Relevant bibliographies by topics / Solar Neutrino Flux

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

Academic literature on the topic 'Solar Neutrino Flux'

Author: Grafiati
Published: 3 June 2025
Last updated: 31 July 2025

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Journal articles on the topic "Solar Neutrino Flux"

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Gutiérrez, Miguel, Manuel Masip, and Sergio Muñoz. "The Solar Disk at High Energies." Astrophysical Journal 941, no. 1 (2022): 86. http://dx.doi.org/10.3847/1538-4357/aca020.

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Abstract High energy cosmic rays illuminate the Sun and produce an image that could be observed in up to five different channels: a cosmic-ray shadow (whose energy dependence has been studied by HAWC); a gamma-ray flux (observed at E ≤ 200 GeV by Fermi-LAT); a muon shadow (detected by ANTARES and IceCube); a neutron flux (undetected, as there are no hadronic calorimeters in space); a flux of high energy neutrinos. Since these signals are correlated, the ones already observed can be used to reduce the uncertainty in the still undetected ones. Here we define a simple setup that uses the Fermi-LA
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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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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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Boyarkin, O. M., and I. O. Boyarkina. "Solar neutrinos as indicators of the Sun’s activity." International Journal of Modern Physics A 34, no. 33 (2019): 1950227. http://dx.doi.org/10.1142/s0217751x19502270.

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Opportunity of the solar flares (SFs) prediction observing the solar neutrino fluxes is investigated. In three neutrino generations, the evolution of the neutrino flux traveling the coupled sunspots (CSs) which are the SF source is considered. It is assumed that the neutrinos possess both the dipole magnetic moment and the anapole moment while the magnetic field above the CSs may reach the values [Formula: see text] Gs, display the twisting nature and posses the nonpotential character. The possible resonance conversions of the solar neutrino flux are examined. Since the [Formula: see text] res
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DEV, S., and JYOTI DHAR SHARMA. "RESOLUTION OF THE Be/B SOLAR NEUTRINO FLUX ANOMALY IN THE RESONANT SPIN-FLAVOR PRECESSION SCENARIO WITH TWISTING SOLAR MAGNETIC FIELDS." Modern Physics Letters A 15, no. 05 (2000): 351–60. http://dx.doi.org/10.1142/s0217732300000335.

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The Be/B neutrino flux anomaly has been examined within the framework of the resonant spin-flavor precession scenario with twisting solar magnetic fields. It is found that the twist of the toroidal component of the solar magnetic field, leads naturally to a complete disappearance of 7 Be neutrinos emerging from one of the solar hemispheres. However, the 7 Be neutrino flux emerging from the other solar hemisphere with oppositely twisted magnetic field must survive completely. Thus, this scenario predicts seasonal variations of the 7 Be neutrino flux to be observed in the Borexino experiment.
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DEV, S., and SANJEEV KUMAR. "CONSTRAINTS ON WEAKLY MIXED STERILE NEUTRINOS IN THE LIGHT OF SNO SALT PHASE AND 766.3 Ty KamLAND DATA." Modern Physics Letters A 20, no. 38 (2005): 2957–67. http://dx.doi.org/10.1142/s0217732305018189.

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The possibility of flavor transitions into sterile neutrinos (accompanying the dominant LMA transitions) in the solar boron neutrino flux has been examined in a scenario proposed by Hollanda and Smirnov to overcome some generic problems of the pure LMA scenario. It is found that the most recent SNO salt phase solar neutrino data and the KamLAND 766.3 Ty spectral data, allow for a significant sterile presence in the solar boron neutrino flux reaching the earth.
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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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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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Khavroshkin, O. B., and V. V. Tsyplakov. "HENRI EFFECT: REGISTRATION PARAMETERS." Metafizika, no. 4 (December 15, 2020): 67–71. http://dx.doi.org/10.22363/2224-7580-2020-4-67-71.

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The detected anomalous neutrino radioisotope (ANRI) absorption or effect allows one to study the variety of interactions of neutrino fluxes with radioactive matter and its consequences. Thus, results were obtained on solar neutrinos v , seismicity and heat flow of the Earth. The study of the features of the mechanical manifestation of the neutrino flux as a mechanical effect of the solar flux v in space on the Pioneer-type spacecraft is promising for many reasons.
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RAYCHAUDHURI, PROBHAS. "TIME VARIATIONS IN KAMIOKANDE SOLAR NEUTRINO DATA." Modern Physics Letters A 06, no. 22 (1991): 2003–7. http://dx.doi.org/10.1142/s0217732391002165.

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Solar neutrino flux (Eν ≥ 7.5 MeV ) data from 1st January to April 1990 as measured in Kamiokande solar neutrino experiment have been analyzed statistically and have found that the solar neutrino data varies with the solar activity cycle with very high statistical significance (> 98% confidence level). Average solar neutrino flux data in the sunspot minimum range cannot be equal to twice the average solar neutrino flux data in the sunspot maximum range, which suggests that the neutrino flip through the magnetic field of the convection zone of the sun is not responsible for the solar neutrin
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Dissertations / Theses on the topic "Solar Neutrino Flux"

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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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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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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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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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Bartra, Jorge Humberto Colonia. "Efeitos das ondas magnetossônicas no fluxo de neutrinos solares." [s.n.], 1996. http://repositorio.unicamp.br/jspui/handle/REPOSIP/278284.

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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 2018-07-21T03:59:05Z (GMT). No. of bitstreams: 1 Bartra_JorgeHumbertoColonia_M.pdf: 807888 bytes, checksum: d8915103e00d9fb655e3e19f2b276e51 (MD5) Previous issue date: 1996<br>Resumo: Estudamos um modelo onde ondas magnetossônicas lentas são produzidas devido a deslocamentos de plasma solar, perturbando o campo magnético no Sol. Como conseqüência, quando se supõe um momento magnético não nulo do neutrino, observam-se flutuações no fl
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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<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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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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Hussain, Asad. "Synergistic effects of neutrons and plasma on materials in fusion reactors & relaxation of merging magnetic flux ropes in fusion and solar plasmas." Thesis, University of Manchester, 2018. https://www.research.manchester.ac.uk/portal/en/theses/synergistic-effects-of-neutrons-and-plasma-on-materials-in-fusion-reactors--relaxation-of-merging-magnetic-flux-ropes-in-fusion-and-solar-plasmas(9802cf3f-f977-460c-9e9d-314e9c0e8bd5).html.

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This thesis comprises of essentially two parts. The first deals with materials in a fusion reactor and examines how neutron damage affects material in a fusion reactor, with focus on how this is important for plasma damage. The methods used are neutron transport, primary event analysis and molecular dynamics. It found that the neutron damage by 14 MeV neutrons is restricted to back scatter events within the surface (first 20 microns). Molecular dynamics analysis showed that the issue of cascades is heavily dependent on direction of primary event and the energy of such. Statistical analysis was
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Maneschg, Werner [Verfasser]. "Low-energy solar neutrino spectroscopy with Borexino : towards the detection of the solar pep and CNO neutrino flux / put forward by Werner Maneschg." 2011. http://d-nb.info/1012586359/34.

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(5929988), Shih-Chieh Liu. "Test of Decay Rate Parameter Variation due to Antineutrino Interactions." Thesis, 2019.

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High precision measurements of a weak interaction decay were conducted to search for possible variation of the decay rate parameter caused by an antineutrino flux. The experiment searched for variation of the <sup>54</sup>Mn electron capture decay rate parameter to a level of precision of 1 part in ∼10<sup>5</sup> by comparing the difference between the decay rate in the presence of an antineutrino flux ∼3×10<sup>12</sup> cm<sup>-2</sup>sec<sup>-1</sup> and no flux measurements. The experiment is located 6.5 meters from the reactor core of the High Flux Isotope Reactor (HFIR) in Oak Ridge Nati
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Book chapters on the topic "Solar Neutrino Flux"

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Singh, Govind, Ashish Sharma, Gazal Sharma, Shankita Bhardwaj, Surender Verma, and B. C. Chauhan. "Bounds on Sterile Neutrino Component in the Solar Neutrino Flux." In XXII DAE High Energy Physics Symposium. Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-319-73171-1_170.

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Bahcall, John N., Raymond Davis, Peter Parker, Alexei Smirnov, and Roger Ulrich. "Solar Neutrino Flux*." In Solar Neutrinos. CRC Press, 2018. http://dx.doi.org/10.1201/9780429502811-12.

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Reines, F., and W. R. Kropp. "Limits on Solar Neutrino Flux and Elastic Scattering*." In Solar Neutrinos. CRC Press, 2018. http://dx.doi.org/10.1201/9780429502811-35.

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Iben, Icko Jr, Kenneth Kalata, and Judah Schwartz. "The Effect of Be7 K-Capture on the Solar Neutrino Flux*." In Solar Neutrinos. CRC Press, 2018. http://dx.doi.org/10.1201/9780429502811-69.

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Reines, F., and W. R. Kropp. "LIMITS ON SOLAR NEUTRINO FLUX AND ELASTIC SCATTERING." In Neutrinos and Other Matters. WORLD SCIENTIFIC, 1991. http://dx.doi.org/10.1142/9789814343060_0041.

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Chattopadhyay, Godhuli, and Probhas Raychaudhuri. "Statistical Analysis of Solar Flare, Solar Neutrino Flux and Sunspot Data." In Physics of the Outer Heliosphere. Elsevier, 1990. http://dx.doi.org/10.1016/b978-0-08-040780-7.50066-x.

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Filippone*, B. W., A. J. Elwyn†, C. N. Davids, and D. D. Koetke. "Proton capture cross section of 7Be and the flux of high energy solar neutrinos." In Solar Neutrinos. CRC Press, 2018. http://dx.doi.org/10.1201/9780429502811-75.

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"Secondary cosmic radiation variations at ground and flight altitudes in the Czech Republic during autumn 2024." In Book of Abstracts - RAD 2025 Conference. RAD Centre, Niš, Serbia, 2025. https://doi.org/10.21175/rad.abstr.book.2025.35.12.

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Temporal variations of secondary cosmic-ray intensity reflect the intricate interplay between geophysical and solar phenomena. The amplitude of these flux changes depends on the type and energy of radiation, as well as on the geographical coordinates and the detector’s characteristics. To study the effects of space radiation on the terrestrial atmosphere, several measurement campaigns within the BIOSPHERE project have been conducted at various locations across Europe. This contribution presents results from a measurement campaign carried out in the Czech Republic during autumn 2024. Variations
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Conference papers on the topic "Solar Neutrino Flux"

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Ludwig, F., L. Wagner, T. Al-Abdullah, D. Bemmerer, and K. Zuber. "Muon flux measurement in the shallow-underground laboratory Felsenkeller." In 5th International Solar Neutrino Conference. WORLD SCIENTIFIC, 2019. http://dx.doi.org/10.1142/9789811204296_0032.

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Ding, X. F., A. Vishneva, Ö. Penek, and S. Marcocci. "GooStats Based Analytical Multivariate Analysis in Borexino Phase-II Precision Measurement of Low Energy Solar Neutrino Flux." In The 28th International Symposium on Lepton Photon Interactions at High Energies. WORLD SCIENTIFIC, 2020. http://dx.doi.org/10.1142/9789811207402_0027.

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GAI, MOSHE. "PRECISION MEASUREMENTS OF THE 7Be(p, γ)8B WITH RADIOACTIVE BEAMS AND THE 8B SOLAR NEUTRINO FLUX". У Proceedings of the Fifteenth Lake Louise Winter Institute. WORLD SCIENTIFIC, 2001. http://dx.doi.org/10.1142/9789812811752_0018.

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Kim, Y. E., M. Rabinowitz, W. D. Braswell, J. H. Yoon, R. A. Rice та A. L. Zubarev. "Condensed matter effects and new resonance parameterization for the p(p,e+νe)D and 8B solar neutrino flux". У The 14th international conference of few-body problems in physics. AIP, 1995. http://dx.doi.org/10.1063/1.48105.

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Ranucci, Gioacchino. "Results and physics implications of the precision measurement of the 7Be solar neutrino flux performed with the Borexino detector." In XXIst International Europhysics Conference on High Energy Physics. Sissa Medialab, 2012. http://dx.doi.org/10.22323/1.134.0082.

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TRINDER, W., E. G. ADELBERGER, Z. JANAS, et al. "GAMOW–TELLER STRENGTH IN THE BETA–DECAY OF 37CA AND ITS IMPLICATIONS FOR THE DETECTION OF THE SOLAR NEUTRINO FLUX." In Proceedings of the Tours Symposium on Nuclear Physics II. WORLD SCIENTIFIC, 1995. http://dx.doi.org/10.1142/9789814447058_0055.

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Gai, Moshe. "Precision measurements of the [sup 7]Be(p,γ)[sup 8]B reaction with radioactive beams and the [sup 8]B solar neutrino flux". У The tenth international symposium on capture gamma-ray spectroscopyand related topics. AIP, 2000. http://dx.doi.org/10.1063/1.1361370.

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Meer, Sneer. "New predictive impact on cancer formation related to solar neutrinos flux crossing the human body." In Aerospace/Defense Sensing, Simulation, and Controls, edited by Patrick J. Gardner. SPIE, 2001. http://dx.doi.org/10.1117/12.438188.

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Reports on the topic "Solar Neutrino Flux"

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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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Lin, Wei, and W. C. Haxton. The very low energy solar flux of electron and heavy-flavor neutrinos and antineutrinos. Office of Scientific and Technical Information (OSTI), 1994. http://dx.doi.org/10.2172/10181244.

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