Cross sections of reactions produced by high energy neutrino beams

Author:

Cabibbo N.,Gatto R.

Publisher

Springer Science and Business Media LLC

Subject

Astronomy and Astrophysics,Nuclear and High Energy Physics,Atomic and Molecular Physics, and Optics

Reference8 articles.

1. We have learned that various physicists, namely Prof.Amaldi, Prof.Bernardini, Prof.Cocconi, Prof.Lederman, Prof.Lee, Prof.Preiswerk and perhaps many others are thinking at present on the possibility of such experiments.

2. C. L. Cowan, F. Reines, F. B. Harrison, H. W. Kruse andA. D. McGuire (Nature,178, 446 (1956)) gave a cross-section 6·10−44 for he reaction $$\bar v + p \to n + e^ + $$ . The experiment was possible because of the high intensity of neutrinos from a thermal neutron reactor.

3. There have already been theoretical discussions on the importance of weak interactions at high energies [see, for instance,D. I. Blokhinstev:On the Limits of applicability of Quantum Electrodynamics, F. 148, Joint Institute for Nuclear Research, (1958)].

4. R. Davis:Bull. Am. Phys. Soc.,1, 219 (1956); and byC. O. Meuhlhanse andS. Oleska:Phys. Rev.,105, 1333 (1957). Evidence against double β decay is discussed for instance byC. L. Cowan andF. Reines:Phys. Rev.,106, 825 (1957). The study of neutrino reactions will also offer a conclusive test of the hypothesis that the neutrino emitted with the electron is the same as that emitted with the muon.

5. A detailed discussion can be found inR. Gatto:Fortschr. d. Phys.,7, 147 (1959).

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1. Physics of Neutrinos;Physics and Astrophysics of Neutrinos;1994

2. Reaction cross section for solar flare neutrinos with Cl-37 and O-16 targets;The Astrophysical Journal;1989-02

3. Pure leptonic weak processes;La Rivista Del Nuovo Cimento Series 3;1984-07

4. Analysis of the antineutrino capture on protons;Physical Review D;1984-05-01

5. Lepton-Pair Production in a Nucleon Field;Annalen der Physik;1980

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