In exposures of the Argonne National Laboratory 12-ft bubble chamber filled with hydrogen and deuterium to a neutrino beam, we have observed events consist... SJ Barish,Y Cho,M Derrick,... - 《Physical Review Letters》 被引量: 123发表: 1974年 ...
The other two NA61/SHINE (SPS Heavy Ion and Neutrino Experiment) physics goals are related to cosmic ray physics and neutrino physics. The first data for the strong interac- tions program were recorded in 2009 and were followed by a comprehensive two-dimensional scan with beam momentum and ...
Charm hadroproduction measurements are also required for cosmic-ray and neutrino astrophysics, where high-energy neutrinos from the decay of charmed hadrons produced in particle showers in the atmosphere constitute an important background for neutrinos from astrophysical sources [23,24,25,26]. In the...
An experiment, being planned at LAMPF, aims to investigate a possible neutrino oscillation channel, anti ν/sub μ/ → anti ν/sub e/. If anti ν/sub μ/, produced in the LAMPF beam stop, oscillate to anti ν/sub e/, then interactions anti ν/sub e/ + p → e+ n, may be ...
The D-meson production is also of great interest from the viewpoint of neutrino astrophysics as the secondary neutrinos from D mesons produced in scatterings of cosmic rays in the atmosphere form a significant background for the extraterrestrial neutrinos. Given that the D-meson measurements at ...