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Mixture-of-experts graph transformers for interpretable particle collision detection. [PDF]
Genovese D +8 more
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Physics Today, 1948
The neutrino is a hypothetical particle which was proposed by Pauli a number of years ago, mainly to save the principle of the conservation of energy in beta-decay.
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The neutrino is a hypothetical particle which was proposed by Pauli a number of years ago, mainly to save the principle of the conservation of energy in beta-decay.
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Atmospheric neutrino data and neutrino oscillations
Physical Review D, 1993Several calculations of the upward throughgoing and stopping muon fluxes produced by atmospheric, or cosmic ray, neutrinos interacting in the material surrounding underground detectors are compared and the uncertainties in the calculations estimated.
, Frati, , Gaisser, , Mann, , Stanev
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Mixing of a heavy neutrino with the electron neutrino
Physical Review D, 1985We show that recent monojet searches in electron-positron annihilation experiments can be used to extend significantly the limits on the mixing of a massive fourth-generation neutrino with the electron neutrino. When combined with other limits from hadron decays and secondary-vertex searches in hadron and electron-positron annihilation experiments ...
, Gilman, , Rhie
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Neutrino oscillations and the solar-neutrino problem
Physical Review D, 1987The values of neutrino masses and mixing angles which are required by the Mikheyev-Smirnov-Wolfenstein (MSW) solution to the solar-neutrino problem are found from analytic solutions to the neutrino propagation equations in the Sun. They coincide with those obtained through extensive numerical computations by Rosen and Gelb.
, Dar, , Mann, , Melina, , Zajfman
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Solar neutrino observations and neutrino oscillations
Physical Review D, 1990The results of recent Kamiokande-II and {sup 37}Cl solar-neutrino experiments are quantitatively analyzed assuming the Mikheyev-Smirnov-Wolfenstein solution to the solar-neutrino problem. It is found that the parameter region known as the large mass'' solution to the solar-neutrino problem is disfavored by a little more than 1 {sigma} while the small ...
, Kuo, , Pantaleone
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Neutrino oscillations in dense neutrino gases
Physical Review D, 1993We consider oscillations of neutrinos under conditions in which the neutrino density is sufficiently large that neutrino-neutrino interactions cannot be neglected. A formalism is developed to treat this highly nonlinear system. Numerical analysis reveals a rich array of phenomena.
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Status and perspectives of neutrino physics
Progress in Particle and Nuclear Physics, 2022M Sajjad Athar +2 more
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