Results 51 to 60 of about 1,187,743 (285)

Solar neutrinos as a probe of dark matter-neutrino interactions [PDF]

, 2017
Sterile neutrinos at the eV scale have long been studied in the context of anomalies in short baseline neutrino experiments. Their cosmology can be made compatible with our understanding of the early Universe provided the sterile neutrino sector enjoys a
F. Capozzi, I. Shoemaker, L. Vecchi
semanticscholar   +1 more source

2020 global reassessment of the neutrino oscillation picture [PDF]

Journal of High Energy Physics, 2020
We present an updated global fit of neutrino oscillation data in the simplest three-neutrino framework. In the present study we include up-to-date analyses from a number of experiments.
P. F. D. Salas, D. V. Forero, S. Gariazzo, P. Martínez-Miravé, O. Mena, C. A. Ternes, M. Tórtola, J. Valle   +7 more
semanticscholar   +1 more source

A road map to solar neutrino fluxes, neutrino oscillation parameters, and tests for new physics [PDF]

, 2003
We analyze all available solar and related reactor neutrino experiments, as well as simulated future 7Be, p-p, pep, and ^8B solar neutrino experiments.
Bahcall, John N., Pena-Garay, Carlos
core   +5 more sources

Recent results from Borexino on solar neutrinos [PDF]

EPJ Web of Conferences, 2023
Borexino has been a neutrino detector based on ultrapure liquid scintillator, located at the Laboratori Nazionali del Gran Sasso, Italy. Its main scientific goal was the real-time measurement of solar neutrino fluxes, which play an irreplaceable role for
Basilico D., Appel S., Bagdasarian Z., Bellini G., Benziger J., Biondi R., Caccianiga B., Calaprice F., Caminata A., Chepurnov A., D’Angelo D., Derbin A., Di Giacinto A., Di Marcello V., Ding X.F., Di Ludovico A., Di Noto L., Drachnev I., Franco D., Galbiati C., Ghiano C., Giammarchi M., Goretti A., Göttel A.S., Gromov L., Guffanti D., Ianni Aldo, Ianni Andrea, Jany A., Kobychev V., Korga G., Kumaran S., Laubenstein M., Litvinovich E., Lombardi P., Lomskaya I., Ludhova L., Lukyanchenko G., Machulin I., Martyn J., Meroni E., Miramonti L., Misiaszek M., Muratova V., Nugmanov R., Oberauer L., Orekhov V., Ortica F., Pallavicini M., Pelicci L., Penek Ö., Pietrofaccia L., Pilipenko N., Pocar A., Raikov G., Ranalli M.T., Ranucci G., Razeto A., Re A., Redchuk M., Rossi N., Schönert S., Semenov D., Settanta G., Skorokhvatov M., Singhal A., Smirnov O., Sotnikov A., Tartaglia R., Testera G., Unzhakov E., Villante F., Vishneva A., Vogelaar R.B., von Feilitzsch F., Wojcik M., Wurm M., Zavatarelli S., Zuber K., Zuzel G.   +79 more
doaj   +1 more source

Solar neutrino physics with low-threshold dark matter detectors [PDF]

, 2014
Dark matter detectors will soon be sensitive to Solar neutrinos via two distinct channels: coherent neutrino-nucleus and neutrino-electron elastic scatterings.
J. Billard, J. Billard, J. Billard, L. Strigari, L. Strigari, L. Strigari, E. Figueroa-Feliciano, E. Figueroa-Feliciano, E. Figueroa-Feliciano   +8 more
semanticscholar   +1 more source

Solar neutrinos: Solar physics and neutrino physics [PDF]

Nuclear Physics B - Proceedings Supplements, 1994
Abstract It is shown that the current solar neutrino situation, with results from the Homestake experiment, the Kamiokande experiment, GALLEX and SAGE is unfortunately still ambiguous. The differences between observations and the standard solar theory may still be due to either astrophysical inputs or new neutrino physics.
D.N. Schramm, D.N. Schramm, X. Shi
openaire   +2 more sources

Frontier of Understanding Earth's Dynamics

, 2023
Perspectives of Earth and Space Scientists, Volume 4, Issue 1, December 2023.
Hiroko Watanabe, Natsue Abe, William F. McDonough, Tamano Omata, Yasuhiro Yamada   +4 more
wiley   +1 more source

Shedding light on LMA-dark solar neutrino solution by medium baseline reactor experiments: JUNO and RENO-50 [PDF]

, 2014
A bstractIn the presence of Non-Standard neutral current Interactions (NSI) a new solution to solar neutrino anomaly with cos 2θ12 < 0 appears. We investigate how this solution can be tested by upcoming intermediate baseline reactor experiments, JUNO and
P. Bakhti, Y. Farzan
semanticscholar   +1 more source

Constraints on flavor-diagonal non-standard neutrino interactions from Borexino Phase-II

Journal of High Energy Physics, 2020
The Borexino detector measures solar neutrino fluxes via neutrino-electron elastic scattering. Observed spectra are determined by the solar-ν e survival probability P ee (E), and the chiral couplings of the neutrino and electron. Some theories of physics
The Borexino collaboration, S. K. Agarwalla, M. Agostini, K. Altenmüller, S. Appel, V. Atroshchenko, Z. Bagdasarian, D. Basilico, G. Bellini, J. Benziger, D. Bick, G. Bonfini, D. Bravo, B. Caccianiga, F. Calaprice, A. Caminata, L. Cappelli, P. Cavalcante, F. Cavanna, A. Chepurnov, K. Choi, D. D’Angelo, S. Davini, A. Derbin, A. Di Giacinto, V. Di Marcello, X. F. Ding, A. Di Ludovico, L. Di Noto, I. Drachnev, K. Fomenko, A. Formozov, D. Franco, F. Gabriele, C. Galbiati, M. Gschwender, C. Ghiano, M. Giammarchi, A. Goretti, M. Gromov, D. Guffanti, C. Hagner, E. Hungerford, Aldo Ianni, Andrea Ianni, A. Jany, D. Jeschke, S. Kumaran, V. Kobychev, G. Korga, T. Lachenmaier, M. Laubenstein, E. Litvinovich, P. Lombardi, L. Ludhova, G. Lukyanchenko, L. Lukyanchenko, I. Machulin, G. Manuzio, S. Marcocci, J. Maricic, J. Martyn, E. Meroni, M. Meyer, L. Miramonti, M. Misiaszek, V. Muratova, B. Neumair, M. Nieslony, L. Oberauer, V. Orekhov, F. Ortica, M. Pallavicini, L. Papp, Ö. Penek, L. Pietrofaccia, N. Pilipenko, A. Pocar, G. Raikov, G. Ranucci, A. Razeto, A. Re, M. Redchuk, A. Romani, N. Rossi, S. Rottenanger, S. Schönert, D. Semenov, M. Skorokhvatov, O. Smirnov, A. Sotnikov, C. Sun, Y. Suvorov, T. Takeuchi, R. Tartaglia, G. Testera, J. Thurn, E. Unzhakov, A. Vishneva, R. B. Vogelaar, F. von Feilitzsch, M. Wojcik, M. Wurm, O. Zaimidoroga, S. Zavatarelli, K. Zuber, G. Zuzel   +106 more
doaj   +1 more source

7Be solar neutrino measurement with KamLAND [PDF]

, 2014
We report a measurement of the neutrino-electron elastic scattering rate of 862 keV ^7Be solar neutrinos based on a 165.4 kt d exposure of KamLAND. The observed rate is 582±94(kt d)^(−1), which corresponds to an 862-keV Be7 solar neutrino flux of (3.26±0.
A. Gando, Y. Gando, H. Hanakago, H. Ikeda, K. Inoue, K. Ishidoshiro, H. Ishikawa, Y. Kishimoto, M. Koga, R. Matsuda, S. Matsuda, T. Mitsui, D. Motoki, K. Nakajima, K. Nakamura, A. Obata, A. Oki, Y. Oki, M. Otani, I. Shimizu, J. Shirai, A. Suzuki, K. Tamae, K. Ueshima, H. Watanabe, B. D. Xu, S. Yamada, Y. Yamauchi, H. Yoshida, A. Kozlov, Y. Takemoto, S. Yoshida, C. Grant, G. Keefer, D. Mckee, A. Piepke, T. Banks, T. Bloxham, S. Freedman, B. Fujikawa, K. Han, L. Hsu, K. Ichimura, H. Murayama, T. O’Donnell, H. Steiner, L. Winslow, D. Dwyer, C. Mauger, R. Mckeown, C. Zhang, B. Berger, C. Lane, J. Maricic, T. Miletić, J. Learned, M. Sakai, G. Horton-Smith, A. Tang, K. Downum, K. Tolich, Y. Efremenko, Y. Kamyshkov, O. Perevozchikov, H. Karwowski, D. Markoff, W. Tornow, J. Detwiler, S. Enomoto, K. Heeger, M. Decowski   +70 more
semanticscholar   +1 more source