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Related papers: Antineutrinos from Earth: A reference model and it…

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We report on the feasibility of using an isotropic flux of cosmic neutrinos in the energy range of 10 to 10,000 TeV to study the interior geophysical structure of the Earth. The angular distribution of events in a $\sim {\rm km}^3$-scale…

Astrophysics · Physics 2007-05-23 John P. Ralston , Pankaj Jain , George M. Frichter

After briefly reviewing various hadronic neutrino source models, we show how to construct generic upper flux bounds. We then turn to the problem of neutrino propagation through the inner Earth and neutrino detection in water-based Cerenkov…

Astrophysics · Physics 2007-05-23 Christian Hettlage , Karl Mannheim

The K2K experiment observes indications of neutrino oscillation: a reduction of $\nu_\mu$ flux together with a distortion of the energy spectrum. Fifty-six beam neutrino events are observed in Super-Kamiokande (SK), 250 km from the neutrino…

High Energy Physics - Experiment · Physics 2009-09-29 K2K Collaboration , M. H. Ahn

Chemical and physical Earth models agree little as to the radioactive power of the planet. Each predicts a range of radioactive powers, overlapping slightly with the other at about 24 TW, and together spanning 14-46 TW. Approximately 20 %…

Nuclear Experiment · Physics 2015-06-03 Steve Dye

The recent geoneutrino experimental results from KamLAND and Borexino detectors reveal the usefulness of analyzing the Earth geoneutrino flux, as it provides a constraint on the strength of the radiogenic heat power and this, in turn,…

An analysis of atmospheric neutrino data from all four run periods of \superk optimized for sensitivity to the neutrino mass hierarchy is presented. Confidence intervals for $\Delta m^2_{32}$, $\sin^2 \theta_{23}$, $\sin^2 \theta_{13}$ and…

High Energy Physics - Experiment · Physics 2018-06-28 Kamiokande Collaboration , K. Abe , C. Bronner , Y. Haga , Y. Hayato , M. Ikeda , K. Iyogi , J. Kameda , Y. Kato , Y. Kishimoto , Ll. Marti , M. Miura , S. Moriyama , M. Nakahata , T. Nakajima , Y. Nakano , S. Nakayama , Y. Okajima , A. Orii , G. Pronost , H. Sekiya , M. Shiozawa , Y. Sonoda , A. Takeda , A. Takenaka , H. Tanaka , S. Tasaka , T. Tomura , R. Akutsu , T. Irvine , T. Kajita , I. Kametani , K. Kaneyuki , Y. Nishimura , K. Okumura , E. Richard , K. M. Tsui , L. Labarga , P. Fernandez , F. d. M. Blaszczyk , J. Gustafson , C. Kachulis , E. Kearns , J. L. Raaf , J. L. Stone , L. R. Sulak , S. Berkman , S. Tobayama , M. Goldhaber , G. Carminati , M. Elnimr , W. R. Kropp , S. Mine , S. Locke , A. Renshaw , M. B. Smy , H. W. Sobel , V. Takhistov , P. Weatherly , K. S. Ganezer , B. L. Hartfiel , J. Hill , N. Hong , J. Y. Kim , I. T. Lim , R. G. Park , T. Akiri , A. Himmel , Z. Li , E. O'Sullivan , K. Scholberg , C. W. Walter , T. Wongjirad , T. Ishizuka , T. Nakamura , J. S. Jang , K. Choi , J. G. Learned , S. Matsuno , S. N. Smith , J. Amey , R. P. Litchfield , W. Y. Ma , Y. Uchida , M. O. Wascko , S. Cao , M. Friend , T. Hasegawa , T. Ishida , T. Ishii , T. Kobayashi , T. Nakadaira , K. Nakamura , Y. Oyama , K. Sakashita , T. Sekiguchi , T. Tsukamoto , KE. Abe , M. Hasegawa , A. T. Suzuki , Y. Takeuchi , T. Yano , T. Hayashino , S. Hirota , K. Huang , K. Ieki , M. Jiang , T. Kikawa , KE. Nakamura , T. Nakaya , N. D. Patel , K. Suzuki , S. Takahashi , R. A. Wendell , L. H. V. Anthony , N. McCauley , A. Pritchard , Y. Fukuda , Y. Itow , G. Mitsuka , M. Murase , F. Muto , T. Suzuki , P. Mijakowski , K. Frankiewicz , J. Hignight , J. Imber , C. K. Jung , X. Li , J. L. Palomino , G. Santucci , C. Vilela , M. J. Wilking , C. Yanagisawa , S. Ito , D. Fukuda , H. Ishino , T. Kayano , A. Kibayashi , Y. Koshio , T. Mori , H. Nagata , M. Sakuda , C. Xu , Y. Kuno , D. Wark , F. Di Lodovico , B. Richards , R. Tacik , S. B. Kim , A. Cole , L. Thompson , H. Okazawa , Y. Choi , K. Ito , K. Nishijima , M. Koshiba , Y. Totsuka , Y. Suda , M. Yokoyama , R. G. Calland , M. Hartz , K. Martens , B. Quilain , C. Simpson , Y. Suzuki , M. R. Vagins , D. Hamabe , M. Kuze , T. Yoshida , M. Ishitsuka , J. F. Martin , C. M. Nantais , P. de Perio , H. A. Tanaka , A. Konaka , S. Chen , L. Wan , Y. Zhang , R. J. Wilkes , A. Minamino

We find that recent results from the KamLAND collaboration on geologically produced antineutrinos, N(U+Th) = 28+16-15 events, correspond to a radiogenic heat production from Uranium and Thorium decay chains H(U+Th) = 38+35-33 TW. The 99%…

High Energy Physics - Phenomenology · Physics 2011-01-04 Gianni Fiorentini , Marcello Lissia , Fabio Mantovani , Barbara Ricci

Decays of radionuclides throughout the Earth's interior produce geothermal heat, but also are a source of antineutrinos. The (angle-integrated) geoneutrino flux places an integral constraint on the terrestrial radionuclide distribution. In…

High Energy Physics - Phenomenology · Physics 2011-04-11 Brian D. Fields , Kathrin A. Hochmuth

We have incorporated a hadron interaction tuning based on accelerator data into our atmospheric neutrino flux calculation, which has been used to analyze atmospheric neutrino oscillations at Super-Kamiokande. This new approach enables a…

High Energy Astrophysical Phenomena · Physics 2026-04-21 Kazufumi Sato , Hiroaki Menjo , Yoshitaka Itow , Morihiro Honda

The atmospheric muon and neutrino flux have been simulated using the same approach which successfully accounted for the recent secondary proton, electron and positron flux measurements in orbit by the AMS experiment. For the muon flux, a…

Astrophysics · Physics 2014-10-13 Yong Liu , L. Derome , M. Buenerd

A comprehensive study on the atmospheric neutrino flux in the energy region from sub-GeV up to several TeV using the Super-Kamiokande water Cherenkov detector is presented in this paper. The energy and azimuthal spectra of the atmospheric…

High Energy Physics - Experiment · Physics 2016-09-07 E. Richard , K. Okumura , K. Abe , Y. Haga , Y. Hayato , M. Ikeda , K. Iyogi , J. Kameda , Y. Kishimoto , M. Miura , S. Moriyama , M. Nakahata , T. Nakajima , Y. Nakano , S. Nakayama , A. Orii , H. Sekiya , M. Shiozawa , A. Takeda , H. Tanaka , T. Tomura , R. A. Wendell , R. Akutsu , T. Irvine , T. Kajita , K. Kaneyuki , Y. Nishimura , L. Labarga , P. Fernandez , J. Gustafson , C. Kachulis , E. Kearns , J. L. Raaf , J. L. Stone , L. R. Sulak , S. Berkman , C. M. Nantais , H. A. Tanaka , S. Tobayama , M. Goldhaber , W. R. Kropp , S. Mine , P. Weatherly , M. B. Smy , H. W. Sobel , V. Takhistov , K. S. Ganezer , B. L. Hartfiel , J. Hill , N. Hong , J. Y. Kim , I. T. Lim , R. G. Park , A. Himmel , Z. Li , E. OSullivan , K. Scholberg , C. W. Walter , T. Wongjirad , T. Ishizuka , S. Tasaka , J. S. Jang , J. G. Learned , S. Matsuno , S. N. Smith , M. Friend , T. Hasegawa , T. Ishida , T. Ishii , T. Kobayashi , T. Nakadaira , K. Nakamura , Y. Oyama , K. Sakashita , T. Sekiguchi , T. Tsukamoto , A. T. Suzuki , Y. Takeuchi , T. Yano , S. V. Cao , T. Hiraki , S. Hirota , K. Huang , T. Kikawa , A. Minamino , T. Nakaya , K. Suzuki , Y. Fukuda , K. Choi , Y. Itow , T. Suzuki , P. Mijakowski , K. Frankiewicz , J. Hignight , J. Imber , C. K. Jung , X. Li , J. L. Palomino , M. J. Wilking , C. Yanagisawa , D. Fukuda , H. Ishino , T. Kayano , A. Kibayashi , Y. Koshio , T. Mori , M. Sakuda , C. Xu , Y. Kuno , R. Tacik , S. B. Kim , H. Okazawa , Y. Choi , K. Nishijima , M. Koshiba , Y. Totsuka , Y. Suda , M. Yokoyama , C. Bronner , M. Hartz , K. Martens , Ll. Marti , Y. Suzuki , M. R. Vagins , J. F. Martin , A. Konaka , S. Chen , Y. Zhang , R. J. Wilkes

Earth neutrino tomography is a realistic possibility with current and future neutrino detectors, complementary to geophysics methods. The two main approaches are based on either partial absorption of the neutrino flux as it propagates…

High Energy Physics - Phenomenology · Physics 2024-08-05 Rasmi Hajjar , Olga Mena , Sergio Palomares-Ruiz

As a unique probe for geophysical research, geoneutrinos can reveal the distribution of internal heat sources in the Earth by detecting electron antineutrinos produced by the radioactive decay of $^{238}$U, $^{232}$Th, and $^{40}$K.…

High Energy Physics - Experiment · Physics 2026-03-27 Keyu Han , Juncheng Qian , Shaomin Chen

In this Letter we show that the evidence for neutrino oscillations from the Super-Kamiokande atmospheric neutrino data fully determines the 3x3 neutrino-oscillations mixing matrix and predicts an energy independent solar neutrino deficit at…

High Energy Physics - Phenomenology · Physics 2011-02-07 Ion Stancu

An evaluation of the principal uncertainties in the computation of neutrino fluxes produced in cosmic ray showers in the atmosphere is presented. The neutrino flux predictions are needed for comparison with experiment to perform neutrino…

Astrophysics · Physics 2008-11-26 G. D. Barr , T. K. Gaisser , S. Robbins , T. Stanev

We develop a first-principles formalism, based on the transport equation in the line-of-sight approximation, to link the expected number of muons at neutrino telescopes to the flux of neutrinos at the Earth's surface. We compute the…

High Energy Physics - Phenomenology · Physics 2025-08-01 Stefano Palmisano , Diego Redigolo , Michele Tammaro , Andrea Tesi

The energy spectrum of geo-neutrinos plays a vital role in the experimental measurement of geo-neutrinos that have profound implications for both particle physics and earth sciences. In this letter, we present a state-of-the-art calculation…

High Energy Physics - Phenomenology · Physics 2024-12-12 Yu-Feng Li , Zhao Xin

We discuss the possibility of forecasting earthquakes by means of (anti)neutrino tomography. Antineutrinos emitted from reactors are used as a probe. As the antineutrinos traverse through a region prone to earthquakes, observable variations…

High Energy Physics - Phenomenology · Physics 2015-05-18 Bin Wang , Ya-Zheng Chen , Xue-Qian Li

The KamLAND and Borexino experiments have detected electron antineutrinos produced in the decay chains of natural thorium and uranium (Th and U geoneutrinos). We analyze the energy spectra of current geoneutrino data in combination with…

High Energy Physics - Phenomenology · Physics 2010-12-13 G. L. Fogli , E. Lisi , A. Palazzo , A. M. Rotunno

Every second greater than $10^{25}$ antineutrinos radiate to space from Earth, shining like a faint antineutrino star. Underground antineutrino detectors have revealed the rapidly decaying fission products inside nuclear reactors, verified…

Instrumentation and Detectors · Physics 2016-02-04 Shawn M. Usman , Glenn R. Jocher , Stephen T. Dye , William F. McDonough , John G. Learned