Results 51 to 60 of about 86,406 (205)

Lessons from the first JUNO results

Journal of High Energy Physics
First results from the JUNO reactor neutrino experiment already determine with world-leading precision the small neutrino squared-mass splitting ∆ m 21 2 $$ \Delta {m}_{21}^2 $$ and the mixing angle θ 12.
Ivan Esteban, M. C. Gonzalez-Garcia, Michele Maltoni, Ivan Martinez-Soler, João Paulo Pinheiro, Thomas Schwetz   +5 more
doaj   +1 more source

Nonstandard interactions in solar neutrino oscillations with Hyper-Kamiokande and JUNO

Physics Letters B, 2017
Measurements of the solar neutrino mass-squared difference from KamLAND and solar neutrino data are somewhat discrepant, perhaps due to nonstandard neutrino interactions in matter.
Jiajun Liao, Danny Marfatia, Kerry Whisnant   +2 more
doaj   +1 more source

IceCube High Energy Starting Events at 7.5 Years -- New Measurements of Flux and Flavor [PDF]

, 2019
The IceCube Neutrino Observatory at the South Pole, which detects Cherenkov light from charged particles produced in neutrino interactions, firmly established the existence of an astrophysical high-energy neutrino component. Here I present IceCube's High-
Stachurska, Juliana
core   +2 more sources

Epidemiology and Genetics of Rheumatic Diseases Suggest a Constant Rate of DNA Damage as Underlying Cause

Immunology, Volume 177, Issue 4, Page 736-748, April 2026.
A constant rate of DNA damage that is not perfectly repaired will cause a constant rate of DNA mutations. The chance of mutation will increase if DNA is prone to damage, such as occurs in somatic hypermutation (SHM) hotspots and GC‐rich DNA. Thus, if one mutation‐prone DNA site drives disease, the age of onset of disease and degree of penetrance should
Piet C. de Groen
wiley   +1 more source

Theory of neutrino slow flavor evolution. Part II. Space-time evolution of linear instabilities

Journal of High Energy Physics
Slow flavor evolution (defined as driven by neutrino masses and not necessarily “slow”) is receiving fresh attention in the context of compact astrophysical environments.
Damiano F. G. Fiorillo, Georg G. Raffelt
doaj   +1 more source

Neutrino Effects in Nucleosynthesis [PDF]

, 2000
The nucleosynthesis within a Type II supernova occurs in an intense neutrino flux. I discuss some of the effects associated with neutrino interactions, including direct synthesis in the neutrino process, the role of neutrinos in controlling the r-process
Haxton, W. C.
core   +3 more sources

Probing non-standard neutrino interactions at neutrino factories

Journal of Physics: Conference Series, 2007
We discuss the sensitivity reach of a neutrino factory measurement to non-standard neutrino interactions (NSI), which may exist as a low-energy manifestation of physics beyond the Standard Model. We use the muon appearance mode _e --> _ and consider two detectors, one at 3000 km and the other at 7000 km.
Ribeiro, N. Cipriano, Minakata, H., Nunokawa, H., Uchinami, S., Funchal, R. Zukanovich   +4 more
openaire   +2 more sources

Toward Large Nonradiating Qubits: When Quantum Engineering Meets Photonics

Advanced Quantum Technologies, Volume 9, Issue 3, March 2026.
Nonradiating superconducting qubits suppress radiative losses through photonic‐inspired mechanisms such as anapole states and bound states in the continuum (BICs). This review surveys theoretical foundations and recent implementations of large, wavelength‐scale qubits that confine electromagnetic energy while maintaining coherence.
Alexey Basharin
wiley   +1 more source

Terrestrial matter effects on reactor antineutrino oscillations: constant vs. fluctuated density profiles

Journal of High Energy Physics
The JUNO Collaboration has recently released its first reactor antineutrino oscillation result, achieving unprecedented precision in the measurement of ∆ m 21 2 $$ \Delta {m}_{21}^2 $$ and sin2 θ 12.
Yu-Feng Li, Andong Wang, Ya Xu, Jing-yu Zhu   +3 more
doaj   +1 more source

Inclusive production of $\rho^{0}(770), f_0(980)$ and $f_2(1270)$ mesons in $\nu_{\mu}$ charged current interactions

, 2001
The inclusive production of the meson resonances $\rho^{0}(770)$, $f_0(980)$ and $f_2(1270)$ in neutrino-nucleus charged current interactions has been studied with the NOMAD detector exposed to the wide band neutrino beam generated by 450 GeV protons at ...
A Baldisseri, A Bueno, A Cardini, A Cervera-Villanueva, A De Santo, A Geiser, A Godley, A Grant, A Guglielmi, A Kovzelev, A Krasnoperov, A Lanza, A Letessier-Selvon, A Ljubičić, A Lupi, A Marchionni, A Placci, A Polyarush, A Rubbia, A Toropin, A.-M Touchard, Abreu, Ackerstaff, Ackerstaff, Agababyan, Aguilar-Benites, Albrecht, Allasia, Allen, Altegoer, Altegoer, Ammosov, Ammosov, Ammosov, Ammosov, Ammosov, Andersson, Apsimon, Apsimon, Arneodo, Autiero, Autiero, Autiero, Autiero, B Blumenfeld, B Lakić, B Popov, B Schmidt, B.D Yabsley, Bassompierre, Bassompierre, Behrend, Berge, Braunschweig, Buskulic, C Conta, C Gößling, C Hagner, C Joseph, C Lachaud, C Nguyen-Mau, C Poulsen, C Roda, Chang, Close, Close, Collazuol, D Autiero, D Daniels, D Ferrère, D Geppert, D Gibin, D Hubbard, D Naumov, D Orestano, D Pollmann, D Sillou, D Steele, Derrick, Deutschmann, E do Couto e Silva, E Gangler, E Iacopini, E Pennacchio, E Tsesmelis, Eszes, F Bobisut, F Juget, F Martelli, F Pastore, F Salvatore, F Vannucci, F.F Wilson, F.J.P Soler, F.V Weber, Fox, G Bassompierre, G Collazuol, G Conforto, G Graziani, G Polesello, G Sozzi, G Vidal-Sitjes, G.F Moorhead, G.J Feldman, G.N Taylor, Graessler, Grassler, Groom, H Degaudenzi, H Pessard, H Zaccone, I Bird, J Bouchez, J Dumarchez, J Gosset, J Hernando, J Kokkonen, J Long, J Rico, J Ulrichs, J.-J Gomez-Cadenas, J.-M Gaillard, J.-M Levy, J.-M Vieira, J.-P Mendiburu, J.-P Meyer, Jackson, Jackson, Jaffe, Jaffe, Jaffe, Jones, Jones, Jones, Jones, K Benslama, K Schahmaneche, K Zuber, K.E Varvell, Kirk, L Camilleri, L Di Lella, L LaRotonda, L Linssen, L Vacavant, L.J Winton, L.S Peak, M Baldo-Ceolin, M Banner, M Contalbrigo, M Ellis, M Fraternali, M Gouanère, M Kirsanov, M Laveder, M Mezzetto, M Sevior, M Stipčević, M Tareb-Reyes, M Valdata-Nappi, M Veltri, M.-T Tran, Minaenko, N Besson, N Hyett, O Klimov, P Astier, P Hurst, P Nédélec, P Rathouit, P Zuccon, P.W Cattaneo, R Cousins, R Ferrari, R Petti, Robson, S Boyd, S Bunyatov, S Gninenko, S Lacaprara, S.N Tovey, S.R Mishra, Sjostrand, T Del Prete, T Dignan, T Fazio, T Vinogradova, T Weisse, Th Stolarczyk, U Stiegler, V Cavasinni, V Flaminio, V Kuznetsov, V Tereshchenko, V Valuev, V Vercesi, Weinstein, Wittek, Wittek, X Méchain, Yu Nefedov, Zaetz   +202 more
core   +2 more sources