Results 81 to 90 of about 41,603 (215)

Solar Neutrinos

, 2009
Proceedings of XXIX Physics in Collisions conference - Kobe, Japan ...
openaire   +3 more sources

Cosmic Ray Counting Variability From Water‐Cherenkov Detectors as a Proxy of Stratospheric Conditions in Antarctica

Earth and Space Science, Volume 12, Issue 11, November 2025.
Abstract This work examines atmospheric effects on cosmic ray counts observed by a Water‐Cherenkov detector at the Argentine Antarctic Marambio Station. We analyze the influence of ground‐level barometric pressure and geopotential height at various pressure levels on daily particle rates, finding the strongest association at 100 hPa, linked to ...
N. A. Santos, N. Gómez, S. Dasso, A. M. Gulisano, L. Rubinstein, M. Pereira, O. Areso, for the LAGO Collaboration   +7 more
wiley   +1 more source

Violation of Equivalence Principle and Solar Neutrinos [PDF]

, 2000
We have updated the analysis for the solution to the solar neutrino problem by the long-wavelength neutrino oscillations induced by a tiny breakdown of the weak equivalence principle of general relativity, and obtained a very good fit to all the solar ...
A.M. Gago, Altmann, Bahcall, Casini, Gago, Gago, Gasperini, Gasperini, H. Nunokawa, Halprin, Hampel, Lande, Mansour, Pantaleone, R. Zukanovich Funchal   +14 more
core   +2 more sources

Solar neutrinos and the strongest oscillation constraints on scalar NSI

Journal of High Energy Physics
Scalar non-standard neutrino interactions (sNSI) is a scenario where neutrinos can develop a medium dependent contribution to their mass due to a new scalar mediator.
Peter B. Denton, Alessio Giarnetti, Davide Meloni   +2 more
doaj   +1 more source

Highlights from Super-Kamiokande

EPJ Web of Conferences, 2016
Recent results from Super-Kamiokande experiment are reviewed in this paper; Neutrino mass hierarchy and CP violation in the lepton sector are investigated via νμ → νe oscillation of the atmospheric neutrinos.
Okumura Kimihiro
doaj   +1 more source

Solar neutrino detection sensitivity in DARWIN via electron scattering

European Physical Journal C: Particles and Fields, 2020
We detail the sensitivity of the proposed liquid xenon DARWIN observatory to solar neutrinos via elastic electron scattering. We find that DARWIN will have the potential to measure the fluxes of five solar neutrino components: pp, $$^7$$ 7 Be, $$^{13 ...
DARWIN Collaboration, J. Aalbers, F. Agostini, S. E. M. Ahmed Maouloud, M. Alfonsi, L. Althueser, F. D. Amaro, J. Angevaare, V. C. Antochi, B. Antunovic, E. Aprile, L. Arazi, F. Arneodo, M. Balzer, L. Baudis, D. Baur, M. L. Benabderrahmane, Y. Biondi, A. Bismark, C. Bourgeois, A. Breskin, P. A. Breur, A. Brown, E. Brown, S. Brünner, G. Bruno, R. Budnik, C. Capelli, J. Cardoso, D. Cichon, M. Clark, A. P. Colijn, J. Conrad, J. J. Cuenca-García, J. P. Cussonneau, M. P. Decowski, A. Depoian, J. Dierle, P. Di Gangi, A. Di Giovanni, S. Diglio, D. Douillet, G. Drexlin, K. Eitel, R. Engel, E. Erdal, A. D. Ferella, H. Fischer, P. Fischer, W. Fulgione, P. Gaemers, M. Galloway, F. Gao, D. Giovagnoli, F. Girard, R. Glade-Beucke, F. Glück, L. Grandi, S. Grohmann, R. Größle, R. Gumbsheimer, V. Hannen, S. Hansmann-Menzemer, C. Hils, B. Holzapfel, J. Howlett, G. Iaquaniello, F. Jörg, M. Keller, J. Kellerer, G. Khundzakishvili, B. Kilminster, M. Kleifges, T. K. Kleiner, G. Koltmann, A. Kopec, A. Kopmann, L. M. Krauss, F. Kuger, L. LaCascio, H. Landsman, R. F. Lang, S. Lindemann, M. Lindner, F. Lombardi, J. A. M. Lopes, A. Loya Villalpando, Y. Ma, C. Macolino, J. Mahlstedt, A. Manfredini, T. Marrodán Undagoitia, J. Masbou, D. Masson, E. Masson, N. McFadden, P. Meinhardt, R. Meyer, B. Milosevic, S. Milutinovic, A. Molinario, C. M. B. Monteiro, K. Morå, E. Morteau, Y. Mosbacher, M. Murra, J. L. Newstead, K. Ni, U. G. Oberlack, M. Obradovic, K. Odgers, I. Ostrovskiy, J. Palacio, M. Pandurovic, B. Pelssers, R. Peres, J. Pienaar, M. Pierre, V. Pizzella, G. Plante, J. Qi, J. Qin, D. Ramírez García, S. E. Reichard, N. Rupp, P. Sanchez-Lucas, J. M. F. dos Santos, G. Sartorelli, D. Schulte, H. C. Schultz-Coulon, H. Schulze Eißing, M. Schumann, L. Scotto Lavina, M. Selvi, P. Shagin, S. Sharma, W. Shen, M. Silva, H. Simgen, M. Steidl, S. Stern, D. Subotic, P. Szabo, A. Terliuk, C. Therreau, D. Thers, K. Thieme, F. Toennies, R. Trotta, C. D. Tunnell, K. Valerius, G. Volta, D. Vorkapic, M. Weber, Y. Wei, C. Weinheimer, M. Weiss, D. Wenz, C. Wittweg, J. Wolf, S. Wuestling, M. Wurm, Y. Xing, T. Zhu, Y. Zhu, J. P. Zopounidis, K. Zuber   +166 more
doaj   +1 more source

Solar neutrino spectroscopy [PDF]

Physics Reports, 2017
More than forty years after the first detection of neutrinos from the Sun, the spectroscopy of solar neutrinos has proven to be an on-going success story. The long-standing puzzle about the observed solar neutrino deficit has been resolved by the discovery of neutrino flavor oscillations.
openaire   +2 more sources

Human flaws and logical tools in engineering

The Canadian Journal of Chemical Engineering, Volume 103, Issue 8, Page 3512-3520, August 2025.
Abstract This paper explores the limitations of human cognition, especially in engineering research, emphasizing the need for mathematical models and methods to guide decision‐making and theory validation. While human cognition excels in certain tasks, it is prone to biases that can distort our understanding.
André C. R. Martins
wiley   +1 more source

Constraints on active-sterile neutrino transition magnetic moments from low-energy electronic recoils at direct detection experiments

Physics Letters B
Sterile neutrinos can potentially be produced through neutrino transition magnetic moments in neutrino-electron scattering. In this work, we investigate this dipole portal by analyzing low-energy electronic recoil data from the PandaX-4T (Run0 and Run1 ...
M.F. Mustamin, M. Demirci
doaj   +1 more source

Recent Borexino results and prospects for the near future

EPJ Web of Conferences, 2016
The Borexino experiment located in the Gran Sasso National Laboratory, is an organic liquid scintillator detector conceived for the real time spectroscopy of low energy solar neutrinos.
D’Angelo D., Agostini M., Altenmüller K., Appel S., Bellini G., Benziger J., Bick D., Bonfini G., Bravo D., Caccianiga B., Calaprice F., Caminata A., Cavalcante P., Chepurnov A., Davini S., Derbin A., Di Noto L., Drachnev I., Etenko A., Fomenko K., Franco D., Gabriele F., Galbiati C., Ghiano C., Giammarchi M., Goeger-Neff M., Goretti A., Gromov M., Hagner C., Hungerford E., Ianni Aldo, Ianni Andrea, Jedrzejczak K., Kaiser M., Kobychev V., Korablev D., Korga G., Kryn D., Laubenstein M., Lehnert B., Litvinovich E., Lombardi F., Lombardi P., Ludhova L., Lukyanchenko G., Machulin I., Manecki S., Maneschg W., Marcocci S., Meroni E., Meyer M., Miramonti L., Misiaszek M., Montuschi M., Mosteiro P., Muratova V., Neumair B., Oberauer L., Obolensky M., Ortica F., Pallavicini M., Papp L., Perasso L., Pocar A., Ranucci G., Razeto A., Re A., Romani A., Roncin R., Rossi N., Schönert S., Semenov D., Simgen H., Skorokhvatov M., Smirnov O., Sotnikov A., Sukhotin S., Suvorov Y., Tartaglia R., Testera G., Thurn J., Toropova M., Unzhakov E., Vishneva A., Vogelaar R.B., von Feilitzsch F., Wang H., Weinz S., Winter J., Wojcik M., Wurm M., Yokley Z., Zaimidoroga O., Zavatarelli S., Zuber K., Zuzel G.   +95 more
doaj   +1 more source