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Get Quantum Probability and Applications, V: Proceedings of the PDF

By Luigi Accardi, Wilhelm v. Waldenfels

ISBN-10: 3540530266

ISBN-13: 9783540530268

Those court cases of the workshop on quantum chance held in Heidelberg, September 26-30, 1988 encompasses a consultant choice of learn articles on quantum stochastic procedures, quantum stochastic calculus, quantum noise, geometry, quantum chance, quantum important restrict theorems and quantum statistical mechanics.

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Additional info for Quantum Probability and Applications, V: Proceedings of the Fourth Workshop, Held in Heidelberg, FRG, Sept. 26-30, 1988

Sample text

Indeed, the relativistic transformation of energy and momentum implies that the equal momentum assumption cannot hold concurrently in different inertial systems. g. an electron is seen as an electron in any system of reference). Therefore, the probability of neutrino oscillations is Lorentz invariant [13,30] and must be derived in a covariant way. In fact, the oscillation probability has been derived without special assumptions about the energies and momenta of the different massive neutrino components both in the plane wave approach 112-151 and in the wave packet treatment [22-24,291.

Petti, paper in preparation. [13] A. Arbuzov, D. Bardin and L. Kalinovskaya, paper in preparation. [14] K. Diener, S. Dittmaier and W. Hollik, hep-ph/0310364. FROM THE EXTREME UNIVERSE SPACE OBSERVATORY (EUSO) TO THE EXTREME ENERGY NEUTRINO OBSERVATORY S. Bottaia, P. ). For the Extreme Energy neutrino astronomy such detectors will probably exhibit a lack of statistics and a further increase of sensitivity will be necessary for this goal. The increase on neutrino events statistics is discussed with respect t o different detector layout 1 Introduction The discovery of cosmic ray particles with energy greater than lo2’ eV (Extreme High Energy Cosmic Rays -”EHECR”) [l]has opened a new perspective for Astrophysics showing the existence of either unexpected extremely powerful acceleration mechanisms (” bottom-up” ) or more fundamental phenomena of emission/creation closely related to the primordial structure of the Universe (”topdown”).

3) This GZK neutrinos are a guaranteed component expected at the extreme energies. To avoid to become "model dependent", no other neutrino sources will be 32 cosmogmic neutrino events msnogenictWnm3 flavoreve& (Max) Figure 3: Detected neutrinos from GZK origin as a function of the energy threshold for a detector with F O V = 60’ from 400km altitude. 5 = 2 . 5 Q F p 0 and larger diameter of the entrance pupill of the optical system. The upper min and Marc curves correspond t o the 3 flavor events, the lower niin and M m curves correspond t o the 1 flavor events.

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Quantum Probability and Applications, V: Proceedings of the Fourth Workshop, Held in Heidelberg, FRG, Sept. 26-30, 1988 by Luigi Accardi, Wilhelm v. Waldenfels


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