Results 161 to 170 of about 3,937 (188)
Some of the next articles are maybe not open access.
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
openaire +2 more sources
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
openaire +2 more sources
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
openaire +2 more sources
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
openaire +2 more sources
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.
openaire +2 more sources