLEIN, JOSHUA R. "SOLAR NEUTRINO RESULTS FROM THE SUDBURY NEUTRINO OBSERVATORY." International Journal of Modern Physics A 17, no. 24 (September 30, 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 the Super-Kamiokande Collaboration's precision value of ϕ ES (νx) yields a 3.3σ difference, assuming the systematic uncertainties are normally distributed, providing evidence that there is non-electron flavor active neutrino component in the solar flux. The total flux of active 8B neutrinos is thus determined to be 5.44 ± 0.99 × 106 cm- 2s- 1, in close agreement with the predictions of solar models.
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Miramonti, Lino, Matteo Agostini, Konrad Altenmueller, Simon Appel, Victor Atroshchenko, Zara Bagdasarian, Davide Basilico, et al. "Solar Neutrinos Spectroscopy with Borexino Phase-II." Universe 4, no. 11 (November 7, 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), will be showcased in this talk—yielding new high-precision, simultaneous wide band flux measurements of the four main solar neutrino components belonging to the “pp” fusion chain (pp, pep, 7 Be, 8 B), as well as upper limits on the remaining two solar neutrino fluxes (CNO and hep).
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Gavrin, V. N., A. I. Abazov, D. N. Abdurashitov, O. L. Anosov, O. V. Bychuk, S. N. Danshin, L. A. Eroshkina, et al. "The Baksan Gallium Solar Neutrino Experiment." International Astronomical Union Colloquium 121 (1990): 201–12. http://dx.doi.org/10.1017/s0252921100067956.

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AbstractA radiochemical 71Ga−71 Ge experiment to determine the integral flux of neutrinos from the sun has been constructed at the Baksan Neutrino Observatory in the USSR. Measurements have begun with 30 tonnes of gallium. The experiment is being expanded with the addition of another 30 tonnes. The motivation, experimental procedures, and present status of this experiment are presented.
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DUNCAN, F. A. "RESULTS FROM THE PURE D2O PHASE OF THE SUDBURY NEUTRINO OBSERVATORY." International Journal of Modern Physics A 18, no. 22 (September 10, 2003): 3789–807. http://dx.doi.org/10.1142/s0217751x0301718x.

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The Sudbury Neutrino Observatory is a 1000 T D2O Cerenkov detector that is sensitive to 8 B and hep solar neutrinos. Both Charged Current and Neutral Current interaction rates on deuterons as well as the Elastic Scattering interaction rate on electrons can be measured simultaneously. Assuming an undistorted 8 B neutrino spectrum, the total flux measured with the NC reaction is [Formula: see text], which is consistent with solar models. The νe component of the 8 B solar flux is [Formula: see text] for a kinetic energy threshold of 5 MeV. The non-νe component is [Formula: see text], which is 5.3σ greater than zero, giving strong evidence for solar νe flavor transformation. The Day-Night Asymmetry for the Charged Current interaction is [Formula: see text]. If the total flux of active neutrinos is additionally constrained to have no asymmetry, the νe asymmetry is found to be [Formula: see text]. Combined with other solar neutrino data, a global MSW oscillation analysis strongly favors the Large Mixing Angle (LMA) solution.
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Schever, M. "Status of the Jiangmen Underground Neutrino Observatory." Ukrainian Journal of Physics 64, no. 7 (September 17, 2019): 635. http://dx.doi.org/10.15407/ujpe64.7.635.

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The Jiangmen Underground Neutrino Observatory (JUNO) is a next generation multipurpose antineutrino detector currently under construction in Jiangmen, China. The central detector, containing 20 kton of a liquid scintillator, will be equipped with ∼18 000 20 inch and 25 600 3 inch photomultiplier tubes. Measuring the reactor antineutrinos of two powerplants at a baseline of 53 km with an unprecedented energy resolution of 3%/√︀E(MeV), the main physics goal is to determine the neutrino mass hierarchy within six years of run time with a significance of 3–4q. Additional physics goals are the measurement of solar neutrinos, geoneutrinos, supernova burst neutrinos, the diffuse supernova neutrino background, and the oscillation parameters sin2 O12, Δm212, and |Δm2ee| with a precision <1%, as well as the search for proton decays. The construction is expected to be completed in 2021.
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Lawson, I. T. "Solar neutrino results from the sudbury neutrino observatory." Progress in Particle and Nuclear Physics 48, no. 1 (January 2002): 5–20. http://dx.doi.org/10.1016/s0146-6410(02)00103-5.

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Lawson, I. "Solar neutrino results from the sudbury neutrino observatory." Nuclear Physics B - Proceedings Supplements 110, no. 2 (July 2002): 308–10. http://dx.doi.org/10.1016/s0920-5632(02)80137-2.

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Miramonti, Lino. "Status and the perspectives of the Jiangmen Underground Neutrino Observatory (JUNO)." Modern Physics Letters A 35, no. 09 (March 13, 2020): 2030004. http://dx.doi.org/10.1142/s0217732320300049.

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One of the remaining undetermined fundamental aspects in neutrino physics is the determination of the neutrino mass hierarchy, i.e. discriminating between the two possible orderings of the mass eigenvalues, known as Normal and Inverted Hierarchies. The Jiangmen Underground Neutrino Observatory (JUNO), a 20 kt Liquid Scintillator Detector currently under construction in the South of China, can determine the neutrino mass hierarchy and improve the precision of three oscillation parameters by one order of magnitude. Moreover, thanks to its large liquid scintillator mass, JUNO will also contribute to study neutrinos from non-reactor sources such as solar neutrinos, atmospheric neutrinos, geoneutrinos, supernova burst and diffuse supernova neutrinos. Furthermore, JUNO will also contribute to nucleon decay studies. In this work, I will describe the status and the perspectives of the JUNO experiment.
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Rott, Carsten. "Progress in neutrino astronomy." Journal of the Korean Physical Society 78, no. 10 (March 19, 2021): 864–72. http://dx.doi.org/10.1007/s40042-021-00106-1.

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AbstractThe dream of observing our universe through neutrinos is rapidly becoming a reality. More than three decades after the first observation of neutrinos from beyond our solar system associated with Supernova SN1987A, neutrino astronomy is in the midst of a revolution. Extraterrestrial neutrinos are now routinely detected, following the discovery of a high-energy diffuse astrophysical neutrino flux in 2013. The detection of a high-energy neutrino in coincidence with a flaring blazar in 2017 has brought the field rapidly into the multi-messenger science era. The latest developments in the field of neutrino astronomy are reviewed and prospects with current and future detectors discussed. Particular emphasis is put on domestic programs in neutrino astronomy and the possibility to construct a large neutrino observatory in Korea.
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Dissertations / Theses on the topic "Solar Neutrino Observatory"

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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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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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Thornewell, Peter Michael. "³He 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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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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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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9

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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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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Books on the topic "Solar Neutrino Observatory"

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Dragowsky, Michael Raymond. Sudbury Neutrino Observatory energy calibration using gamma-ray sources. 1999.

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Book chapters on the topic "Solar Neutrino Observatory"

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Ewan, George. "Solar Neutrino Measurements at the SUDBURY Neutrino Observatory." In Beyond the Desert 2003, 279–91. Berlin, Heidelberg: Springer Berlin Heidelberg, 2004. http://dx.doi.org/10.1007/978-3-642-18534-2_19.

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Ewan, G. T. "Sudbury Neutrino Observatory." In Solar Neutrinos, 133–35. CRC Press, 2018. http://dx.doi.org/10.1201/9780429502811-44.

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Bahcall, John N., Raymond Davis, Peter Parker, Alexei Smirnov, and Roger Ulrich. "Measurement of the Rate of ve + d→p + p + e- Interactions Produced by 8B Solar Neutrinos at the Sudbury Neutrino Observatory." In Solar Neutrinos, 451–56. CRC Press, 2018. http://dx.doi.org/10.1201/9780429502811-121.

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Maneira, J. "Combined Analysis of all Three Phases of Solar Neutrino Data from the Sudbury Neutrino Observatory." In Astroparticle, Particle, Space Physics, Radiation Interaction, Detectors and Medical Physics Applications, 360–66. WORLD SCIENTIFIC, 2012. http://dx.doi.org/10.1142/9789814405072_0052.

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Conference papers on the topic "Solar Neutrino Observatory"

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KLEIN, JOSHUA R. "SOLAR NEUTRINO RESULTS FROM THE SUDBURY NEUTRINO OBSERVATORY." In Proceedings of the XX International Symposium on Lepton and Photon Interactions at High Energies. WORLD SCIENTIFIC, 2002. http://dx.doi.org/10.1142/9789812777881_0031.

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Oblath, Noah, Ricardo Alarcon, Philip L. Cole, Chaden Djalali, and Fernando Umeres. "Precision Solar Neutrino Measurements with the Sudbury Neutrino Observatory." In VII Latin American Symposium on Nuclear Physics and Applications. AIP, 2007. http://dx.doi.org/10.1063/1.2813811.

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Balantekin, A. B., and F. Loreti. "Solar antineutrino detection at Sudbury Neutrino Observatory." In Intersections between particle and nuclear physics. AIP, 1992. http://dx.doi.org/10.1063/1.41482.

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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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De Wasseige, Gwenhaël, Paul Evenson, Kael Hanson, Nick van Eijndhoven, and Karl-Ludwig Klein. "Evaluation of expected solar flare neutrino events in the IceCube observatory." In The 34th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2016. http://dx.doi.org/10.22323/1.236.1049.

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EJIRI, H., T. ITAHASHI, T. SHIMA, R. HAZAMA, Y. IKEGAMI, K. MATSUOKA, H. NAKAMURA, et al. "MOON(MO OBSERVATORY OF NEUTRINOS) FOR NEUTRINO STUDIES BY DOUBLE BETA DECAYS AND LOW ENERGY SOLAR NEUTRINOS." In Proceedings of the Fourth International Workshop. WORLD SCIENTIFIC, 2004. http://dx.doi.org/10.1142/9789812703101_0038.

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De Wasseige, Gwenhaël. "First search for GeV neutrinos from bright gamma-ray solar flares using the IceCube Neutrino Observatory." In 36th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2019. http://dx.doi.org/10.22323/1.358.1075.

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KLAPDOR-KLEINGROTHAUS, H. V. "NEW UNDERGROUND NEUTRINO OBSERVATORY — GENIUS— IN THE NEW MILLENIUM : FOR SOLAR NEUTRINOS, DARK MATTER AND DOUBLE BETA DECAY." In Proceedings of the 2nd International Workshop. WORLD SCIENTIFIC, 2002. http://dx.doi.org/10.1142/9789812778000_0013.

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Hazama, Ryuta, Hiroyasu Ejiri, Jonathan Engel, Plamen Krastev, Nobuyuki Kudomi, Masaharu Nomachi, and R. G. Hamish Robertson. "MOON (Mo Observatory Of Neutrinos) for neutrino studies in [sup 100]Mo by double beta decays and solar-ν capture reactions." In NUCLEAR PHYSICS IN THE 21st CENTURY:International Nuclear Physics Conference INPC 2001. AIP, 2002. http://dx.doi.org/10.1063/1.1470263.

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Ryan, J., D. Forrest, J. Lockwood, M. Loomis, M. McConnell, D. Morris, W. Webber, et al. "COMPTEL gamma ray and neutron measurements of solar flares." In COMPTON GAMMA-RAY OBSERVATORY. AIP, 1993. http://dx.doi.org/10.1063/1.44245.

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Journal articles Dissertations / Theses
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