Results 81 to 90 of about 3,937 (188)
PHENOMENOLOGY OF NEUTRINO OSCILLATIONS AT A NEUTRINO FACTORY [PDF]
, 2000 It is shown in the three flavor framework that neutrino factories enable us to measure some of the oscillation parameters, such as the sign of $Δm_{32}^2$, $θ_{13}$, $δ$. Some efforts are made to determine the parameters (the muon energy and the neutrino path length) of a neutrino factory to optimize the signals.
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Whipped and Mixed Warm Clouds in the Deep Sea
Geophysical Research Letters, Volume 53, Issue 2, 28 January 2026.Abstract Turbulence is indispensable to redistribute nutrients for all life forms larger than microbial, on land and in the ocean. Yet, the development of deep‐sea turbulence was not studied in three dimensions to date. As a disproportionate laboratory, an array of nearly 3,000 high‐resolution temperature sensors had been installed for three years on ...
Hans van Haren, KM3NeT collaboration
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Annalen der Physik, Volume 538, Issue 1, January 2026.The BRST invariant Lagrangian of the gravitationally interacting U(1)$U(1)$ gauge theory, namely the Quantum GraviElectro Dynamics (QGED). The Yan–Mills theory with the Hilbert–Einstein gravitational Lagrangian, namely the Yang–Mills–Utiyama (YMU) theory, is defined and quantised using the standard procedure. The theory is perturbatively renormalisable,
Yoshimasa Kurihara
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MEASURING NEUTRINO MASSES WITH SUPERNOVA NEUTRINOS [PDF]
The Tenth Marcel Grossmann Meeting, 2006 3 pages; contribution to the proceedings of X Marcel Grossmann Meeting, Rio de Janeiro, 20-26 July ...
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Acta Universitaria, 2012 From all the proposals to understand the structure of matter, and the way the natural world is conformed, the one about neutrinos is the most enigmatic, abstract, and foreign to immediate experience; however, this is the one that has delved more deeply ...
Julián Félix
doaj
Testing exotic neutrino-neutrino interactions with AGN neutrinos [PDF]
Physics Letters B, 1998 8 pages, latex, no ...
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Astronomy & AstrophysicsWe study the early postbounce neutrino signal of the published Garching 15 M⊙ rotating core-collapse supernova (CCSN) sequence consisting of nonrotating (NR), slowly rotating (SR, Ω0 = 0.5 rad s−1), and fast-rotating (FR, Ω0 = 150 rad s−1, artificially ...
Viaux N.
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Hadronic Models of the Fermi Bubbles: Future Perspectives
Galaxies, 2018 The origin of sub-TeV gamma rays detected by Fermi-LAT from the Fermi bubbles at the Galactic center is still unknown. In a hadronic model, acceleration of protons and/or nuclei and their subsequent interactions with gas in the bubble volume can produce ...
Soebur Razzaque, Lili Yang
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Phenomenology of neutrino oscillations at the neutrino factory
Journal of Physics: Conference Series, 2012 We consider the prospects for a neutrino factory to measure mixing angles, the CP violating phase and mass-squared differences by detecting wrong-charged muons arising from the chain μ^+ to ν_e to ν_μ to μ^- and the right-charged muons coming from the chain μ^+ to \barν_μ to \barν_μ to μ^+ (similar to μ^- chains), where ν_e to ν_μ and \barν_μ to ...
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