By Robert W. Fox
Fox R.W. advent to Fluid Mechanics sixth variation simply Ask with Registration Card and E--Commerace Card simply Ask sixth version Set (Wiley Inc, 2006)(ISBN 0471775878)
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Sample text
These experiments are conveniently divided into those that start from muon neutrinos or antineutrinos (muon neutrino oscillations) and those that start with electron neutrinos or antineutinos (electron neutrino oscillations). 2(a) Muon neutrino oscillations The first experiment to produce definitive evidence for neutrino oscillations was that of the SuperKamiokande group, who in 1998 used a giant detector to study atmospheric neutrinos. When cosmic ray protons collide with nuclei in the upper atmosphere they create many pions and, as we shall see presently, the decay sequence of pions in turn creates neutrinos, with two muon neutrinos being produced for every electron neutrino.
The data show clear evidence for a deviation of this ratio from unity, particularly at large values of L/E.
Thus, in the reaction ve + n → e− + p, an electron neutrino ve collides with a neutron n to produce an electron e− and a proton p while the equation e− + p → e− + p represents an electron and proton interacting to give the same particles in the final state, but in general travelling in different directions. The forces producing the above interactions are due to the exchange of particles and a convenient way of illustrating this is to use the pictorial technique of Feynman diagrams. These were introduced by Feynman in the 1940s and are now one of the cornerstones of the analysis of elementary particle physics.