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Radioactive sources presented annual periodical half-life changes in several accurate measurements, although customary practice claims that radioactive decay should be a physical constant for each radionuclide. Besides that, the Purdue…

核实验 · 物理学 2020-02-26 Jonathan Walg , Anatoly Rodnianski , Itzhak Orion

Neutrinos generated during solar flares remain elusive. However, after $50$ years of discussion and search, the potential knowledge unleashed by their discovery keeps the search crucial. Neutrinos associated with solar flares provide…

太阳与恒星天体物理 · 物理学 2020-10-12 K. Okamoto , Y. Nakano , S. Masuda , Y. Itow , M. Miyake , T. Terasawa , S. Ito , M. Nakahata

Recently, Jenkins, et al. have reported the detection of correlations between fluctuations in nuclear decay rates and Earth-Sun distance, which suggest that nuclear decay rates can be affected by solar activity. In this paper, we report the…

天体物理学 · 物理学 2010-07-07 Jere H. Jenkins , Ephraim Fischbach

Since the end of the eighties and in response to a reported increase in the total neutrino flux in the Homestake experiment in coincidence with solar flares, solar neutrino detectors have searched for solar flare signals. Even though these…

高能天体物理现象 · 物理学 2015-05-22 G. de Wasseige , K. Hanson , N. van Eijndhoven , P. Evenson , K. -L. Klein

The deacay rate of three different radioactive sources 40K, 137Cs and natTh has been measured with NaI and Ge detectors. Data have been analyzed to search for possible variations in coincidence with the two strongest solar flares of the…

核实验 · 物理学 2015-06-12 E. Bellotti , C. Broggini , G. Di Carlo , M. Laubenstein , R. Menegazzo

The physics-based method of forecasting the high energy solar flares (SFs) with the help of the neutrino detectors utilizing the coherent elastic neutrino-nucleus scattering (CE$\nu$NS) is considered. The behavior of the neutrino beams…

太阳与恒星天体物理 · 物理学 2023-08-01 Oleg Boyarkin , Iren Boyarkina

To foresee a solar flare neutrino signal we infer its upper and lower bound. The upper bound was derived since a few years by general energy equipartition arguments on observed solar particle flare. The lower bound, the most compelling one…

天体物理学 · 物理学 2010-04-21 Daniele Fargion , Paola Di Giacomo

The neutrino flux from the sun is predicted to have a CNO-cycle contribution as well as the known pp-chain component. Previously, only the fluxes from beta+ decays of 13N, 15O, and 17F have been calculated in detail. Another neutrino…

高能物理 - 唯象学 · 物理学 2009-11-10 L. C. Stonehill , J. A. Formaggio , R. G. H. Robertson

Largest Solar Neutrino Flare may be soon detectable by Deep Core neutrino detector immediately and comunicate to satellites or astronauts. Its detection is the fastest manifestation of a later (tens minutes,hours) dangerous cosmic shower.…

太阳与恒星天体物理 · 物理学 2015-05-28 Daniele Fargion

Intense solar flares originated in sun spots produce high energy particles (protons, $\alpha$) well observable by satellites and ground-based detectors. The flare onset produces signals in different energy bands (radio, X, gamma and…

高能物理 - 唯象学 · 物理学 2009-11-10 D. Fargion

Neutrinos associated with solar flares (solar-flare neutrinos) provide information on particle acceleration mechanisms during the impulsive phase of solar flares. We searched using the Super-Kamiokande detector for neutrinos from solar…

太阳与恒星天体物理 · 物理学 2022-10-27 K. Okamoto , K. Abe , Y. Hayato , K. Hiraide , K. Hosokawa , K. Ieki , M. Ikeda , J. Kameda , Y. Kanemura , Y. Kaneshima , Y. Kataoka , Y. Kashiwagi , S. Miki , S. Mine , M. Miura , S. Moriyama , Y. Nagao , M. Nakahata , Y. Nakano , S. Nakayama , Y. Noguchi , K. Sato , H. Sekiya , K. Shimizu , M. Shiozawa , H. Shiba , Y. Sonoda , Y. Suzuki , A. Takeda , Y. Takemoto , A. Takenaka , H. Tanaka , S. Watanabe , T. Yano , S. Han , T. Kajita , K. Okumura , T. Tashiro , T. Tomiya , X. Wang , J. Xia , S. Yoshida , G. D. Megias , P. Fernandez , L. Labarga , N. Ospina , B. Zaldivar , B. W. Pointon , E. Kearns , J. L. Raaf , L. Wan , T. Wester , J. Bian , N. J. Griskevich , W. R. Kropp , S. Locke , M. B. Smy , H. W. Sobel , V. Takhistov , A. Yankelevich , J. Hill , J. Y. Kim , S. H. Lee , I. T. Lim , D. H. Moon , R. G. Park , B. Bodur , K. Scholberg , C. W. Walter , A. Beauchene , L. Bernard , A. Coffani , O. Drapier , S. El Hedri , A. Giampaolo , Th. A. Mueller , A. D. Santos , P. Paganini , B. Quilain , T. Ishizuka , T. Nakamura , J. S. Jang , J. G. Learned , K. Choi , S. Cao , L. H. V. Anthony , D. Martin , M. Scott , A. A. Sztuc , Y. Uchida , V. Berardi , M. G. Catanesi , E. Radicioni , N. F. Calabria , L. N. Machado , G. De Rosa , G. Collazuol , F. Iacob , M. Lamoureux , M. Mattiazzi , L. Ludovici , M. Gonin , G. Pronost , C. Fujisawa , Y. Maekawa , Y. Nishimura , M. Friend , T. Hasegawa , T. Ishida , T. Kobayashi , M. Jakkapu , T. Matsubara , T. Nakadaira , K. Nakamura , Y. Oyama , K. Sakashita , T. Sekiguchi , T. Tsukamoto , N. Bhuiyan , T. Boschi , G. T. Burton , F. Di Lodovico , J. Gao , A. Goldsack , T. Katori , J. Migenda , M. Taani , Z. Xie , S. Zsoldos , Y. Kotsar , H. Ozaki , A. T. Suzuki , Y. Takeuchi , S. Yamamoto , C. Bronner , J. Feng , T. Kikawa , M. Mori , T. Nakaya , R. A. Wendell , K. Yasutome , S. J. Jenkins , N. McCauley , P. Mehta , A. Tarrant , K. M. Tsui , Y. Fukuda , Y. Itow , H. Menjo , K. Ninomiya , J. Lagoda , S. M. Lakshmi , M. Mandal , P. Mijakowski , Y. S. Prabhu , J. Zalipska , M. Jia , J. Jiang , C. K. Jung , C. Vilela , M. J. Wilking , C. Yanagisawa , M. Harada , H. Ishino , S. Ito , H. Kitagawa , Y. Koshio , W. Ma , F. Nakanishi , N. Piplani , S. Sakai , G. Barr , D. Barrow , L. Cook , S. Samani , D. Wark , A. Holin , F. Nova , J. Y. Yang , J. E. P. Fannon , M. Malek , J. M. McElwee , O. Stone , M. D. Thiesse , L. F. Thompson , H. Okazawa , S. B. Kim , E. Kwon , J. W. Seo , I. Yu , A. K. Ichikawa , K. D. Nakamura , S. Tairafune , K. Nishijima , M. Koshiba , K. Iwamoto , K. Nakagiri , Y. Nakajima , S. Shima , N. Taniuchi , M. Yokoyama , K. Martens , P. de Perio , M. R. Vagins , M. Kuze , S. Izumiyama , M. Inomoto , M. Ishitsuka , H. Ito , T. Kinoshita , R. Matsumoto , Y. Ommura , N. Shigeta , M. Shinoki , T. Suganuma , K. Yamauchi , J. F. Martin , H. A. Tanaka , T. Towstego , R. Akutsu , R. Gaur , V. Gousy-Leblanc , M. Hartz , A. Konaka , X. Li , N. W. Prouse , S. Chen , B. D. Xu , B. Zhang , M. Posiadala-Zezula , S. B. Boyd , D. Hadley , M. Nicholson , M. O'Flaherty , B. Richards , A. Ali , B. Jamieson , J. Walker , Ll. Marti , A. Minamino , G. Pintaudi , S. Sano , R. Sasaki , S. Suzuki , K. Wada

More than 40 years ago, neutrinos where conceived as a way to test the validity of the solar models which tell us that stars are powered by nuclear fusion reactions. The first measurement of the neutrino flux, in 1968 in the Homestake mine…

高能物理 - 实验 · 物理学 2009-05-12 Lino Miramonti

Limiting ourselves to two flavor approximation the motion of the neutrino flux in the solar matter and twisting magnetic field is considered. For the neutrino system described by the 4-component wave function $\Psi^T = (\nu_{eL}, \nu_{XL},…

高能物理 - 唯象学 · 物理学 2016-10-26 O. M. Boyarkin , G. G. Boyarkina

Power-spectrum analyses of the decay rates of certain nuclides reveal (at very high confidence levels) an annual oscillation and periodicities that may be attributed to solar rotation and to solar r-mode oscillations. A comparison of…

高能物理 - 唯象学 · 物理学 2013-01-17 Peter Sturrock , Ephraim Fischbach , Daniel Javorsek , Jere Jenkins , Robert Lee

Results obtained with multichannel installation created for long-term studies of various processes, are collated with the data published by J.H. Jenkins and E.Fischbach, who found a decrease of 54Mn radioactivity near the time of series of…

综合物理 · 物理学 2010-06-14 A. G. Parkhomov

The Fermi Lab Liquid ARgon experiment, FLARE, a huge neutrino argon-liquid project detector of 50 kt mass, might in a near future enlarge the neutrino telescope accuracy revealing in detail solar, supernova, atmospheric as well as largest…

天体物理学 · 物理学 2007-05-23 D. Fargion

Since the end of the eighties, in response to a reported increase of the total neutrino flux in the Homestake experiment in coincidence with solar flares, neutrino detectors have searched for signals of neutrinos associated with solar flare…

高能天体物理现象 · 物理学 2016-06-03 G. de Wasseige

Spacecraft observations in the inner heliosphere offer the first opportunity to measure 1-10 MeV solar neutrons. We discuss the physics of low-energy neutron production in solar flares and show that, even at interacting-particle energies of…

太阳与恒星天体物理 · 物理学 2015-01-16 Gerald H. Share , Ronald J. Murphy , Allan J. Tylka , Benz Kozlovsky , James M. Ryan , Chul Gwon

Solar neutrinos coming from different nuclear reactions are now detected with a high statistics. Consequently, an accurate spectroscopic analysis of the neutrino fluxes arriving on the Earth's detectors become available, in the context of…

太阳与恒星天体物理 · 物理学 2013-02-13 Ilídio Lopes , Sylvaine Turck-Chièze
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