Results 21 to 30 of about 1,199,141 (307)

Constraining light mediators via detection of coherent elastic solar neutrino nucleus scattering

Nuclear Physics B, 2022
Dark matter (DM) direct detection experiments are entering the multiple-ton era and will be sensitive to the coherent elastic neutrino nucleus scattering (CEνNS) of solar neutrinos, enabling the possibility to explore contributions from new physics with ...
Yu-Feng Li, Shuo-yu Xia
doaj   +1 more source

Solar neutrino detection [PDF]

AIP Conference Proceedings, 2009
8 pages, 5 figures. III School on Cosmic Rays and Astrophysics August 25 to September 5, 2008 Arequipa (Peru) AIP conference ...
Lino Miramonti, Carlos Javier Solano Salinas, Jose Bellido, David Wahl, Oscar Saavedra   +4 more
openaire   +5 more sources

The potential to probe solar neutrino physics with LiCl water solution

European Physical Journal C: Particles and Fields, 2023
A solar neutrino detector relying on the charged-current (CC) interaction of $$\nu _e$$ ν e on $$\mathrm{{}^{7}Li}$$ 7 Li is attractive. The total CC interaction cross-section weighted by the solar $$^8$$ 8 B electron neutrino spectrum is approximately ...
Wenhui Shao, Weiran Xu, Ye Liang, Wentai Luo, Tong Xu, Ming Qi, Jialiang Zhang, Benda Xu, Zhe Wang, Shaomin Chen   +9 more
doaj   +1 more source

Solar Neutrino Measurements in Super-Kamiokande-IV [PDF]

, 2016
Upgraded electronics, improved water system dynamics, better calibration and analysis techniques allowed Super-Kamiokande-IV to clearly observe very low-energy 8B solar neutrino interactions, with recoil electron kinetic energies as low as 3.49 MeV ...
S. Abe, Y. Haga, Y. Hayato, M. Ikeda, K. Iyogi, J. Kameda, Y. Kishimoto, L. Marti, M. Miura, S. Moriyama, M. Nakahata, T. Nakajima, S. Nakayama, A. Orii, H. Sekiya, M. Shiozawa, Y. Sonoda, A. Takeda, H. Tanaka, Y. Takenaga, S. Tasaka, T. Tomura, K. Ueno, T. Yokozawa, R. Akutsu, T. Irvine, H. Kaji, T. Kajita, I. Kametani, K. Kaneyuki, K. P. Lee, Y. Nishimura, T. McLachlan, K. Okumura, E. Richard, L. Labarga, P. Fernández, F. Blaszczyk, J. Gustafson, C. Kachulis, E. Kearns, 32 J. L. Raaf, J. Stone, 32 L. R. Sulak, S. Berkman, S. Tobayama, M. Goldhaber, K. Bays, G. Carminati, N. J. Griskevich, W. Kropp, S. Mine, A. Renshaw, M. Smy, H. Sobel, V. Takhistov, P. Weatherly, K. Ganezer, B. Hartfiel, J. Hill, W. Keig, N. Hong, J. Kim, I. Lim, R. Park, T. Akiri, J. Albert, A. Himmel, Z. Li, E. O’Sullivan, K. Scholberg, C. Walter, T. Wongjirad, T. Ishizuka, T. Nakamura, J. Jang, K. Choi, J. Learned, S. Matsuno, S. Smith, M. Friend, T. Hasegawa, T. Ishida, T. Ishii, T. Kobayashi, T. Nakadaira, K. Nakamura, K. Nishikawa, Y. Oyama, K. Sakashita, T. Sekiguchi, T. Tsukamoto, Y. Nakano, A. Suzuki, Y. Takeuchi, T. Yano, S. Cao, T. Hayashino, T. Hiraki, S. Hirota, K. Huang, K. Ieki, M. Jiang, T. Kikawa, A. Minamino, A. Murakami, T. Nakaya, N. Patel, K. Suzuki, S. Takahashi, R. Wendell, Y. Fukuda, Y. Itow, G. Mitsuka, F. Muto, T. Suzuki, P. Mijakowski, K. Frankiewicz, J. Hignight, J. Imber, C. Jung, X. Li, J. Palomino, G. Santucci, I. Taylor, C. Vilela, M. Wilking, C. Yanagisawa, D. Fukuda, H. Ishino, T. Kayano, A. Kibayashi, Y. Koshio, T. Mori, M. Sakuda, J. Takeuchi, R. Yamaguchi, Y. Kuno, R. Tacik, S. Kim, H. Okazawa, Y. Choi, K. Itô, K. Nishijima, M. Koshiba, Y. Totsuka, Y. Suda, M. Yokoyama, C. Bronner, R. Calland, M. Hartz, K. Martens, Y. Obayashi, Y. Suzuki, M. Vagins, C. Nantais, J. Martin, P. Perio, H. Tanaka, A. Konaka, S. Chen, H. Sui, L. Wan, Z. Yang, H. Zhang, Y. Zhang, K. Connolly, M. Dziomba, R. Observatory, Inst. for Nucl. Research, U. Tokyo, Research Center for Cosmic Neutrinos, Department of Applied Physics, U. A. Madrid, Department of Applied Physics, Boston University, Astronomy, U. Columbia, P. Department, Brookhaven National Laboratory, U. California, Irvine, California Polytechnic State University, Chonnam National University, D. University, Junior College, Fukuoka Institute of Technology, G. University, Gist College, Gwangju Institute of Science, Technology, U. Hawaii, High Energy Accelerator Research Organization, K. University, Kyoto University, Miyagi University of Education, Inst. for Nucl. Research, Nagoya University, Kobayashi-Maskawa Institute for the Origin of Particles, the Universe, N. C. F. N. Research, State University of New York at Stony Brook, O. University, Okayama, Okayama 700-8530, J. D. O. Physics, O. University, U. O. Regina, Seoul National University, Department of Informatics in Social Welfare, Shizuoka University of Welfare, S. University, T. University, T. U. O. Tokyo, K. I. F. T. Physics, M. Universe, The University of Tokyo Institutes for Advanced Study, U. Toronto, Triumf, 4004 Wesbrook Mall, Department of Applied Physics, Tsinghua University, U. Washington   +222 more
semanticscholar   +1 more source

Constraining neutrino lifetimes and magnetic moments via solar neutrinos in the large xenon detectors [PDF]

Journal of Cosmology and Astroparticle Physics, 2018
The multi-ton-scale liquid xenon detectors, with an excellent energy resolution of a few keV, will be constructed to probe the dark-matter particles. In this paper, we show that precision measurements of the low-energy solar neutrinos via the elastic ...
Guo-Yuan Huang, Shun Zhou
semanticscholar   +1 more source

Is bi-maximal mixing compatible with the large angle MSW solution of the solar neutrino problem? [PDF]

, 1998
It is shown that the large angle MSW solution of the solar neutrino problem with a bi-maximal neutrino mixing matrix implies an energy-independent suppression of the solar nu_e flux.
A.J. Baltz, B.T. Cleveland, C. Caso, C. Giunti, G. Altarelli, H. Fritzsch, H. Fritzsch, J.N. Abdurashitov, J.N. Bahcall, J.N. Bahcall, K.S. Kang, L. Wolfenstein, L. Wolfenstein, N. Haba, R. Becker-Szendy, S.M. Bilenky, S.M. Bilenky, S.M. Bilenky, S.P. Mikheyev, S.P. Mikheyev, T.K. Kuo, V. Barger, W. Hampel, W.W.M. Allison, Y. Fukuda, Y. Fukuda, Y. Fukuda, Y. Nomura   +27 more
core   +2 more sources

Solar neutrinos [PDF]

AIP Conference Proceedings, 1966
I summarize the current state of solar neutrino research and then give my answer to the question: What should we do next?
openaire   +6 more sources

Advice for a Young Scientist

Perspectives of Earth and Space Scientists, Volume 4, Issue 1, December 2023., 2023
Abstract My career has included astrophysics and space physics, always with a theoretical emphasis. My first papers calculated nuclear reaction rates in dense stars, particularly neutron stars, but I branched out to other areas or theoretical astrophysics.
R. A. Wolf
wiley   +1 more source

Solar neutrino flux at keV energies [PDF]

, 2017
We calculate the solar neutrino and antineutrino flux in the keV energy range. The dominant thermal source processes are photo production (γ e→ e νν̄), bremsstrahlung (e+Ze→ Ze+e+νν̄), plasmon decay (γ→νν̄), and νν̄ emission in free-bound and bound-bound
E. Vitagliano, J. Redondo, G. Raffelt
semanticscholar   +1 more source

The fate of hints: updated global analysis of three-flavor neutrino oscillations [PDF]

Journal of High Energy Physics, 2020
Our herein described combined analysis of the latest neutrino oscillation data presented at the Neutrino2020 conference shows that previous hints for the neutrino mass ordering have significantly decreased, and normal ordering (NO) is favored only at the
I. Esteban, M. Gonzalez-Garcia, M. Maltoni, T. Schwetz, A. Zhou   +4 more
semanticscholar   +1 more source